Pics of SBCs

.gitignore

@@ -1,18 +1,27 @@
+Cover.pdf
 SNOUG.pdf
 SNOUG-web.pdf
+tmp/
 *~
 .~lock.*.ods#
 .fuse_hidden*
 _minted-*
+*.acn
+*.acr
+*.alg
 *.aux
 *.bak
 *.bak0
 *.bbl
 *.bcf
 *.blg
+*.fits
 *.glg
+*.glg-abr
 *.glo
+*.glo-abr
 *.gls
+*.gls-abr
 *.glstex
 *.idx
 *.ilg

BUILD.md

@@ -41,6 +41,12 @@ Run the build script to make a PDF:
 make
 ```
 
+To just make a cover:
+
+```
+make cover
+```
+
 To clean:
 
 ```

Makefile

@@ -7,6 +7,10 @@ all:
 # ps2pdf breaks ToC and other internal links
 #	ps2pdf SNOUG.pdf SNOUG-web.pdf
 
+cover:
+	$(MAKE) -C src cover
+	mv src/Cover.pdf .
+
 clean:
 	rm -f *.pdf
 	$(MAKE) clean -C src

TODO.md

@@ -7,6 +7,5 @@
 * See also for acronyms, index, glossary.
 * Separate list of acronyms.
 * Using ps2pdf to resize PDF for web breaks internal links.
-* Some missing italics.
 * Content.
-* Tracking.
+* ntpdate -b 192.168.1.1

src/Abbreviations.bib

@@ -0,0 +1,43 @@
+% Encoding: UTF-8
+@dualabbreviation{V,
+  description = {Volt.},
+  short = {V},
+  long = {Volt}
+}
+
+@dualabbreviation{Hz,
+  description = {hertz.},
+  short = {Hz},
+  long = {hertz}
+}
+
+@dualabbreviation{kHz,
+  description = {kilohertz.},
+  short = {kHz},
+  long = {kilohertz}
+}
+
+@dualabbreviation{MHz,
+  description = {megahertz.},
+  short = {MHz},
+  long = {megahertz}
+}
+
+@dualabbreviation{GHz,
+  description = {gigahertz.},
+  short = {GHz},
+  long = {gigahertz}
+}
+
+@dualabbreviation{USSPACECOM,
+  description = {United States Space Command.},
+  short = {USSPACECOM},
+  long = {United States Space Command}
+}
+
+@dualabbreviation{SPACECOM,
+  description = {United States Space Command.},
+  short = {SPACECOM},
+  long = {United States Space Command}
+}
+

src/Acquire.tex

@@ -12,12 +12,12 @@
 \section{Overview of Operation}
 \label{sec:overview-operation}
 \index{operation}
-Below shows how to run a SatNOGS Optical  \gls{ground-station},
+Below shows how to run a \gls{SatNOGS-Optical} \gls{ground-station},
 after it has been set up and configured.
 
 \section{Setup with \texttt{stvid}}
 \label{sec:stvid-setup}
-\index{stvid}\index{acquire}
+\index{acquire}
 \index{virtualenv}
 Acquire data with \texttt{acquire.py} from \texttt{\gls{stvid}}.
 Enter \texttt{virtualenv}, if used:
@@ -28,7 +28,7 @@ source env/bin/activate
 \end{minted}
 
 Get the latest \glspl{TLE}:
-\index{TLE}
+
 
 \begin{minted}{sh}
 ./update_tle.py
@@ -41,18 +41,19 @@ Acquire live data from camera.
 cd stvid/
 ./acquire.py
 \end{minted}
+\index{acquire}
 
 \begin{sidewaysfigure}[p!]
 	\includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{stvid-acquire-0.png}
 	\caption{Satellite images acquired by stvid.}
 	\label{fig:stvid-acquire}
-	\index{stvid}\index{acquire}
+	\index{acquire}
 \end{sidewaysfigure}
 
 
 \section{\texttt{acquire.py} Output}
 \label{sec:acquire-output}
-\index{acquire}\index{stvid}
+\index{acquire}\index{configuration.ini}\index{FITS}
 
 Example output while running \texttt{acquire.py}.
 

src/Acronyms.bib

@@ -0,0 +1,540 @@
+% Encoding: UTF-8
+@dualacronym{NORAD-ID,
+  description = {is a sequential nine-digit number assigned by the \gls{USSPACECOM} in the order of launch or discovery to all artificial objects in the \glspl{orbit} of Earth and those that left Earth's \glspl{orbit}. Space Command shares the catalog via \url{space-track.org}, which is maintained by the 18th \gls{SDS}. NORAD ID is also known as a satellite catalog number.%
+	\footnote{\cite{enwiki:Satellite_Catalog_Number}}},
+  short = {NORAD ID},
+  long = {North American Aerospace Defense Catalog Number}
+}
+
+@dualacronym{USM,
+  description = {is a type of piezoelectric motor powered by the ultrasonic vibration of a component, the stator, placed against another component, the rotor or slider depending on the scheme of operation (rotation or linear translation). One common application of ultrasonic motors is in camera lenses where they are used to move lens elements as part of the auto-focus system.%
+	\footnote{\cite{enwiki:Ultrasonic_motor}}},
+  short = {USM},
+  long = {Ultrasonic Motor}
+}
+
+@dualacronym{OS,
+  description = {An operating system is system software that manages computer hardware, software resources, and provides common services for computer programs.%
+	\footnote{\cite{enwiki:Operating_system}}},
+  short = {OS},
+  long = {Operating System}
+}
+
+@dualacronym{INDI,
+  description = {Instrument Neutral Distributed Interface is a \gls{DCS} protocol to enable control, data acquisition and exchange among hardware devices and software front ends, emphasizing astronomical instrumentation.%
+	\footnote{\cite{enwiki:Instrument-Neutral-Distributed-Interface}}},
+  short = {INDI},
+  long = {Instrument Neutral Distributed Interface}
+}
+
+@dualacronym{DFSG,
+  description = {Debian Free Software Guidelines is a set of guidelines that the \gls{Debian} Project uses to determine whether a software license is a \gls{free-software} license, which in turn is used to determine whether a piece of software can be included in \gls{Debian}. The DFSG is part of the \gls{Debian} Social Contract.%
+	\footnote{\cite{enwiki:Debian-Free-Software-Guidelines}}},
+  short = {DFSG},
+  long = {Debian Free Software Guidelines}
+}
+
+@dualacronym{FITS,
+  description = {Flexible Image Transport System is an open standard defining a digital file format useful for storage, transmission and processing of data: formatted as multi-dimensional arrays (for example a 2D image), or tables. FITS is the most commonly used digital file format in astronomy. The FITS standard was designed specifically for astronomical data, and includes provisions such as describing photometric and spatial calibration information, together with image origin metadata.%
+	\footnote{\cite{Wiki22:fitswikipfreeencyc}}},
+  short = {FITS},
+  long = {Flexible Image Transport System}
+}
+
+@dualacronym{SDR,
+  description = {Software-defined radio is a radio communication system where components that have been traditionally implemented in analog hardware (e.g. mixers, filters, amplifiers, modulators/demodulators, detectors, etc.) are instead implemented by means of software on a \gls{PC} or \gls{embedded-system}. SDRs are used in \gls{SatNOGS} \glspl{ground-station}.%
+			\footnote{\cite{Wiki22:softwdefinradiowikipfreeencyc}}
+},
+  short = {SDR},
+  long = {Software-defined radio}
+}
+
+@dualacronym{LSF,
+  description = {Libre Space Foundation is a non-profit foundation registered since 2015 in Greece and the creators of the SatNOGS project.%
+			\footnote{\url{https://libre.space/about-us/}}
+},
+  short = {LSF},
+  long = {Libre Space Foundation}
+}
+
+@dualacronym{RF,
+  description = {Radio frequency is the oscillation rate of an alternating electric current or voltage or of a magnetic, electric or electromagnetic field or mechanical system in the frequency range from around 20 \gls{kHz} to around 300 \gls{GHz}. This is roughly between the upper limit of audio frequencies and the lower limit of infrared frequencies; these are the frequencies at which energy from an oscillating current can radiate off a conductor into space as radio waves.%
+			\footnote{\cite{Wiki22:radiofrequwikipfreeencyc}}
+},
+  short = {RF},
+  long = {Radio Frequency}
+}
+
+@dualacronym{VHF,
+  description = {Very High Frequency is the \gls{ITU} designation for the range of radio frequency electromagnetic waves (radio waves) from 30 to 300 \gls{MHz}, with corresponding wavelengths of ten meters to one meter. Frequencies immediately below VHF are denoted high frequency (HF), and the next higher frequencies are known as \gls{UHF}.%
+			\footnote{\cite{Wiki22:veryhighfrequwikipfreeencyc}}
+},
+  short = {VHF},
+  long = {Very High Frequency}
+}
+
+@dualacronym{UHF,
+  description = {Ultra High Frequency is the \gls{ITU} designation for radio frequencies in the range between 300 \gls{MHz} and 3 \gls{GHz}, also known as the decimetre band as the wavelengths range from one meter to one tenth of a meter (one decimeter). Lower frequency signals fall into the \gls{VHF} or lower bands.%
+			\footnote{\cite{Wiki22:ultrahighfrequwikipfreeencyc}}
+},
+  short = {UHF},
+  long = {Ultra High Frequency}
+}
+
+@dualacronym{ITU,
+  description = {The International Telecommunication Union is a specialized agency of the United Nations responsible for many matters related to information and communication technologies.%
+			\footnote{\cite{Wiki22:intertelecunionwikipfreeencyc}}
+},
+  short = {ITU},
+  long = {International Telecommunication Union}
+}
+
+@dualacronym{GNU,
+  description = {``GNU's Not Unix!'' is an extensive collection of \gls{free-software}, which can be used as an \gls{OS} or can be used in parts with other \glspl{OS}. The use of the completed GNU tools led to the family of operating systems popularly known as \gls{Linux}. Most of GNU is licensed under the GNU Project's own \gls{GPL}. GNU is also the project within which the \gls{free-software} concept originated.%
+			\footnote{\cite{Wiki22:gnuwikipfreeencyc}}
+},
+  short = {GNU},
+  long = {GNU's Not Unix!}
+}
+
+@dualacronym{GPL,
+  description = {GNU General Public License is a series of widely used \gls{free-software} licenses that guarantee end users the four freedoms to run, study, share, and modify the software. The license was the first copyleft for general use. Historically, the GPL license family has been one of the most popular software licenses in the \gls{FLOSS} software domain.%
+			\footnote{\cite{Wiki22:gnugenerpublilicenwikipfreeencyc}}
+},
+  short = {GPL},
+  long = {GNU General Public License}
+}
+
+@dualacronym{SGP,
+  description = {Simplified General Perturbations models apply to near earth objects with an orbital period of less than 225 minutes. Simplified \glspl{perturbation} models are a set of five mathematical models (SGP, SGP4, SDP4, SGP8 and SDP8) used to calculate orbital state vectors of \glspl{satellite} and space debris relative to the Earth-centered inertial coordinate system. This set of models is often referred to collectively as SGP4 due to the frequency of use of that model particularly with \gls{TLE} sets produced by \gls{NORAD} and \gls{NASA}. These models predict the effect of \glspl{perturbation} caused by the Earth's shape, drag, radiation, and gravitation effects from other bodies such as the sun and moon. See also: \gls{SDP}.%
+			\footnote{\cite{enwiki:Simplified_perturbations_models}}
+},
+  short = {SGP},
+  long = {Simplified General Perturbations}
+}
+
+@dualacronym{SDP,
+  description = {Simplified Deep Space Perturbations models apply to objects with an orbital period greater than 225 minutes, which corresponds to an altitude of 5,877.5 km, assuming a circular orbit. See also: \gls{SGP}.%
+			\footnote{\cite{enwiki:Simplified_perturbations_models}}
+},
+  short = {SDP},
+  long = {Simplified Deep Space Perturbations}
+}
+
+@dualacronym{NORAD,
+  description = {North American Aerospace Defense Command is a combined organization of the United States and Canada that provides aerospace warning, air sovereignty, and protection for Canada and the continental United States.%
+			\footnote{\cite{enwiki:NORAD}}
+},
+  short = {NORAD},
+  long = {North American Aerospace Defense Command}
+}
+
+@dualacronym{NASA,
+  description = {is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research.%
+			\footnote{\cite{enwiki:NASA}}
+},
+  short = {NASA},
+  long = {National Aeronautics and Space Administration}
+}
+
+@dualacronym{OSH,
+  description = {open-source hardware consists of physical artifacts of technology designed and offered by the open-design movement. Both \gls{FOSS} and open-source hardware are created by the open-source culture movement and apply a like concept to a variety of components. It is sometimes, thus, referred to as \gls{FOSH}. The term usually means that information about the hardware is easily discerned so that others can make it---coupling it closely to the maker movement. Hardware design (i.e. mechanical drawings, schematics, bills of material, \gls{PCB} layout data, \gls{HDL} source code and integrated circuit layout data), in addition to the software that drives the hardware, are all released under free/\gls{libre} terms. The original sharer gains feedback and potentially improvements on the design from the \gls{FOSH} community. There is now significant evidence that such sharing can drive a high return on investment for the scientific community. It is not enough to merely use an \gls{open-source} license; an \gls{open-source} product or project will follow \gls{open-source} principles, such as modular design and community collaboration.%
+			\footnote{\cite{enwiki:Open-source-hardware}}
+},
+  short = {OSH},
+  long = {Open Source Hardware}
+}
+
+@dualacronym{FOSS,
+  description = {free and \gls{open-source} software is a term used to refer to groups of software consisting of both \gls{free-software} and \gls{OSS} where anyone is freely licensed to use, copy, study, and change the software in any way, and the source code is openly shared so that people are encouraged to voluntarily improve the design of the software. This is in contrast to proprietary software, where the software is under restrictive copyright licensing and the source code is usually hidden from the users. FOSS maintains the software user's civil liberty rights. Other benefits of using FOSS can include decreased software costs, increased security and stability (especially in regard to malware), protecting privacy, education, and giving users more control over their own hardware. Free and open-source operating systems such as \gls{Linux} and descendants of \gls{BSD} are widely utilized today, powering millions of servers, desktops, smartphones (e.g., Android), and other devices. Free-software licenses and \gls{open-source} licenses are used by many software packages. The free software movement and the \gls{open-source} software movement are online social movements behind widespread production and adoption of FOSS, with the former preferring to use the terms \gls{FLOSS} or free/\gls{libre}.%
+			\footnote{\cite{enwiki:Free-and-open-source-software}}
+},
+  short = {FOSS},
+  long = {Free and Open Source Software}
+}
+
+@dualacronym{OSS,
+  description = {open-source software is computer software that is released under a license in which the copyright holder grants users the rights to use, study, change, and distribute the software and its source code to anyone and for any purpose. Open-source software may be developed in a collaborative public manner. Open-source software is a prominent example of open collaboration, meaning any capable user is able to participate online in development, making the number of possible contributors indefinite. The ability to examine the code facilitates public trust in the software. Open source code can be used for studying and allows capable end users to adapt software to their personal needs in a similar way user scripts and custom style sheets allow for web sites, and eventually publish the modification as a fork for users with similar preference.%
+			\footnote{\cite{enwiki:Open-source-software}}
+},
+  short = {OSS},
+  long = {Open Source Software}
+}
+
+@dualacronym{IP,
+  longplural = {Internet Protocol Addresses},
+  description = {Internet Protocol Address.},
+  short = {IP},
+  long = {Internet Protocol Address}
+}
+
+@dualacronym{DSLR,
+  description = {digital single-lens reflex.},
+  short = {DSLR},
+  long = {Digital Single Lens Reflex}
+}
+
+@dualacronym{PoE,
+  description = {Power over Ethernet.},
+  short = {PoE},
+  long = {Power over Ethernet}
+}
+
+@dualacronym{GNSS,
+  description = {Global Navigation \Gls{satellite} System.},
+  short = {GNSS},
+  long = {Global Navigation Satellite System}
+}
+
+@dualacronym{GPS,
+  description = {Global Positioning System.},
+  short = {GPS},
+  long = {Global Positioning System}
+}
+
+@dualacronym{IP67,
+  description = {Ingress Protection code 67.},
+  short = {IP67},
+  long = {Ingress Protection code 67}
+}
+
+@dualacronym{SSA,
+  description = {Space Situational Awareness.},
+  short = {SSA},
+  long = {Space Situational Awareness}
+}
+
+@dualacronym{WCS,
+  description = {World Coordinate System.},
+  short = {WCS},
+  long = {World Coordinate System}
+}
+
+@dualacronym{CMOS,
+  description = {Complementary metal-oxide-semiconductor (pronounced ``see-moss'').},
+  short = {CMOS},
+  long = {Complementary Metal Oxide Semiconductor}
+}
+
+@dualacronym{CCD,
+  description = {charge-coupled device.},
+  short = {CCD},
+  long = {Charge Coupled Device}
+}
+
+@dualacronym{SIDLOC,
+  description = {Spacecraft Identification and Localization.},
+  short = {SIDLOC},
+  long = {Spacecraft Identification and Localization}
+}
+
+@dualacronym{RASA,
+  description = {Rowe-Ackermann Schmidt \Gls{astrograph}.},
+  short = {RASA},
+  long = {Rowe-Ackermann Schmidt Astrograph}
+}
+
+@dualacronym{COTS,
+  description = {Commodity off the shelf.},
+  short = {COTS},
+  long = {Commodity Off The Shelf}
+}
+
+@dualacronym{FOSH,
+  description = {Free open-source hardware. See also: \gls{OSH}.},
+  short = {FOSH},
+  long = {Free Open Source Hardware}
+}
+
+@dualacronym{FLOSS,
+  description = {Free/libre and open-source software. See also: \gls{FOSS}.},
+  short = {FLOSS},
+  long = {Free/Libre and Open Source Software}
+}
+
+@dualacronym{SIP,
+  description = {Simple Imaging Polynomial.},
+  short = {SIP},
+  long = {Simple Imaging Polynomial}
+}
+
+@dualacronym{FoV,
+  description = {Field of view.},
+  short = {FoV},
+  long = {Field of View}
+}
+
+@dualacronym{DCS,
+  description = {distributed control system.},
+  short = {DCS},
+  long = {Distributed Control System}
+}
+
+@dualacronym{PNG,
+  description = {Portable Network Graphics.},
+  short = {PNG},
+  long = {Portable Network Graphics}
+}
+
+@dualacronym{CSV,
+  description = {Comma Separated Value.},
+  short = {CSV},
+  long = {Comma Separated Value}
+}
+
+@dualacronym{NTP,
+  description = {Network Time Protocol.},
+  short = {NTP},
+  long = {Network Time Protocol}
+}
+
+@dualacronym{IPv6,
+  description = {Internet Protocol version 6.},
+  short = {IPv6},
+  long = {Internet Protocol version 6}
+}
+
+@dualacronym{ISS,
+  description = {International Space Station.},
+  short = {ISS},
+  long = {International Space Station}
+}
+
+@dualacronym{LEO,
+  description = {Low Earth Orbit.},
+  short = {LEO},
+  long = {Low Earth Orbit}
+}
+
+@dualacronym{GEO,
+  description = {Geostationary orbit.},
+  short = {GEO},
+  long = {Geostationary Orbit}
+}
+
+@dualacronym{HEO,
+  description = {High Earth orbit.},
+  short = {HEO},
+  long = {High Earth Orbit}
+}
+
+@dualacronym{MEO,
+  description = {Medium Earth orbit.},
+  short = {MEO},
+  long = {Medium Earth Orbit}
+}
+
+@dualacronym{GSO,
+  description = {Geosynchronous orbit.},
+  short = {GSO},
+  long = {Geosynchronous Orbit}
+}
+
+@dualacronym{PCB,
+  description = {Printed circuit board.},
+  short = {PCB},
+  long = {Printed Circuit Board}
+}
+
+@dualacronym{HDL,
+  description = {Hardware description language.},
+  short = {HDL},
+  long = {Hardware Description Language}
+}
+
+@dualacronym{V4L2,
+  description = {Video for Linux v2.},
+  short = {V4L2},
+  long = {Video for Linux v2}
+}
+
+@dualacronym{BSD,
+description = {Berkeley Software Distribution.},
+  short = {BSD},
+  long = {Berkeley Software Distribution}
+}
+
+@dualacronym{SDK,
+  description = {Software development kit.},
+  short = {SDK},
+  long = {Software Development Kit}
+}
+
+@dualacronym{MIPI,
+  description = {Mobile Industry Processor Interface.},
+  short = {MIPI},
+  long = {Mobile Industry Processor Interface}
+}
+
+@dualacronym{ASM,
+  description = {All Sky Monitor.},
+  short = {ASM},
+  long = {All Sky Monitor}
+}
+
+@dualacronym{PTZ,
+  description = {Pan-tilt-zoom.},
+  short = {PTZ},
+  long = {Pan Tilt Zoom}
+}
+
+@dualacronym{PPS,
+  description = {Pulse per second.},
+  short = {PPS},
+  long = {Pulse Per Second}
+}
+
+@dualacronym{USB,
+  description = {Universal Serial Bus.},
+  short = {USB},
+  long = {Universal Serial Bus}
+}
+
+@dualacronym{NUC,
+  description = {Next Unit of Computing.},
+  short = {NUC},
+  long = {Next Unit of Computing}
+}
+
+@dualacronym{DC,
+  description = {Direct current.},
+  short = {DC},
+  long = {Direct Current}
+}
+
+@dualacronym{EQ,
+  description = {Equatorial.},
+  short = {EQ},
+  long = {Equatorial}
+}
+
+@dualacronym{IDK,
+  description = {I don't know.},
+  short = {IDK},
+  long = {I Don't Know}
+}
+
+@dualacronym{DB,
+  description = {Database.},
+  short = {DB},
+  long = {Database}
+}
+
+@dualacronym{UVC,
+  description = {USB video device class.},
+  short = {UVC},
+  long = {USB Video device Class}
+}
+
+@dualacronym{CV,
+  description = {Computer vision.},
+  short = {CV},
+  long = {Computer Vision}
+}
+
+@dualacronym{PIP,
+  description = {Package Installer for Python.},
+  short = {PIP},
+  long = {Package Installer for Python}
+}
+
+@dualacronym{RAM,
+  description = {Random-access memory.},
+  short = {RAM},
+  long = {Random Access Memory}
+}
+
+@dualacronym{GLONASS,
+  description = {Global Navigation Satellite System.},
+  short = {GLONASS},
+  long = {Global Navigation Satellite System}
+}
+
+@dualacronym{BDS,
+  description = {BeiDou Navigation Satellite System.},
+  short = {BDS},
+  long = {BeiDou Navigation Satellite System}
+}
+
+@dualacronym{SBC,
+  description = {Single board computer.},
+  short = {SBC},
+  long = {Single Board Computer}
+}
+
+@dualacronym{BIOS,
+  description = {Basic Input/Output System.},
+  short = {BIOS},
+  long = {Basic Input/Output System}
+}
+
+@dualacronym{OSAT,
+  description = {open-source appropriate technology.},
+  short = {OSAT},
+  long = {Open Source Appropriate Technology}
+}
+
+@dualacronym{PC,
+  description = {Personal Computer.},
+  short = {PC},
+  long = {Personal Computer}
+}
+
+@dualacronym{CGPM,
+  description = {General Conference on Weights and Measures.},
+  short = {CGPM},
+  long = {General Conference on Weights and Measures}
+}
+
+@dualacronym{API,
+  description = {application programming interface.},
+  short = {API},
+  long = {Application Programming Interface}
+}
+
+@dualacronym{CPU,
+  description = {central processing unit.},
+  short = {CPU},
+  long = {Central Processing Unit}
+}
+
+@dualacronym{NGC,
+  description = {New General Catalogue of Nebulae and Clusters of Stars.},
+  short = {NGC},
+  long = {New General Catalogue of Nebulae and Clusters of Stars}
+}
+
+@dualacronym{FLIR,
+  description = {Forward-looking infrared.},
+  short = {FLIR},
+  long = {Forward Looking Infrared}
+}
+
+@dualacronym{SDS,
+  description = {Space Defense Squadron.},
+  short = {SDS},
+  long = {Space Defense Squadron}
+}
+
+@dualacronym{PaaS,
+  description = {Platform as a Service.},
+  short = {PaaS},
+  long = {Platform as a Service}
+}
+
+@dualacronym{SI,
+  description = {The International System of Units, known by the international abbreviation SI in all languages and sometimes pleonastically as the SI system, is the modern form of the metric system and the world's most widely used system of measurement. Established and maintained by the \gls{CGPM}, it is the only system of measurement with an official status in nearly every country in the world, employed in science, technology, industry, and everyday commerce.%
+			\footnote{\cite{Wiki22:intersysteunitswikipfreeencyc}}
+},
+  short = {SI},
+  long = {International System of Units}
+}
+
+@dualacronym{TLE,
+  description = {two-line element set is a data format encoding a list of orbital elements of an Earth-orbiting object for a given point in time, the epoch. Using a suitable prediction formula, the state (position and velocity) at any point in the past or future can be estimated to some accuracy. TLEs can describe the trajectories only of Earth-orbiting objects. TLEs are widely used as input for projecting the future orbital tracks of space debris for purposes of characterizing ``future debris events to support risk analysis, close approach analysis, collision avoidance maneuvering'' and forensic analysis. The format was originally intended for punched cards, encoding a set of elements on two standard 80-column cards.%
+			\footnote{\cite{Wiki22:twolineelemesetwikipfreeencyc}}
+},
+  short = {TLE},
+  long = {Two Line Element set}
+}
+

src/Cover.tex

@@ -0,0 +1,121 @@
+\documentclass{book}
+\usepackage[utf8x]{inputenc}
+\usepackage{rotating}
+\usepackage{fontspec}
+\defaultfontfeatures{Ligatures=TeX}
+\graphicspath{{./figures/}}
+
+% Crown Quarto
+\usepackage[papersize={24.58cm,18.90cm},topmargin=5mm,
+    botmargin,strictheight,
+    textwidth=14.2cm,textheight=18.6cm,
+    leftmargin=0cm,spine=1.7cm,
+    rightmargin=2cm,
+    cropmarks,croptitle=Cover]{zwpagelayout}
+
+%\usepackage{graphics,color}
+%\usepackage[SC0,ISBN=999-99-9999-999-4]{ean13isbn}
+%\usepackage[LY1]{fontenc}
+%\pagestyle{empty}
+%\parindent 0mm
+%\def\thePageNumber{Brodie}
+
+\def\moe{\rotatebox{33.0}{\upshape \kern-.5em \hbox{M}}%
+	\rotatebox{20.0}{\scshape\kern-.425em\lower-.4ex\hbox{o}}
+	}
+
+\begin{document}
+
+\newsavebox{\mysquare}
+%  39  173  207   .15  .68  .81
+% 255  255  255   100  100  100
+\definecolor{brodieblue}{rgb}{0.15,0.68,.81}
+
+\pagecolor{white}
+
+\small
+\hbox to \textwidth{%
+
+%%% BACK FLAP %%%
+\hss
+%  \vbox to \textheight{\hsize \CropFlap \centering
+%        backflap\vfill}\hss
+%%% END BACK FLAP %%%
+
+%%% BACK COVER %%%
+  \vbox to \textheight{\hsize \UserWidth \centering
+        \vfill
+	\vspace*{85pt}
+	\leavevmode }\hss
+%        ISBNbackcover\vfill \leavevmode \EANisbn}\hss
+%%% END BACK COVER %%%
+
+%%% SPINE %%%
+	\colorbox{white}{
+	\vbox to \textheight{\hsize \CropSpine \centering
+        \vfill
+        \begin{sideways}
+	\rotatebox{180}{
+	\includegraphics[keepaspectratio=true,angle=0,height=0.02\textheight,width=0.02\textwidth]{spacecruft.png}
+	\hspace*{20pt}
+	\large\itshape\textcolor{black}{}
+	\fontspec{GemunuLibre-ExtraBold.otf}\fontsize{14pt}{1em}\selectfont
+	SatNOGS Optical Unofficial Guide
+	\hspace*{20pt}
+	\includegraphics[keepaspectratio=true,angle=0,height=0.02\textheight,width=0.02\textwidth]{spacecruft.png}
+	\large\itshape\textcolor{black}{}
+	\hspace*{20pt}
+	\fontspec{GemunuLibre-ExtraBold.otf}\fontsize{12pt}{1em}\selectfont
+	Jeff Moe
+	\hspace*{15pt}
+	\includegraphics[keepaspectratio=true,angle=0,height=0.02\textheight,width=0.02\textwidth]{spacecruft.png}
+	}
+	\end{sideways}\vfill}\hss
+	}
+%%% END SPINE %%%
+
+%%% FRONT COVER %%%
+\fcolorbox{white}{brodieblue}{
+\vbox to \textheight{\hsize \UserWidth \centering
+\begingroup
+\vspace*{60pt}
+        \fontspec{GemunuLibre-ExtraBold.otf}\fontsize{40pt}{1em}\selectfont %
+        SatNOGS Optical \\
+        \fontspec{LinLibertine_RI.otf}\fontsize{16pt}{0em}\selectfont %
+        \emph{\textcolor{white}{\begin{turn}{15}Unofficial\end{turn}}} \\
+        \fontspec{GemunuLibre-ExtraBold.otf}\fontsize{68pt}{1em}\selectfont %
+        Guide\\
+
+\vfill
+
+\begin{center}
+        \null\vfill
+        \centering
+        \includegraphics[keepaspectratio=true,angle=0,height=0.40\textheight,width=0.40\textwidth]{frontispiece.png}
+        \par
+	\null
+	\par
+        \includegraphics[keepaspectratio=true,angle=0,height=0.02\textheight,width=0.02\textwidth]{spacecruft.png}
+        \includegraphics[keepaspectratio=true,angle=0,height=0.02\textheight,width=0.02\textwidth]{spacecruft.png}
+        \includegraphics[keepaspectratio=true,angle=0,height=0.02\textheight,width=0.02\textwidth]{spacecruft.png}
+        \par
+\end{center}
+
+
+\color{white}\rule{120pt}{2.0pt}\\[\baselineskip]
+\endgroup
+\vspace*{10pt}
+\fontspec{GemunuLibre-ExtraBold.otf}\fontsize{14pt}{1em}\selectfont %
+{Jeff Moe}
+\vspace*{55pt}
+}
+}
+%%% END FRONT COVER
+
+%%% FRONT FLAP %%%
+\hss
+%  \vbox to \textheight{\hsize \CropFlap \centering
+%        frontflap\vfill}}
+%%% END FRONT FLAP %%%
+}
+\end{document}

src/Detect.tex

@@ -11,23 +11,22 @@
 
 \section{Satellite Detection with stvid}
 \label{sec:satellite-detection}
-\index{detection}\index{stvid}\index{process}\index{Python}
-\index{FITS}
+\index{detect}\index{process}
 
 This is a description of \gls{satellite} detection processes.
-To detect \gls{satellite} in a \gls{FITS} file using the stvid toolchain,
+To detect \gls{satellite} in a \gls{FITS} file using the \gls{stvid} \gls{toolchain},
 run \texttt{process.py} or, if it exists, the \texttt{process\_new.py}
-Python script.
+\gls{Python} script.
 
 Note the \texttt{stvid} application's \texttt{process.py} and \texttt{process\_new.py}
 will perform both the detection and identification steps.
-\index{identify}
+\index{identify}\index{detect}
 
 \subsection{\texttt{process\_new.py} Usage}
 \index{process}
 
-This assumes you have installed \texttt{stvid} as shown in section \ref{sec:stvid-setup}
-\pageref{sec:stvid-setup}.
+This assumes you have installed \texttt{\gls{stvid}} as shown in
+section \ref{sec:stvid-setup}, page \pageref{sec:stvid-setup}.
 Adjust the dated directory used in this example to the actual directory name.
 
 \begin{minted}{sh}
@@ -37,8 +36,10 @@ cd stvid/
 # Process directory
 ./process_new.py -c config_new.ini -d data/obs/20220825_1/020502/
 \end{minted}
+\index{process}\index{TLE}\index{config\_new.ini}
 
 \subsection{\texttt{process.py} Usage}
+
 If there is no \texttt{process\_new.py} it has likely been merged into
 \texttt{process.py}. Or perhaps, to use the ``older'' script it would
 be run as shown below. Note, the old and new configuration files
@@ -49,12 +50,12 @@ script.
 cd stvid/
 ./process.py -c configuration.ini -d data/obs/20220825_1/020502/
 \end{minted}
-\index{stvid}\index{process}
+\index{process}\index{configuration.ini}
 
 
-\section{\texttt{process\_new.py Example Output}}
+\subsection{\texttt{process\_new.py Example Output}}
 \label{sec:process-output}
-\index{stvid}\index{FITS}
+\index{process}\index{config\_new.ini}
 
 \begin{minted}{sh}
 Computing astrometric calibration for /srv/obs/odroid-01/obs/20220902_1/043309/2022-09-02T04:33:09.871.fits
@@ -67,11 +68,12 @@ File queue empty, waiting for new files...
 90000 22 500A   9999 G 20220902043336020 17 25 1433368+375908 37 S
 2022-09-02T04:33:40.315.fits 216.815570  31.756676  206/ 342  10.1  13.1  16.54 +-   0.70
 \end{minted}
+\index{astometry.net}\index{process}
 
 
 \section{AstroImageJ}
 \label{sec:astroimagej}
-\index{identify}\index{AstroImageJ}\index{FITS}
+\index{identify}
 
 Analyze data with applications, such as \gls{AstroImageJ}.
 
@@ -82,13 +84,11 @@ See
 \ref{fig:astroimagej}, page \pageref{fig:astroimagej},
 for a screenshot displaying a \gls{FITS} file generated by
 \texttt{\gls{stvid}}.
-\index{stvid}
 
 \begin{sidewaysfigure}[p!]
 	\begin{center}
 		\includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{astroimagej.png}
 		\caption{AstroImageJ screenshot viewing FITS file.}
-		\index{AstroImageJ}\index{FITS}
 		\label{fig:astroimagej}
 	\end{center}
 \end{sidewaysfigure}

src/Glossary.bib

@@ -0,0 +1,508 @@
+% Encoding: UTF-8
+@entry{artificial-satellite,
+  name = {artificial satellite},
+  long = {artificial satellite},
+  description = {is a \gls{satellite} put into \gls{orbit} by humans, not ``naturally'' occurring.}
+}
+
+@entry{libre-software,
+  name = {libre software},
+  long = {libre software},
+  description = {See: \gls{free-software}.}
+}
+
+@entry{AstroImageJ,
+  name = {AstroImageJ},
+  long = {AstroImageJ},
+  description = {Application for astronomy and \gls{satellite} image analysis.%
+			\footnote{\url{https://www.astro.louisville.edu/software/astroimagej/}}
+}
+}
+
+@entry{skymap,
+  name = {skymap},
+  long = {skymap},
+  description = {is part of \gls{sattools}. Visualize \glspl{satellite} on a map of the sky.%
+			\footnote{\url{https://github.com/cbassa/sattools/blob/master/skymap.c}}
+}
+}
+
+@entry{satid,
+  name = {satid},
+  long = {satid},
+  description = {is part of \gls{sattools}.%
+			\footnote{\url{https://github.com/cbassa/sattools/blob/master/satid.c}}
+}
+}
+
+@entry{sattools,
+  name = {sattools},
+  long = {sattools},
+  description = {Satellite Tracking Toolkit. The main \texttt{sattools} applications are being ported to \gls{stvid} and other related \gls{Python} applications.%
+			\footnote{\url{https://github.com/cbassa/sattools}}
+}
+}
+
+@entry{satpredict,
+  name = {satpredict},
+  long = {satpredict},
+  description = {is a software application to compute \gls{satellite} predictions. It is used by \gls{stvid}.%
+			\footnote{\url{https://github.com/cbassa/satpredict}}
+}
+}
+
+@entry{stvid,
+  name = {stvid},
+  long = {stvid},
+  description = {\Gls{satellite} tools video application for acquiring and processing sky images.%
+			\footnote{\url{https://github.com/cbassa/stvid}}
+}
+}
+
+@entry{hough3d-code,
+  name = {hough3d-code},
+  long = {hough3d-code},
+  description = {is a software application for Iterative Hough Transform for Line Detection in 3D Point Clouds.%
+			\footnote{\url{https://gitlab.com/pierros/hough3d-code}}
+}
+}
+
+@entry{ground-station,
+  name = {ground station},
+  long = {ground station},
+  description = {a setup of equipment such as computers, cameras, \glspl{SDR}, antennas, and receivers, located on Earth, observing space.
+}
+}
+
+@entry{SatNOGS-Optical,
+  name = {SatNOGS Optical},
+  long = {SatNOGS Optical},
+  description = {is a project by the \gls{LSF} to add optical ground stations to the SatNOGS network.%
+			\footnote{\url{https://satnogs.org/}}
+}
+}
+
+@entry{SatNOGS-DB,
+  name = {SatNOGS DB},
+  long = {SatNOGS DB},
+  description = {is an effort to create an hollistic, unified, global database for all artificial objects in space (\glspl{satellite} and spacecrafts). Users can view and export the data, contribute to it, or connect applications using an \gls{API}. It is part of the \gls{SatNOGS} project.%
+			\footnote{\url{https://db.satnogs.org/}}
+}
+}
+
+@entry{SatNOGS,
+  name = {SatNOGS},
+  long = {SatNOGS},
+  description = {Open Source global network of \gls{satellite} ground stations.%
+			\footnote{\url{https://satnogs.org/}}
+}
+}
+
+@entry{optical-ground-station,
+  name = {optical ground station},
+  long = {optical ground station},
+  description = {a ground station using optical equipment (cameras) instead of antennas.
+}
+}
+
+@entry{antenna,
+  name = {antenna},
+  long = {antenna},
+  description = {the interface between radio waves propagating through space and electric currents moving in metal conductors, used with a transmitter or receiver.%
+			\footnote{\cite{Wiki22:antenradiowikipfreeencyc}}
+}
+}
+
+@entry{mast,
+  name = {mast},
+  long = {mast},
+  description = {typically tall structures designed to support antennas for telecommunications and broadcasting.%
+			\footnote{\cite{Wiki22:radiomaststowerwikipfreeencyc}}
+}
+}
+
+@entry{rotator,
+  name = {rotator},
+  long = {rotator},
+  description = {a device used to change the orientation, within the horizontal plane, of a directional antenna. Most antenna rotators have two parts, the rotator unit and the controller. The controller is normally placed near the equipment which the antenna is connected to, while the rotator is mounted on the antenna mast directly below the antenna. Rotators are commonly used in amateur radio.%
+			\footnote{\cite{Wiki22:antenrotatwikipfreeencyc}}
+}
+}
+
+@entry{Debian,
+  name = {Debian},
+  long = {Debian},
+  description = {a \gls{GNU}/\gls{Linux} distribution composed of free and open-source software, developed by the community-supported Debian Project, which was established by Ian Murdock on August 16, 1993. Debian is the basis for many other distributions, notably Ubuntu.
+			Debian is one of the oldest operating systems based on the Linux kernel.%
+			\footnote{\cite{Wiki22:debiawikipfreeencyc}}
+}
+}
+
+@entry{Linux,
+  name = {Linux},
+  long = {Linux},
+  description = {is a free and open-source, monolithic, modular, multitasking, \gls{Unix}-like operating system kernel. It was originally authored in 1991 by Linus Torvalds for his i386-based \gls{PC}, and it was soon adopted as the kernel for the \gls{GNU} \gls{OS}, which was written to be a free (\gls{libre}) replacement for \gls{Unix}.%
+			\footnote{\cite{Wiki22:linuxkernewikipfreeencyc}}
+}
+}
+
+@entry{open-source,
+  name = {Open Source},
+  long = {Open Source},
+  description = {is source code that is made freely available for possible modification and redistribution. Products include permission to use the source code, design documents, or content of the product. The open-source model is a decentralized software development model that encourages open collaboration. A main principle of open-source software development is peer production, with products such as source code, blueprints, and documentation freely available to the public. The open-source movement in software began as a response to the limitations of proprietary code. The model is used for projects such as in open-source \gls{appropriate-technology}.%
+			\footnote{\cite{Wiki22:opensourcwikipfreeencyc}}
+}
+}
+
+@entry{free-software,
+  name = {Free Software},
+  long = {Free Software},
+  description = {or \gls{libre} software, is computer software distributed under terms that allow users to run the software for any purpose as well as to study, change, and distribute it and any adapted versions. Free software is a matter of liberty, not price; all users are legally free to do what they want with their copies of a free software (including profiting from them) regardless of how much is paid to obtain the program. Computer programs are deemed ``free'' if they give end-users (not just the developer) ultimate control over the software and, subsequently, over their devices.%
+			\footnote{\cite{Wiki22:freesoftwwikipfreeencyc}}
+}
+}
+
+@entry{Matrix,
+  name = {Matrix},
+  long = {Matrix},
+  description = {an open standard and communication protocol for real-time communication.%
+			\footnote{\cite{Wiki22:matriprotowikipfreeencyc}}
+}
+}
+
+@entry{telescope,
+  name = {telescope},
+  long = {telescope},
+  description = {is an optical instrument using lenses, curved mirrors, or a combination of both to observe distant objects, or various devices used to observe distant objects by their emission, absorption, or reflection of electromagnetic radiation. The word telescope now refers to a wide range of instruments capable of detecting different regions of the electromagnetic spectrum, and in some cases other types of detectors.%
+			\footnote{\cite{enwiki:Telescope}}
+}
+}
+
+@entry{astrograph,
+  name = {astrograph},
+  long = {astrograph},
+  description = {is a telescope designed for the sole purpose of astrophotography. Astrographs are mostly used in wide-field astronomical surveys of the sky and for detection of objects such as asteroids, meteors, and comets.%
+			\footnote{\cite{enwiki:Astrograph}}
+}
+}
+
+@entry{satellite,
+  name = {satellite},
+  long = {satellite},
+  description = {is an object intentionally placed into \gls{orbit} in outer space. Except for passive satellites, most satellites have an electricity generation system for equipment on board. Most satellites also have a method of communication to ground stations, called transponders. Many satellites use a standardized bus to save cost and work, the most popular of which is small \Glspl{cubesat}. Similar satellites can work together as a group, forming constellations.%
+			\footnote{\cite{enwiki:Satellite}}
+}
+}
+
+@entry{cubesat,
+  name = {CubeSat},
+  long = {CubeSat},
+  description = {is a class of miniaturized \gls{satellite} based around a form factor consisting of 10 cm (3.9 in) cubes. CubeSats have a mass of no more than 2 kg per unit, and often use \gls{COTS} components for their electronics and structure. CubeSats are put into \gls{orbit} by deployers on the \gls{ISS}, or launched as secondary payloads on a launch vehicle. More than a thousand CubeSats have been launched.%
+			\footnote{\cite{enwiki:CubeSat}}
+}
+}
+
+@entry{orbit,
+  name = {orbit},
+  long = {orbit},
+  description = {is the curved trajectory of an object such as the trajectory of a planet around a star, or of a natural satellite around a planet, or of an artificial satellite around an object or position in space such as a planet, moon, asteroid, or \gls{Lagrange-point}. Normally, orbit refers to a regularly repeating trajectory, although it may also refer to a non-repeating trajectory. To a close approximation, planets and \glspl{satellite} follow elliptic orbits, with the center of mass being orbited at a focal point of the ellipse, as described by Kepler's laws of planetary motion. For most situations, orbital motion is adequately approximated by Newtonian mechanics, which explains gravity as a force obeying an inverse-square law. However, Albert Einstein's general theory of relativity, which accounts for gravity as due to curvature of spacetime, with orbits following geodesics, provides a more accurate calculation and understanding of the exact mechanics of orbital motion.%
+			\footnote{\cite{enwiki:Orbit}}
+}
+}
+
+@entry{perturbation,
+  name = {perturbation},
+  long = {perturbation},
+  description = {is the complex motion of a massive body subjected to forces other than the gravitational attraction of a single other massive body. The other forces can include a third (fourth, fifth, etc.) body, resistance, as from an atmosphere, and the off-center attraction of an oblate or otherwise misshapen body.%
+			\footnote{\cite{enwiki:Perturbation-astronomy}}
+}
+}
+
+@entry{telemetry,
+  name = {telemetry},
+  long = {telemetry},
+  description = {is the in situ collection of measurements or other data at remote points and their automatic transmission to receiving equipment (telecommunication) for monitoring. The word is derived from the Greek roots tele, ``remote'', and metron, ``measure''. Although the term commonly refers to wireless data transfer mechanisms (e.g., using radio, ultrasonic, or infrared systems), it also encompasses data transferred over other media such as a telephone or computer network, optical link or other wired communications like power line carriers.%
+			\footnote{\cite{enwiki:Telemetry}}
+}
+}
+
+@entry{Grafana,
+  name = {Grafana},
+  long = {Grafana},
+  description = {is a multi-platform \gls{open-source} analytics and interactive visualization web application. It provides charts, graphs, and alerts for the web when connected to supported data sources. Users can create complex monitoring dashboards using interactive query builders. It is used by the \gls{SatNOGS} project to visualize \gls{satellite} \gls{telemetry}.%
+			\footnote{\cite{enwiki:Grafana}}
+}
+}
+
+@entry{Python,
+  name = {Python},
+  long = {Python},
+  description = {is a high-level, interpreted, general-purpose programming language. Its design philosophy emphasizes code readability. It is often described as a ``batteries included'' language due to its comprehensive standard library. Python consistently ranks as one of the most popular programming languages. It is one of the main languages of the \gls{SatNOGS} project and \gls{stvid}.%
+			\footnote{\cite{enwiki:Python-language}}
+}
+}
+
+@entry{C,
+  name = {C},
+  long = {C},
+  description = {is a general-purpose computer programming language. It was created in the 1970s by Dennis Ritchie, and remains very widely used and influential. By design, C's features cleanly reflect the capabilities of the targeted \glspl{CPU}. It has found lasting use in \glspl{OS}, device drivers, protocol stacks, though decreasingly for application software. C is commonly used on computer architectures that range from the largest supercomputers to the smallest microcontrollers and \glspl{embedded-system}. C is used in the \gls{sattools} suite of applications.%
+			\footnote{\cite{enwiki:C-language}}
+}
+}
+
+@entry{libre,
+  name = {libre},
+  long = {libre},
+  description = {The English adjective free is commonly used in one of two meanings: ``at no monetary cost'' (gratis) and ``with little or no restriction'' (libre). This ambiguity of free can cause issues where the distinction is important, as it often is in dealing with laws concerning the use of information, such as copyright and patents. The terms gratis and libre may be used to categorise computer programs, according to the licenses and legal restrictions that cover them, in the \gls{free-software} and \gls{open-source} communities, as well as the broader free culture movement. For example, they are used to distinguish freeware (software gratis) from \gls{free-software} (software libre). ``Think free as in free speech, not free beer.'' -- Richard Stallman.%
+			\footnote{\cite{enwiki:Gratis-versus-libre}}
+}
+}
+
+@entry{plate-solver,
+  name = {plate solver},
+  long = {plate solver},
+  description = {is software implementing a technique used in astronomy and applied on celestial images. Solving an image is finding match between the imaged stars and a \gls{star-catalogue}. The solution is a math model describing the corresponding astronomical position of each image pixel. The position of reference catalogue stars has to be known to a high accuracy so an astrometric reference catalogue is used. The image solution contains a reference point, often the image centre, image scale, image orientation and in some cases an image distortion model. With the astrometric solution it is possible to: 1) Calculate the celestial coordinates of any object on the image. 2) Synchronize the telescope mount or satellite pointing position to the center of the image taken. Astrometric solving programs extract the star x,y positions from the celestial image, groups them in three-star triangles or four-star quads. Then it calculates for each group a geometric hash code based on the distance and/or angles between the stars in the group. It then compares the resulting hash codes with the hash codes created from catalogue stars to find a match. If it finds sufficient statistically reliable matches, it can calculate transformation factors. There are several conventions to model the transformation from image pixel location to the corresponding celestial coordinates. The simplest linear model is called the \gls{WCS}. A more advanced convention is \gls{SIP} describing the transformation in polynomials to cope with non-linear geometric distortion in the celestial image, mainly caused by the optics.%
+			\footnote{\cite{enwiki:Astrometric-solving}}
+}
+}
+
+@entry{OpenCV,
+  name = {OpenCV},
+  long = {OpenCV},
+  description = {Open Source Computer Vision Library is a library of programming functions mainly aimed at real-time computer vision.%
+			\footnote{\cite{enwiki:OpenCV}}
+}
+}
+
+@entry{KStars,
+  name = {KStars},
+  long = {KStars},
+  description = {is a planetarium program. It provides an accurate graphical representation of the night sky, from any location on Earth, at any date and time. The display includes up to 100 million stars (with additional addons), 13,000 deep sky objects, constellations from different cultures, all 8 planets, the Sun and Moon, and thousands of comets, asteroids, satellites, and supernovae. It has features to appeal to users of all levels, from informative hypertext articles about astronomy, to robust control of telescopes and \gls{CCD} cameras, and logging of observations of specific objects.%
+			\footnote{\cite{enwiki:KStars}}
+}
+}
+
+@entry{gPhoto,
+  name = {gPhoto},
+  long = {gPhoto},
+  description = {is a set of software applications and libraries for use in digital photography. gPhoto supports not just retrieving of images from camera devices, but also upload and remote controlled configuration and capture, depending on whether the camera supports those features. gPhoto supports more than 2500 cameras.%
+			\footnote{\cite{enwiki:GPhoto}}
+}
+}
+
+@entry{Raspberry-Pi,
+  name = {Raspberry Pi},
+  long = {Raspberry Pi},
+  description = {is a series of small \glspl{SBC}. It is typically used by computer and electronic hobbyists as an \gls{embedded-system}.%
+			\footnote{\cite{enwiki:Raspberry_Pi}}
+}
+}
+
+@entry{Celestron,
+  name = {Celestron},
+  long = {Celestron},
+  description = {is an American company based in Torrance, California, United States, that manufactures telescopes and distributes telescopes, binoculars, spotting scopes, microscopes, and accessories.%
+			\footnote{\cite{enwiki:Celestron}}
+}
+}
+
+@entry{amateur-radio,
+  name = {amateur radio},
+  long = {amateur radio},
+  description = {is the use of the radio frequency spectrum for purposes of non-commercial exchange of messages, wireless experimentation, self-training, private recreation, radiosport, contesting, and emergency communications.%
+			\footnote{\cite{enwiki:Amateur_radio}}
+}
+}
+
+@entry{firmware,
+  name = {firmware},
+  long = {firmware},
+  description = {firmware is a specific class of computer software that provides the low-level control for a device's specific hardware. Firmware, such as the \gls{BIOS} of a \gls{PC}, may contain basic functions of a device, and may provide hardware abstraction services to higher-level software such as \glspl{OS}. For less complex devices, firmware may act as the device's complete \gls{OS}, performing all control, monitoring and data manipulation functions. Typical examples of devices containing firmware are \glspl{embedded-system} (running embedded software), home and personal-use appliances, computers, and computer peripherals.%
+			\footnote{\cite{enwiki:Firmware}}
+}
+}
+
+@entry{gpsd,
+  name = {gpsd},
+  long = {gpsd},
+  description = {is a computer software program that collects data from a \gls{GPS} receiver and provides the data via a network to potentially multiple client applications in a server-client application architecture. Gpsd may be run as a \gls{daemon} to operate transparently as a background task of the server. The network interface provides a standardized data format for multiple concurrent client applications.%
+			\footnote{\cite{enwiki:Gpsd}}
+}
+}
+
+@entry{star-catalogue,
+  name = {star catalogue},
+  long = {star catalogue},
+  description = {is an \gls{astronomical-catalogue} that lists stars. In astronomy, many stars are referred to simply by catalogue numbers. There are a great many different star catalogues which have been produced for different purposes over the years. Most modern catalogues are available in electronic format and can be freely downloaded from space agencies' data centres. The largest is being compiled from the spacecraft Gaia and thus far has over a billion stars. Completeness and accuracy are described by the faintest limiting magnitude and the accuracy of the positions.%
+			\footnote{\cite{enwiki:Star_catalogue}}
+}
+}
+
+@entry{sky-chart,
+  name = {sky chart},
+  long = {sky chart},
+  description = {or star chart or star map, also called or sky map, is a map of the night sky. Astronomers divide these into grids to use them more easily. They are used to identify and locate constellations and astronomical objects such as stars, nebulae, and galaxies. They have been used for human navigation since time immemorial. Note that a sky chart differs from an \gls{astronomical-catalogue}, which is a listing or tabulation of astronomical objects for a particular purpose.%
+			\footnote{\cite{enwiki:Star_chart}}
+}
+}
+
+@entry{astronomical-catalogue,
+  name = {astronomical catalogue},
+  long = {astronomical catalogue},
+  description = {is a list or tabulation of astronomical objects, typically grouped together because they share a common type, morphology, origin, means of detection, or method of discovery. The oldest and largest are \glspl{star-catalogue}. Hundreds have been published, including general ones and special ones for such items as infrared stars, variable stars, giant stars, multiple star systems, and star clusters. Since the late 20th century catalogs are increasingly often compiled by computers from an automated survey, and published as computer files rather than on paper.%
+			\footnote{\cite{enwiki:Astronomical_catalog}}
+}
+}
+
+@entry{Unix,
+  name = {Unix},
+  long = {Unix},
+  description = {is a family of multitasking, multiuser computer \glspl{OS} that derive from the original AT\&T Unix, whose development started in 1969 at the Bell Labs research center by Ken Thompson, Dennis Ritchie, and others.%
+			\footnote{\cite{enwiki:Unix}}
+}
+}
+
+@entry{appropriate-technology,
+  name = {appropriate technology},
+  long = {appropriate technology},
+  description = {is a movement (and its manifestations) encompassing technological choice and application that is small-scale, affordable by locals, decentralized, labor-intensive, energy-efficient, environmentally sustainable, and locally autonomous. Appropriate technology has been used to address issues in a wide range of fields. Today appropriate technology is often developed using \gls{open-source} principles, which have led to \gls{OSAT} and thus many of the plans of the technology can be freely found on the Internet.%
+			\footnote{\cite{enwiki:Appropriate_technology}}
+}
+}
+
+@entry{distribution,
+  name = {distribution},
+  long = {distribution},
+  description = {is an \gls{OS} made from a software collection that includes the \gls{Linux} kernel and, often, a package management system. \gls{Linux} users usually obtain their \gls{OS} by downloading one of the \gls{Linux} distributions, which are available for a wide variety of systems ranging from \glspl{embedded-system} and \glspl{PC} to powerful supercomputers. A typical \gls{Linux} distribution comprises a \gls{Linux} kernel, \gls{GNU} tools and libraries, additional software, documentation, a window system, a window manager, and a desktop environment. Most of the included software is \gls{FOSS} made available both as compiled binaries and in source code form, allowing modifications to the original software.%
+			\footnote{\cite{enwiki:Linux_distribution}}
+}
+}
+
+@entry{Lagrange-point,
+  name = {Lagrange point},
+  long = {Lagrange point},
+  description = {are points of equilibrium for small-mass objects under the influence of two massive orbiting bodies. At the Lagrange points, the gravitational forces of the two large bodies and the centrifugal force balance each other. This can make Lagrange points an excellent location for satellites, as few \gls{orbit} corrections are needed to maintain the desired orbit. Small objects placed in orbit at Lagrange points are in equilibrium in at least two directions relative to the center of mass of the large bodies.%
+			\footnote{\cite{enwiki:Lagrange_point}}
+}
+}
+
+@entry{GoTo,
+  name = {GoTo},
+  long = {GoTo},
+  description = {In amateur astronomy, ``GoTo'' refers to a type of telescope mount and related software that can automatically point a telescope at astronomical objects that the user selects. Both axes of a GoTo mount are driven by a motor and controlled by a computer. It may be either a microprocessor-based integrated controller or an external \gls{PC}. This differs from the single-axis semi-automated tracking of a traditional clock-drive equatorial mount. The user can command the mount to point the telescope to the celestial coordinates that the user inputs, or to objects in a pre-programmed database including ones from the Messier catalogue, the \gls{NGC}, and even major Solar System bodies (the Sun, Moon, and planets). Like a standard \gls{EQ} mount, \gls{EQ} GoTo mounts can track the night sky by driving the right ascension axis. Since both axes are computer controlled, GoTo technology also allows telescope manufacturers to add \gls{EQ} tracking to mechanically simpler altazimuth mounts.%
+			\footnote{\cite{enwiki:GoTo_telescopes}}
+}
+}
+
+@entry{slew,
+  name = {slew},
+  long = {slew},
+  description = {The process of rotating a telescope to observe a different region of the sky.%
+			\footnote{\cite{enwiki:Slewing}}
+}
+}
+
+@entry{toolchain,
+  name = {toolchain},
+  long = {toolchain},
+  description = {is a set of programming tools that is used to perform a complex software development task or to create a software product, which is typically another computer program or a set of related programs.%
+			\footnote{\cite{enwiki:Toolchain}}
+}
+}
+
+@entry{pipeline,
+  name = {pipeline},
+  long = {pipeline},
+  description = {is a set of data processing elements connected in series, where the output of one element is the input of the next one. The elements of a pipeline are often executed in parallel or in time-sliced fashion.%
+			\footnote{\cite{enwiki:Pipeline_computing}}
+}
+}
+
+@entry{embedded-system,
+  name = {embedded system},
+  long = {embedded system},
+  description = {is a computer system---a combination of a computer processor, computer memory, and input/output peripheral devices---that has a dedicated function within a larger mechanical or electronic system. It is embedded as part of a complete device often including electrical or electronic hardware and mechanical parts. Because an embedded system typically controls physical operations of the machine that it is embedded within, it often has real-time computing constraints. embedded systems control many devices in common use today. it was estimated that ninety-eight percent of all microprocessors manufactured were used in embedded systems.%
+			\footnote{\cite{enwiki:Embedded_system}}
+}
+}
+
+@entry{star-trail,
+  name = {star trail},
+  long = {star trail},
+  description = {is a type of photograph that uses long exposure times to capture diurnal circles, the apparent motion of stars in the night sky due to Earth's rotation. A star-trail photograph shows individual stars as streaks across the image, with longer exposures yielding longer arcs.%
+			\footnote{\cite{enwiki:Star_trail}}
+}
+}
+
+@entry{satellite-flare,
+  name = {satellite flare},
+  long = {satellite flare},
+  description = {is a satellite pass visible to the naked eye as a brief, bright ``flare''. It is caused by the reflection toward the Earth below of sunlight incident on satellite surfaces such as solar panels and \glspl{antenna}. Many satellites flare with magnitudes bright enough to see with the unaided eye, i.e. brighter than magnitude +6.5.%
+			\footnote{\cite{enwiki:Satellite_flare}}
+}
+}
+
+@entry{photon,
+  name = {photon},
+  long = {photon},
+  description = {is an elementary particle that is a quantum of the electromagnetic field, including electromagnetic radiation such as light and radio waves, and the force carrier for the electromagnetic force. Photons are massless, so they always move at the speed of light in vacuum, 299,792,458 meters/second.%
+			\footnote{\cite{enwiki:Photon}}
+}
+}
+
+@entry{software-repository,
+  name = {software repository},
+  long = {software repository},
+  description = {or repo for short, is a storage location for software packages. Often a table of contents is also stored, along with metadata. A software repository is typically managed by source control or repository managers. Package managers allow automatically installing and updating repositories (sometimes called ``packages'').%
+			\footnote{\cite{enwiki:Software_repository}}
+}
+}
+
+@entry{upstream,
+  name = {upstream},
+  long = {upstream},
+  description = {refers to a direction toward the original authors or maintainers of software that is distributed as source code, and is a qualification of either a version (released by the original authors, based on their upstream source code), a bug or a patch.%
+			\footnote{\cite{enwiki:Upstream}}
+}
+}
+
+@entry{daemon,
+  name = {daemon},
+  long = {daemon},
+  description = {a service in a \gls{Unix} \gls{OS}.%
+			\footnote{\cite{enwiki:Daemon}}
+}
+}
+
+@entry{Teledyne-FLIR,
+  name = {Teledyne FLIR},
+  long = {Teledyne FLIR},
+  description = {a subsidiary of Teledyne Technologies, specializes in the design and production of thermal imaging cameras and sensors. The name is based on the acronym \gls{FLIR}.%
+			\footnote{\cite{enwiki:Teledyne_FLIR}}
+}
+}
+
+@entry{Docker,
+  name = {Docker},
+  long = {Docker},
+  description = {is a set of \gls{PaaS} products that use \gls{OS}-level virtualization to deliver software in packages called containers.%
+			\footnote{\cite{enwiki:Docker}}
+}
+}
+
+@entry{binning,
+  name = {binning},
+  long = {binning},
+  description = {is the process of combining adjacent pixels throughout an image, by summing or averaging their values, during or after readout. Charge from adjacent pixels in \gls{CCD} image sensors and some other image sensors can be combined during readout, increasing the line rate or frame rate. In the context of image processing, binning is the procedure of combining clusters of adjacent pixels, throughout an image, into single pixels. For example, in 2x2 binning, an array of 4 pixels becomes a single larger pixel, reducing the number of pixels to 1/4 and halving the image resolution in each dimension. The result can be the sum, average, median, minimum, or maximum value of the cluster. This aggregation, although associated with loss of information, reduces the amount of data to be processed, facilitating analysis. The binned image has lower resolution, but the relative noise level in each pixel is generally reduced. Also called pixel binning.%
+			\footnote{\cite{enwiki:Pixel_binning}}
+}
+}
+
+@entry{alt-az-mount,
+  name = {altazimuth mount},
+  long = {altazimuth mount},
+  description = {a simple two-axis mount for supporting and rotating an instrument about two perpendicular axes --- one vertical and the other horizontal. Rotation about the vertical axis varies the azimuth (compass bearing) of the pointing direction of the instrument. Rotation about the horizontal axis varies the altitude angle (angle of elevation) of the pointing direction. These mounts are used, for example, with telescopes, cameras, and radio antennas.%
+			\footnote{\cite{Wiki21:altazmountwikipfreeencyc}}
+}
+}
+

src/Glossary.tex

@@ -1,439 +0,0 @@
-%
-% Glossary.tex
-%
-% SatNOGS Optical Unofficial Guide
-%
-% Copyright (C) 2022, Jeff Moe
-%
-% This document is licensed under the Creative Commons Attribution 4.0
-% International Public License (CC BY-SA 4.0) by Jeff Moe.
-%
-
-%%%%%%%%%%%
-% ACRONYM %
-%%%%%%%%%%%
-\newacronym[
-	description={Instrument Neutral Distributed Interface is a \gls{DCS} protocol to enable control, data acquisition and exchange among hardware devices and software front ends, emphasizing astronomical instrumentation.%
-	\footnote{\cite{enwiki:Instrument-Neutral-Distributed-Interface}}%
-		}]
-{INDI}{INDI}{Instrument Neutral Distributed Interface}
-
-\newacronym[
-	description={Debian Free Software Guidelines is a set of guidelines that the \gls{Debian} Project uses to determine whether a software license is a free software license, which in turn is used to determine whether a piece of software can be included in \gls{Debian}. The DFSG is part of the \gls{Debian} Social Contract.%
-	\footnote{\cite{enwiki:Debian-Free-Software-Guidelines}}%
-		}]
-{DFSG}{DFSG}{Debian Free Software Guidelines}
-
-\newacronym[
-	description={Flexible Image Transport System is an open standard defining a digital file format useful for storage, transmission and processing of data: formatted as multi-dimensional arrays (for example a 2D image), or tables. FITS is the most commonly used digital file format in astronomy. The FITS standard was designed specifically for astronomical data, and includes provisions such as describing photometric and spatial calibration information, together with image origin metadata.%
-	\footnote{\cite{Wiki22:fitswikipfreeencyc}}%
-		}]
-{FITS}{FITS}{Flexible Image Transport System}
-
-\newacronym[
-	description={Software-defined radio is a radio communication system where components that have been traditionally implemented in analog hardware (e.g. mixers, filters, amplifiers, modulators/demodulators, detectors, etc.) are instead implemented by means of software on a personal computer or embedded system. SDRs are used in \gls{SatNOGS} \glspl{ground-station}.%
-			\footnote{\cite{Wiki22:softwdefinradiowikipfreeencyc}}
-		}]
-{SDR}{SDR}{Software-defined radio}
-
-\newacronym[
-	description={Libre Space Foundation is a non-profit foundation registered since 2015 in Greece and the creators of the SatNOGS project.%
-			\footnote{\url{https://libre.space/about-us/}}
-		}]
-{LSF}{LSF}{Libre Space Foundation}
-
-\newacronym[
-	description={Radio frequency is the oscillation rate of an alternating electric current or voltage or of a magnetic, electric or electromagnetic field or mechanical system in the frequency range from around 20 \gls{kHz} to around 300 \gls{GHz}. This is roughly between the upper limit of audio frequencies and the lower limit of infrared frequencies; these are the frequencies at which energy from an oscillating current can radiate off a conductor into space as radio waves.%
-			\footnote{\cite{Wiki22:radiofrequwikipfreeencyc}}
-		}]
-{RF}{RF}{radio frequency}
-
-\newacronym[
-	description={Very High Frequency is the \gls{ITU} designation for the range of radio frequency electromagnetic waves (radio waves) from 30 to 300 \gls{MHz}, with corresponding wavelengths of ten meters to one meter. Frequencies immediately below VHF are denoted high frequency (HF), and the next higher frequencies are known as \gls{UHF}.%
-			\footnote{\cite{Wiki22:veryhighfrequwikipfreeencyc}}
-		}]
-{VHF}{VHF}{Very High Frequency}
-
-\newacronym[
-	description={Ultra High Frequency is the \gls{ITU} designation for radio frequencies in the range between 300 \gls{MHz} and 3 \gls{GHz}, also known as the decimetre band as the wavelengths range from one meter to one tenth of a meter (one decimeter). Lower frequency signals fall into the \gls{VHF} or lower bands.%
-			\footnote{\cite{Wiki22:ultrahighfrequwikipfreeencyc}}
-		}]
-{UHF}{UHF}{Ultra High Frequency}
-
-\newacronym[
-	description={The International Telecommunication Union is a specialized agency of the United Nations responsible for many matters related to information and communication technologies.%
-			\footnote{\cite{Wiki22:intertelecunionwikipfreeencyc}}
-		}]
-{ITU}{ITU}{International Telecommunication Union}
-
-\newacronym[
-	description={``GNU's Not Unix!'' is an extensive collection of \gls{free-software}, which can be used as an operating system or can be used in parts with other operating systems. The use of the completed GNU tools led to the family of operating systems popularly known as \gls{Linux}. Most of GNU is licensed under the GNU Project's own \gls{GPL}. GNU is also the project within which the \gls{free-software} concept originated.%
-			\footnote{\cite{Wiki22:gnuwikipfreeencyc}}
-		}]
-{GNU}{GNU}{GNU's Not Unix!}
-
-\newacronym[
-	description={GNU General Public License is a series of widely used \gls{free-software} licenses that guarantee end users the four freedoms to run, study, share, and modify the software. The license was the first copyleft for general use. Historically, the GPL license family has been one of the most popular software licenses in the \gls{FLOSS} software domain.%
-			\footnote{\cite{Wiki22:gnugenerpublilicenwikipfreeencyc}}
-		}]
-{GPL}{GPL}{GNU General Public License}
-
-\newacronym[
-	description={Simplified General Perturbations models apply to near earth objects with an orbital period of less than 225 minutes. Simplified \glspl{perturbation} models are a set of five mathematical models (SGP, SGP4, SDP4, SGP8 and SDP8) used to calculate orbital state vectors of \glspl{satellite} and space debris relative to the Earth-centered inertial coordinate system. This set of models is often referred to collectively as SGP4 due to the frequency of use of that model particularly with \gls{TLE} sets produced by \gls{NORAD} and \gls{NASA}. These models predict the effect of \glspl{perturbation} caused by the Earth's shape, drag, radiation, and gravitation effects from other bodies such as the sun and moon. See also: \gls{SDP}.%
-			\footnote{\cite{enwiki:Simplified_perturbations_models}}
-		}]
-{SGP}{SGP}{Simplified General Perturbations}
-
-\newacronym[
-	description={Simplified Deep Space Perturbations models apply to objects with an orbital period greater than 225 minutes, which corresponds to an altitude of 5,877.5 km, assuming a circular orbit. See also: \gls{SGP}.%
-			\footnote{\cite{enwiki:Simplified_perturbations_models}}
-		}]
-{SDP}{SDP}{Simplified Deep Space Perturbations}
-
-\newacronym[
-	description={North American Aerospace Defense Command is a combined organization of the United States and Canada that provides aerospace warning, air sovereignty, and protection for Canada and the continental United States.%
-			\footnote{\cite{enwiki:NORAD}}
-		}]
-{NORAD}{NORAD}{North American Aerospace Defense Command}
-
-\newacronym[
-	description={is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research.%
-			\footnote{\cite{enwiki:NASA}}
-		}]
-{NASA}{NASA}{National Aeronautics and Space Administration}
-
-\newacronym[
-	description={open-source hardware consists of physical artifacts of technology designed and offered by the open-design movement. Both \gls{FOSS} and open-source hardware are created by the open-source culture movement and apply a like concept to a variety of components. It is sometimes, thus, referred to as \gls{FOSH}. The term usually means that information about the hardware is easily discerned so that others can make it---coupling it closely to the maker movement. Hardware design (i.e. mechanical drawings, schematics, bills of material, PCB layout data, HDL source code and integrated circuit layout data), in addition to the software that drives the hardware, are all released under free/libre terms. The original sharer gains feedback and potentially improvements on the design from the \gls{FOSH} community. There is now significant evidence that such sharing can drive a high return on investment for the scientific community. It is not enough to merely use an open-source license; an open source product or project will follow open source principles, such as modular design and community collaboration.%
-			\footnote{\cite{enwiki:Open-source-hardware}}
-		}]
-{OSH}{OSH}{open-source hardware}
-
-\newacronym[
-	description={free and open-source software is a term used to refer to groups of software consisting of both \gls{free-software} and \gls{OSS} where anyone is freely licensed to use, copy, study, and change the software in any way, and the source code is openly shared so that people are encouraged to voluntarily improve the design of the software. This is in contrast to proprietary software, where the software is under restrictive copyright licensing and the source code is usually hidden from the users. FOSS maintains the software user's civil liberty rights. Other benefits of using FOSS can include decreased software costs, increased security and stability (especially in regard to malware), protecting privacy, education, and giving users more control over their own hardware. Free and open-source operating systems such as \gls{Linux} and descendants of BSD are widely utilized today, powering millions of servers, desktops, smartphones (e.g., Android), and other devices. Free-software licenses and open-source licenses are used by many software packages. The free software movement and the open-source software movement are online social movements behind widespread production and adoption of FOSS, with the former preferring to use the terms \gls{FLOSS} or free/libre.%
-			\footnote{\cite{enwiki:Free-and-open-source-software}}
-		}]
-{FOSS}{FOSS}{free and open-source software}
-
-\newacronym[
-	description={open-source software is computer software that is released under a license in which the copyright holder grants users the rights to use, study, change, and distribute the software and its source code to anyone and for any purpose. Open-source software may be developed in a collaborative public manner. Open-source software is a prominent example of open collaboration, meaning any capable user is able to participate online in development, making the number of possible contributors indefinite. The ability to examine the code facilitates public trust in the software. Open source code can be used for studying and allows capable end users to adapt software to their personal needs in a similar way user scripts and custom style sheets allow for web sites, and eventually publish the modification as a fork for users with similar preference.%
-			\footnote{\cite{enwiki:Open-source-software}}
-		}]
-{OSS}{OSS}{open-source software}
-
-%%%
-% Acronyms without citations.
-%%%
-\newacronym[description={hertz.}]{Hz}{Hz}{hertz}
-\newacronym[description={kilohertz.}]{kHz}{kHz}{kilohertz}
-\newacronym[description={megahertz.}]{MHz}{MHz}{megahertz}
-\newacronym[description={gigahertz.}]{GHz}{GHz}{gigahertz}
-\newacronym[description={digital single-lens reflex.}]{DSLR}{DSLR}{digital single-lens reflex}
-\newacronym[description={Power over Ethernet.}]{PoE}{PoE}{Power over Ethernet}
-\newacronym[description={Global Navigation \Gls{satellite} System.}]{GNSS}{GNSS}{Global Navigation Satellite System}
-\newacronym[description={Global Positioning System.}]{GPS}{GPS}{Global Positioning System}
-\newacronym[description={Ingress Protection code 67.}]{IP67}{IP67}{Ingress Protection code 67}
-\newacronym[description={Space Situational Awareness.}]{SSA}{SSA}{Space Situational Awareness}
-\newacronym[description={World Coordinate System.}]{WCS}{WCS}{World Coordinate System}
-\newacronym[description={Complementary metal-oxide-semiconductor (pronounced ``see-moss'').}]{CMOS}{CMOS}{Complementary metal–oxide–semiconductor}
-\newacronym[description={charge-coupled device.}]{CCD}{CCD}{charge-coupled device}
-\newacronym[description={Spacecraft Identification and Localization.}]{SIDLOC}{SIDLOC}{Spacecraft Identification and Localization}
-\newacronym[description={Rowe-Ackermann Schmidt \Gls{astrograph}.}]{RASA}{RASA}{Rowe-Ackermann Schmidt Astrograph}
-\newacronym[description={Commodity off the shelf.}]{COTS}{COTS}{Commodity off the shelf}
-\newacronym[description={Free open-source hardware. See also: \gls{OSH}.}]{FOSH}{FOSH}{Free open-source hardware}
-\newacronym[description={Free/libre and open-source software. See also: \gls{FOSS}.}]{FLOSS}{FLOSS}{Free/libre and open-source software}
-\newacronym[description={Simple Imaging Polynomial.}]{SIP}{SIP}{Simple Imaging Polynomial}
-\newacronym[description={Field of view.}]{FOV}{FOV}{Field of View}
-\newacronym[description={distributed control system.}]{DCS}{DCS}{distributed control system}
-\newacronym[description={Portable Network Graphics.}]{PNG}{PNG}{Portable Network Graphics}
-\newacronym[description={Comma Separated Value.}]{CSV}{CSV}{Comma Separated Value}
-
-
-%%%%%%%%%%%
-% Acronyms with citations
-%%%%%%%%%%%
-
-\newacronym[
-	description={The International System of Units, known by the international abbreviation SI in all languages and sometimes pleonastically as the SI system, is the modern form of the metric system and the world's most widely used system of measurement. Established and maintained by the General Conference on Weights and Measures (CGPM), it is the only system of measurement with an official status in nearly every country in the world, employed in science, technology, industry, and everyday commerce.%
-			\footnote{\cite{Wiki22:intersysteunitswikipfreeencyc}}
-		}]
-{SI}{SI}{International System of Units}
-
-\newacronym[
-	description={a simple two-axis mount for supporting and rotating an instrument about two perpendicular axes -- one vertical and the other horizontal. Rotation about the vertical axis varies the azimuth (compass bearing) of the pointing direction of the instrument. Rotation about the horizontal axis varies the altitude angle (angle of elevation) of the pointing direction. These mounts are used, for example, with telescopes, cameras, and radio antennas.%
-			\footnote{\cite{Wiki21:altazmountwikipfreeencyc}}
-		}]
-{Alt-Az}{Alt/Az mount}{Altazimuth mount}
-
-\newacronym[
-	description={two-line element set is a data format encoding a list of orbital elements of an Earth-orbiting object for a given point in time, the epoch. Using a suitable prediction formula, the state (position and velocity) at any point in the past or future can be estimated to some accuracy. TLEs can describe the trajectories only of Earth-orbiting objects. TLEs are widely used as input for projecting the future orbital tracks of space debris for purposes of characterizing ``future debris events to support risk analysis, close approach analysis, collision avoidance maneuvering'' and forensic analysis. The format was originally intended for punched cards, encoding a set of elements on two standard 80-column cards.%
-			\footnote{\cite{Wiki22:twolineelemesetwikipfreeencyc}}
-		}]
-{TLE}{TLE}{two-line element set}
-
-%%%%%%%%%%%%
-% GLOSSARY %
-%%%%%%%%%%%%
-
-%%%%%%%%%%%%
-% Glossary entries without citations that are not acronyms.
-%%%%%%%%%%%%
-
-\newglossaryentry{artificial satellite}
-{ name={artificial satellite},
-	description={is a \gls{satellite} put into \gls{orbit} by humans, not ``naturally'' occurring.}}
-
-\newglossaryentry{libre-software}
-{ name={libre software},
-	description={See: \gls{free-software}.}}
-
-
-%%%%%%%%%%%%
-% Glossary entries with footnotes that are not acronyms.
-%%%%%%%%%%%%
-\newglossaryentry{AstroImageJ}
-{ name={AstroImageJ},
-	description={Application for astronomy and \gls{satellite} image analysis.%
-			\footnote{\url{https://www.astro.louisville.edu/software/astroimagej/}}
-		}}
-
-\newglossaryentry{skymap}
-{ name={skymap},
-	description={is part of \gls{sattools}. Visualize \glspl{satellite} on a map of the sky.%
-			\footnote{\url{https://github.com/cbassa/sattools/blob/master/skymap.c}}
-		}}
-
-\newglossaryentry{satid}
-{ name={satid},
-	description={is part of \gls{sattools}.%
-			\footnote{\url{https://github.com/cbassa/sattools/blob/master/satid.c}}
-		}}
-
-\newglossaryentry{sattools}
-{ name={sattools},
-	description={Satellite Tracking Toolkit. The main \texttt{sattools} applications are being ported to \gls{stvid} and other related \gls{Python} applications.%
-			\footnote{\url{https://github.com/cbassa/sattools}}
-		}}
-
-\newglossaryentry{satpredict}
-{ name={satpredict},
-	description={is a software application to compute \gls{satellite} predictions. It is used by \gls{stvid}.%
-			\footnote{\url{https://github.com/cbassa/satpredict}}
-		}}
-
-\newglossaryentry{stvid}
-{ name={stvid},
-	description={\Gls{satellite} tools video application for acquiring and processing sky images.%
-			\footnote{\url{https://github.com/cbassa/stvid}}
-		}}
-
-\newglossaryentry{hough3d-code}
-{ name={hough3d-code},
-	description={is a software application for Iterative Hough Transform for Line Detection in 3D Point Clouds.%
-			\footnote{\url{https://gitlab.com/pierros/hough3d-code}}
-		}}
-
-\newglossaryentry{ground-station}
-{ name={ground station},
-	description={a setup of equipment such as computers, cameras, \glspl{SDR}, antennas, and receivers, located on Earth, observing space.
-		}}
-
-\newglossaryentry{SatNOGS-Optical}
-{ name={SatNOGS Optical},
-	description={is a project by the \gls{LSF} to add optical ground stations to the SatNOGS network.%
-			\footnote{\url{https://satnogs.org/}}
-		}}
-
-\newglossaryentry{SatNOGS DB}
-{ name={SatNOGS DB},
-	description={is an effort to create an hollistic, unified, global database for all artificial objects in space (\glspl{satellite} and spacecrafts). Users can view and export the data, contribute to it, or connect applications using an API. It is part of the \gls{SatNOGS} project.%
-			\footnote{\url{https://db.satnogs.org/}}
-		}}
-
-\newglossaryentry{SatNOGS}
-{ name={SatNOGS},
-	description={Open Source global network of \gls{satellite} ground stations.%
-			\footnote{\url{https://satnogs.org/}}
-		}}
-
-\newglossaryentry{optical-ground-station}
-{ name={optical ground station},
-	description={a ground station using optical equipment (cameras) instead of antennas.
-		}}
-
-\newglossaryentry{antenna}
-{ name={antenna},
-	description={the interface between radio waves propagating through space and electric currents moving in metal conductors, used with a transmitter or receiver.%
-			\footnote{\cite{Wiki22:antenradiowikipfreeencyc}}
-		}}
-
-\newglossaryentry{mast}
-{ name={mast},
-	description={typically tall structures designed to support antennas for telecommunications and broadcasting.%
-			\footnote{\cite{Wiki22:radiomaststowerwikipfreeencyc}}
-		}}
-
-\newglossaryentry{rotator}
-{ name={rotator},
-	description={a device used to change the orientation, within the horizontal plane, of a directional antenna. Most antenna rotators have two parts, the rotator unit and the controller. The controller is normally placed near the equipment which the antenna is connected to, while the rotator is mounted on the antenna mast directly below the antenna. Rotators are commonly used in amateur radio.%
-			\footnote{\cite{Wiki22:antenrotatwikipfreeencyc}}
-		}}
-
-\newglossaryentry{Debian}
-{ name={Debian},
-	description={a \gls{GNU}/\gls{Linux} distribution composed of free and open-source software, developed by the community-supported Debian Project, which was established by Ian Murdock on August 16, 1993. Debian is the basis for many other distributions, notably Ubuntu.
-			Debian is one of the oldest operating systems based on the Linux kernel.%
-			\footnote{\cite{Wiki22:debiawikipfreeencyc}}
-		}}
-
-\newglossaryentry{Linux}
-{ name={Linux},
-	description={is a free and open-source, monolithic, modular, multitasking, Unix-like operating system kernel. It was originally authored in 1991 by Linus Torvalds for his i386-based PC, and it was soon adopted as the kernel for the \gls{GNU} operating system, which was written to be a free (libre) replacement for Unix.%
-			\footnote{\cite{Wiki22:linuxkernewikipfreeencyc}}
-		}}
-
-\newglossaryentry{open-source}
-{ name={Open Source},
-	description={is source code that is made freely available for possible modification and redistribution. Products include permission to use the source code, design documents, or content of the product. The open-source model is a decentralized software development model that encourages open collaboration. A main principle of open-source software development is peer production, with products such as source code, blueprints, and documentation freely available to the public. The open-source movement in software began as a response to the limitations of proprietary code. The model is used for projects such as in open-source appropriate technology.%
-			\footnote{\cite{Wiki22:opensourcwikipfreeencyc}}
-		}}
-
-\newglossaryentry{free-software}
-{ name={Free Software},
-	description={or libre software, is computer software distributed under terms that allow users to run the software for any purpose as well as to study, change, and distribute it and any adapted versions. Free software is a matter of liberty, not price; all users are legally free to do what they want with their copies of a free software (including profiting from them) regardless of how much is paid to obtain the program. Computer programs are deemed ``free'' if they give end-users (not just the developer) ultimate control over the software and, subsequently, over their devices.%
-			\footnote{\cite{Wiki22:freesoftwwikipfreeencyc}}
-		}}
-
-\newglossaryentry{Matrix}
-{ name={Matrix},
-	description={an open standard and communication protocol for real-time communication.%
-			\footnote{\cite{Wiki22:matriprotowikipfreeencyc}}
-		}}
-
-\newglossaryentry{telescope}
-{ name={telescope},
-	description={is an optical instrument using lenses, curved mirrors, or a combination of both to observe distant objects, or various devices used to observe distant objects by their emission, absorption, or reflection of electromagnetic radiation. The word telescope now refers to a wide range of instruments capable of detecting different regions of the electromagnetic spectrum, and in some cases other types of detectors.%
-			\footnote{\cite{enwiki:Telescope}}
-		}}
-
-\newglossaryentry{astrograph}
-{ name={astrograph},
-	description={is a telescope designed for the sole purpose of astrophotography. Astrographs are mostly used in wide-field astronomical surveys of the sky and for detection of objects such as asteroids, meteors, and comets.%
-			\footnote{\cite{enwiki:Astrograph}}
-		}}
-
-\newglossaryentry{satellite}
-{ name={satellite},
-	description={is an object intentionally placed into \gls{orbit} in outer space. Except for passive satellites, most satellites have an electricity generation system for equipment on board. Most satellites also have a method of communication to ground stations, called transponders. Many satellites use a standardized bus to save cost and work, the most popular of which is small \Glspl{cubesat}. Similar satellites can work together as a group, forming constellations.%
-			\footnote{\cite{enwiki:Satellite}}
-		}}
-
-\newglossaryentry{cubesat}
-{ name={CubeSat},
-	description={is a class of miniaturized \gls{satellite} based around a form factor consisting of 10 cm (3.9 in) cubes. CubeSats have a mass of no more than 2 kg (4.4 lb) per unit, and often use \gls{COTS} components for their electronics and structure. CubeSats are put into \gls{orbit} by deployers on the International Space Station, or launched as secondary payloads on a launch vehicle. More than a thousand CubeSats have been launched.%
-			\footnote{\cite{enwiki:CubeSat}}
-		}}
-
-\newglossaryentry{orbit}
-{ name={orbit},
-	description={is the curved trajectory of an object such as the trajectory of a planet around a star, or of a natural satellite around a planet, or of an artificial satellite around an object or position in space such as a planet, moon, asteroid, or Lagrange point. Normally, orbit refers to a regularly repeating trajectory, although it may also refer to a non-repeating trajectory. To a close approximation, planets and \glspl{satellite} follow elliptic orbits, with the center of mass being orbited at a focal point of the ellipse, as described by Kepler's laws of planetary motion. For most situations, orbital motion is adequately approximated by Newtonian mechanics, which explains gravity as a force obeying an inverse-square law. However, Albert Einstein's general theory of relativity, which accounts for gravity as due to curvature of spacetime, with orbits following geodesics, provides a more accurate calculation and understanding of the exact mechanics of orbital motion.%
-			\footnote{\cite{enwiki:Orbit}}
-		}}
-
-\newglossaryentry{perturbation}
-{ name={perturbation},
-	description={is the complex motion of a massive body subjected to forces other than the gravitational attraction of a single other massive body. The other forces can include a third (fourth, fifth, etc.) body, resistance, as from an atmosphere, and the off-center attraction of an oblate or otherwise misshapen body.%
-			\footnote{\cite{enwiki:Perturbation-astronomy}}
-		}}
-
-\newglossaryentry{telemetry}
-{ name={telemetry},
-	description={is the in situ collection of measurements or other data at remote points and their automatic transmission to receiving equipment (telecommunication) for monitoring. The word is derived from the Greek roots tele, ``remote'', and metron, ``measure''. Although the term commonly refers to wireless data transfer mechanisms (e.g., using radio, ultrasonic, or infrared systems), it also encompasses data transferred over other media such as a telephone or computer network, optical link or other wired communications like power line carriers.%
-			\footnote{\cite{enwiki:Telemetry}}
-		}}
-
-\newglossaryentry{Grafana}
-{ name={Grafana},
-	description={is a multi-platform \gls{open-source} analytics and interactive visualization web application. It provides charts, graphs, and alerts for the web when connected to supported data sources. Users can create complex monitoring dashboards using interactive query builders. It is used by the \gls{SatNOGS} project to visualize \gls{satellite} \gls{telemetry}.%
-			\footnote{\cite{enwiki:Grafana}}
-		}}
-
-\newglossaryentry{Python}
-{ name={Python},
-	description={is a high-level, interpreted, general-purpose programming language. Its design philosophy emphasizes code readability. It is often described as a ``batteries included'' language due to its comprehensive standard library. Python consistently ranks as one of the most popular programming languages. It is one of the main languages of the \gls{SatNOGS} project and \gls{stvid}.%
-			\footnote{\cite{enwiki:Python-language}}
-		}}
-
-\newglossaryentry{C}
-{ name={C},
-	description={is a general-purpose computer programming language. It was created in the 1970s by Dennis Ritchie, and remains very widely used and influential. By design, C's features cleanly reflect the capabilities of the targeted CPUs. It has found lasting use in operating systems, device drivers, protocol stacks, though decreasingly for application software. C is commonly used on computer architectures that range from the largest supercomputers to the smallest microcontrollers and embedded systems. C is used in the \gls{sattools} suite of applications.%
-			\footnote{\cite{enwiki:C-language}}
-		}}
-
-\newglossaryentry{libre}
-{ name={libre},
-	description={The English adjective free is commonly used in one of two meanings: ``at no monetary cost'' (gratis) and ``with little or no restriction'' (libre). This ambiguity of free can cause issues where the distinction is important, as it often is in dealing with laws concerning the use of information, such as copyright and patents. The terms gratis and libre may be used to categorise computer programs, according to the licenses and legal restrictions that cover them, in the free software and open source communities, as well as the broader free culture movement. For example, they are used to distinguish freeware (software gratis) from \gls{free-software} (software libre). ``Think free as in free speech, not free beer.'' -- Richard Stallman.%
-			\footnote{\cite{enwiki:Gratis-versus-libre}}
-		}}
-
-\newglossaryentry{plate-solver}
-{ name={plate solver},
-	description={is software implementing a technique used in astronomy and applied on celestial images. Solving an image is finding match between the imaged stars and a star catalogue. The solution is a math model describing the corresponding astronomical position of each image pixel. The position of reference catalogue stars has to be known to a high accuracy so an astrometric reference catalogue is used. The image solution contains a reference point, often the image centre, image scale, image orientation and in some cases an image distortion model. With the astrometric solution it is possible to: 1) Calculate the celestial coordinates of any object on the image. 2) Synchronize the telescope mount or satellite pointing position to the center of the image taken. Astrometric solving programs extract the star x,y positions from the celestial image, groups them in three-star triangles or four-star quads. Then it calculates for each group a geometric hash code based on the distance and/or angles between the stars in the group. It then compares the resulting hash codes with the hash codes created from catalogue stars to find a match. If it finds sufficient statistically reliable matches, it can calculate transformation factors. There are several conventions to model the transformation from image pixel location to the corresponding celestial coordinates. The simplest linear model is called the \gls{WCS}. A more advanced convention is \gls{SIP} describing the transformation in polynomials to cope with non-linear geometric distortion in the celestial image, mainly caused by the optics.%
-			\footnote{\cite{enwiki:Astrometric-solving}}
-		}}
-
-% TO ADD
-% RamSat
-% Dashboard
-% photon
-% giza (pgplot?)
-% decay
-% astrometry.net
-% astap
-% Source Extractor
-% Watney
-% PiCamera
-% BSD
-% Unix
-% SDK
-% IMX174
-% OpenCV
-% MIPI
-% f-stop etc.
-% KStars
-% ekos
-% gphoto
-% distributions
-% stphot
-% ASM
-% allsky
-% V4L
-% Pi/Raspberry Pi
-% appropriate technology
-% Lagrange point
-% LEO, GEO etc
-% PCB
-% HDL
-% constellations
-% fork
-% port
-% hamlib
-% PTZ
-% pier
-% Celestron
-% iOptron
-% amateur radio
-% ham
-% star trails
-% EQ equitorial
-% fork software, fork mount
-% firmware
-% ISS
-% GOTO
-% sidereal
-% slew
-% sky chart
-% PPS (gps)
-% gpsd
-% List of Software ?
-% NTP
-% IP

src/Ground_Stations.tex

@@ -11,71 +11,65 @@
 
 \section{Overview of Ground Stations}
 \label{sec:overview-groundstations}
-\index{ground station}\index{SDR}\index{antenna}\index{camera}
-\index{receiver}\index{antenna}
-\Glspl{ground-station} are a setup of equipment such as computers, cameras,
-\glspl{SDR}, antennas, and receivers, located on Earth, observing space.
+\index{camera}
+\index{receiver}
+\Glspl{ground-station} are a setup of equipment such as \glspl{embedded-system}, cameras,
+\glspl{SDR}, \glspl{antenna}, and receivers, located on Earth, observing space.
 
 
 \section{SatNOGS Ground Stations}
-\index{ground station}\index{Libre Space Foundation}
-\index{rotator}
 
 The \gls{LSF} built the \gls{SatNOGS} network using distributed,
 volunteer-run, \gls{RF} \glspl{ground-station} using \glspl{SDR}, such as in
 figure \ref{fig:spacecruft-rotator}, page \pageref{fig:spacecruft-rotator}.%
 \footnote{\url{https://spacecruft.org/assets/i/spacecruft-rotator.png}}
 It shows a \gls{SatNOGS} \gls{ground-station} with \gls{VHF} (right) and \gls{UHF} (left)
-\glspl{antenna} on a \gls{mast} with an \gls{Alt-Az} \gls{rotator}.
+\glspl{antenna} on a \gls{mast} with an \gls{alt-az-mount} \gls{rotator}.
 \glspl{SDR} can be used as \gls{RF} receivers.%
 \footnote{\cite{Wiki22:softwdefinradiowikipfreeencyc}}
-\index{radio}\index{SDR}\index{RF}\index{VHF}\index{UHF}\index{rotator}\index{antenna}
 
 \begin{figure}[p!]
 	\begin{center}
 		\centering
 		\includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{spacecruft-rotator.png}
-		\caption{SatNOGS ground station with antennas.}
+		\caption{\gls{SatNOGS} \gls{ground-station} with antennas.}
 		\label{fig:spacecruft-rotator}
-		\index{radio}\index{RF}\index{rotator}\index{antenna}\index{ground station}
 	\end{center}
 \end{figure}
 
-Ground stations can be viewed on the SatNOGS network website, such as
+\Glspl{ground-station} can be viewed on the \gls{SatNOGS} network website, such as
 as the example in figure \ref{fig:satnogs-ground-station-web}, page \pageref{fig:satnogs-ground-station-web}.%
 \footnote{\url{https://network.satnogs.org/stations/2733/}}
 
-\begin{figure}[h!]
-	\begin{framed}
+\begin{sidewaysfigure}[p!]
 	\begin{center}
 		\centering
-		\includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{satnogs-ground-station-web.png}
+		\includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{satnogs-ground-station-web.png}
 		\caption{Ground station viewed on SatNOGS website, example.}
 		\label{fig:satnogs-ground-station-web}
-		\index{ground station}
 	\end{center}
-	\end{framed}
-\end{figure}
+\end{sidewaysfigure}
 
 
 \section{SatNOGS Optical Ground Stations}
-\index{ground station}\index{Libre Space Foundation}
+
 The \gls{LSF} is developing \gls{SatNOGS-Optical} to add
-\glspl{optical-ground-station} to the distributed network.
+\glspl{optical-ground-station} to the network.
 
 Prototype \glspl{optical-ground-station} are being developed. An example
-setup, using a Sky-Watcher EQ6-R Pro telescope tripod and tracking mount,
-\index{Sky-Watcher}\index{telescope}\index{tripod}\index{mount}\index{enclosure}
-can be seen in Figure
+setup, using a Sky-Watcher EQ6-R Pro \gls{telescope} tripod and tracking mount,
+\index{Sky-Watcher}\index{tripod}\index{mount}\index{enclosure}
+\index{mount}\index{track}
+can be seen in figure
 \ref{fig:video-enclosure-mount-tripod}, page \pageref{fig:video-enclosure-mount-tripod}.
 
 \begin{figure}[p!]
 	\begin{center}
 		\centering
 		\includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{video-enclosure-mount-tripod.png}
-		\caption{SatNOGS Optical ground station prototype.}
+		\caption{\gls{SatNOGS-Optical} \gls{ground-station} prototype.}
 		\label{fig:video-enclosure-mount-tripod}
-		\index{telescope}\index{tripod}\index{mount}\index{enclosure}
+		\index{tripod}\index{mount}\index{enclosure}
 	\end{center}
 \end{figure}
 

src/Hardware.tex

@@ -14,35 +14,37 @@
 \index{hardware}
 Hardware considerations for a \gls{SatNOGS-Optical} \gls{ground-station}.
 
-Main hardware components in an optical ground station:
+Main hardware components in an \gls{optical-ground-station}:
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{itemize}
 	\item Lens. \index{lens}
 	\item Camera. \index{camera}
-	\item Computer. \index{computer}
+	\item \Gls{embedded-system} (computer).
 \end{itemize}
 \end{mdframed}
-\index{lens}\index{camera}\index{embedded computer}
+\index{lens}\index{camera}
 
 Other components:
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{itemize}
 	\item Ethernet cable. \index{ethernet}
-	\item USB cable. \index{USB}
+	\item \gls{USB} cable. 
 	\item Enclosure. \index{enclosure}
 	\item Power supply. \index{power supply}
 	\item Tripod. \index{tripod}
-	\item Manual or tracking mount. \index{mount}
+	\item Manual or tracking mount. \index{mount}\index{track}
 	\item Power source, grid or alternative.
-	\item Internet, wifi or ethernet.
+	\item Internet, wifi or ethernet.\index{ethernet}
 \end{itemize}
 \end{mdframed}
-\index{ethernet}\index{USB}\index{enclosure}\index{power supply}
+\index{ethernet}\index{enclosure}\index{power supply}
 \index{tripod}\index{mount}\index{wifi}
 
 \section{Camera}
 \label{sec:hardware-camera}
+\index{camera}
+% XXX aravis
 
 Cameras being evaluated:
 
@@ -51,7 +53,7 @@ Cameras being evaluated:
 	\item The Imaging Source IMX174 based, monochrome. \index{The Imaging Source}\index{IMX174}
 	\item ZWO ASI174MM, monochrome. \index{ZWO ASI}
 	\item ZWO ASI1600MM Pro, monochrome. \index{ZWO ASI}
-	\item \gls{DSLR} camera. \index{DSLR}
+	\item \gls{DSLR} camera. 
 	\item PiCamera. \index{PiCamera}
 \end{itemize}
 \end{mdframed}
@@ -59,8 +61,8 @@ Cameras being evaluated:
 \fbox{
 	\parbox{\linewidth}{
 		\textcolor{red}{NOTICE:} \\
-		ZWO/ASI cameras require proprietary non-libre software on host computer and is not \gls{DFSG} compatible.
-		\index{proprietary}\index{DFSG}
+		ZWO/ASI cameras require proprietary non-\gls{libre} software on host computer and is not \gls{DFSG} compatible.
+		\index{proprietary}
 	}
 }
 
@@ -69,36 +71,34 @@ Cameras being evaluated:
 \index{lens}
 For lenses, the faster the better.
 F1.2 works well.
-F1.8 is the maxmimum recommended.
+F1.8 is the maximum recommended.
 
 Lenses being tested:
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{itemize}
 	\item Kowa 50mm f1.4 C-mount. \index{Kowa}
-	\item Canon EF 50mm f1.2 USM. \index{Canon}
+	\item Canon EF 50mm f1.2 \gls{USM}. \index{Canon}
 \end{itemize}
 \end{mdframed}
 
-\section{Embedded Computer}
+\section{Embedded System}
 \label{sec:hardware-computer}
-\index{hardware}\index{embedded computer}
-Embedded computers, such as Raspberry Pi, that can be used.
-\index{Raspberry Pi}
+\index{hardware}
+\Glspl{embedded-system}, such as \gls{Raspberry-Pi}, that can be used.
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
 	\item [Odroid N2] --- Confirmed working. \index{Odroid}
 	\item [Odroid M1] --- Testing.
-	\item [Raspberry Pi 3] --- ? \index{Raspberry Pi}
-	\item [Raspberry Pi 4] --- ? \index{Raspberry Pi}
-	\item [Intel NUC] --- ? \index{Intel}
+	\item [\gls{Raspberry-Pi} 3] --- ?
+	\item [\gls{Raspberry-Pi} 4] --- ?
+	\item [Intel \gls{NUC}] --- ? \index{Intel}
 \end{description}
 \end{mdframed}
 
-\subsection{Comparison}
-Comparing embedded computers for \gls{SatNOGS-Optical}.
-\index{embedded computer}
+\subsection{Embedded Systems Comparison}
+Comparing \glspl{embedded-system} for \gls{SatNOGS-Optical}.
 
 \begin{center}
 \begin{table}[ht]
@@ -107,14 +107,14 @@ Comparing embedded computers for \gls{SatNOGS-Optical}.
 	\hspace*{-1.5cm}
 	\begin{tabularx}{250pt}{|c|c|c|c|c|}
 		\hline
-		Make   & Model & Architecture & Max RAM & eMMC \\
+		Make   & Model & Architecture & Max RAM & eMMC\\
 		\hline
-		Odroid & N2    & ARM64        & 4 GB    & Yes  \\
+		Odroid & N2    & ARM64        & 4 GB    & Yes\\
 		\hline
-		Odroid & M1    & ARM64        & 8 GB    & Yes  \\
+		Odroid & M1    & ARM64        & 8 GB    & Yes\\
 		\hline
 	\end{tabularx}
-	\caption{Comparison of embedded computers}
+	\caption{Comparison of embedded systems}
 	\label{compare-embed}
 	\end{center}
 	\end{mdframed}
@@ -123,9 +123,9 @@ Comparing embedded computers for \gls{SatNOGS-Optical}.
 \index{Odroid}\index{ARM64}\index{eMMC}
 
 
-\section{Example Optical Ground Station wtih Tracking}
+\section{Example Optical Ground Station with Tracking}
 \label{sec:hardware-tracking-ground-station}
-\index{ground station}\index{mount}\index{tracking}
+\index{mount}\index{track}
 \index{tripod}
 
 This is an example of a tracking \gls{ground-station}.
@@ -136,25 +136,26 @@ The full setup on tripod, can be seen in
 
 A close up of the setup can be seen at
 \ref{fig:video-enclosure-mount}, page \pageref{fig:video-enclosure-mount},
-showing the Sky-Watcher telescope tracking mount,
+showing the Sky-Watcher \gls{telescope} tracking mount,
 a Bosch \gls{PoE} camera enclosure,
 and through the glass the camera lens.
-\index{Sky-Watcher}\index{telescope}\index{mount}\index{Bosch}\index{PoE}\index{camera}
+\index{Sky-Watcher}\index{mount}\index{Bosch}\index{camera}
 \index{lens}
-In the background is a white antenna for \gls{GNSS} (\gls{GPS}) and a solar power setup.
-\index{GNSS}\index{GPS}\index{solar power}
+In the background is a white \gls{antenna} for \gls{GNSS} (\gls{GPS}) and a solar power setup.
+\index{solar power}
 
 \begin{figure}[p!]
 	\begin{center}
 		\includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{video-enclosure-mount.png}
 		\caption{SatNOGS-Optical ground station prototype.}
 		\label{fig:video-enclosure-mount}
-		\index{telescope}\index{mount}\index{camera}
+		\index{mount}\index{camera}
 	\end{center}
 \end{figure}
 
 The camera lens is protected by the enclosure glass, which is \gls{IP67} (XXX) rated.
 See a close up of the front of the enclosure and camera lens in figure
+\index{enclosure}\index{lens}\index{camera}
 \ref{fig:video-enclosure-front}, page \pageref{fig:video-enclosure-front}.
 
 \begin{figure}[h!]
@@ -171,7 +172,8 @@ See a close up of the front of the enclosure and camera lens in figure
 As seen in figure
 \ref{fig:video-enclosure-left}, page \pageref{fig:video-enclosure-left},
 the left side of the enclosure has a hinge for opening.
-The bottom white component is part of the telescope mount.
+The bottom white component is part of the \gls{telescope} mount.
+\index{mount}
 
 \begin{figure}[h!]
 	\begin{framed}
@@ -203,6 +205,7 @@ These are unscrewed with a hex head tool (supplied) to open the enclosure.
 \end{figure}
 
 The enclosure is opened from the right side, as shown in figure
+\index{enclosure}
 \ref{fig:video-enclosure-right}, page \pageref{fig:video-enclosure-right}.
 
 \begin{sidewaysfigure}[p!]
@@ -215,6 +218,7 @@ The enclosure is opened from the right side, as shown in figure
 \end{sidewaysfigure}
 
 Inside the camera enclosure, as shown in Figure
+\index{enclosure}
 \ref{fig:video-enclosure-top-open}, page \pageref{fig:video-enclosure-top-open},
 is:
 
@@ -222,23 +226,23 @@ is:
 \begin{itemize}
 	\item The Imaging Source DMX camera with Sony IMX174 \gls{CMOS}. \index{The Imaging Source}\index{IMX174}
 	\item Kowa 50mm f1.4 C-mount lens.\index{Kowa}
-	\item Odroid N2 running \gls{Debian} \gls{GNU} \gls{Linux} system. \index{Odroid}\index{Debian}\index{GNU}\index{Linux}
+	\item Odroid N2 running \gls{Debian} \gls{GNU} \gls{Linux} system. \index{Odroid}
 	\item Odroid N2 plastic enclosure, large half, hole drilled for ad-hoc mounting.
 	\item Blower fan on top, with power cable (came with Bosch enclosure). \index{fan}
 	\item Fan, maybe not so useful, with power cable (came with Bosch enclosure).
 	\item Camera mounting plate (came with Bosch enclosure). \index{camera}
 	\item Camera mounting screws, M6x25 (?).
-	\item Ethernet cable, internal, short white (came with Bosch enclosure). \index{ethernet}
-	\item \gls{PoE} ethernet cable, external, plugged into \gls{PoE} switch for data and power. \index{PoE}
-	\item USB 3 cable, internal, way too long, needs replacing, from Odroid to camera. XXX flat connector
-	\item USB 3 cable, external, from Odroid to telescope mount. XXX large rectangle connector \index{USB}
-	\item ``Custom'' 12V DC power cable from Bosch \gls{PoE} to Odroid.
+	\item Ethernet cable, internal, short white (came with Bosch enclosure). \index{ethernet}\index{Bosch}
+	\item \gls{PoE} ethernet cable, external, plugged into \gls{PoE} switch for data and power. 
+	\item \gls{USB} 3 cable, internal, way too long, needs replacing, from Odroid to camera. XXX flat connector
+	\item \gls{USB} 3 cable, external, from Odroid to \gls{telescope} mount. XXX large rectangle connector 
+	\item ``Custom'' 12\gls{V} \gls{DC} power cable from Bosch \gls{PoE} to Odroid.
 	\item Assorted nuts, bolts, and washers for an ad-hoc standoff height.
 \end{itemize}
 \end{mdframed}
-\index{camera}\index{Kowa}\index{The Imaging Source}\index{Odroid}\index{Debian}
-\index{fan}\index{power cable}\index{mount plate}\index{Bosh}
-\index{ethernet cable}\index{PoE}\index{USB}\index{power cable}
+\index{camera}\index{Kowa}\index{The Imaging Source}\index{Odroid}
+\index{fan}\index{power cable}\index{mount plate}\index{Bosch}
+\index{ethernet}\index{power cable}
 
 \begin{sidewaysfigure}[p!]
 	\begin{center}
@@ -250,6 +254,7 @@ is:
 \end{sidewaysfigure}
 
 The top of the enclosure shows weather protection and a sun visor.
+\index{enclosure}\index{weather}
 See figure \ref{fig:video-enclosure-top}, page \pageref{fig:video-enclosure-top}.
 
 \begin{figure}[h!]
@@ -266,7 +271,7 @@ See figure \ref{fig:video-enclosure-top}, page \pageref{fig:video-enclosure-top}
 
 \section{Tripods}
 \label{sec:hardware-tripod}
-\index{hardware}\index{tripod}\index{camera}
+\index{hardware}\index{tripod}\index{camera}\index{pier}
 
 The camera setup can be mounted a wide variety of ways,
 from just setting the camera somewhere (worst option), to a heavy duty
@@ -281,13 +286,13 @@ Tripod and similar options include:
 \begin{description}
 	\item [No mount] --- Quick and dirty, just hang the camera out somewhere sitting on something.
 	\item [Small tripod] --- There are small desk tripods than can be used with lighter
-         setups, such as used with a Raspberry Pi PiCamera.
+         setups, such as used with a \gls{Raspberry-Pi} PiCamera.\index{tripod}
 	\item [Photography Tripod] --- Using a common camera tripod, of which there is a wide
-         variety, from light to heavy.
-	\item [Telescope Tripod] --- Similar to photography tripods, but typically heavier weight.
-	\item [Telescope Portable Pier] --- Similar to a telescope tripod, but much heavier, typically
-         with a larger center pier post. Still movable, and folds up similar to a photography tripod.
-	\item [Telescope Pier] --- A wide variety, such as making a ~1.5 meter permanent cement post.
+         variety, from light to heavy.\index{tripod}
+	\item [\Gls{telescope} Tripod] --- Similar to photography tripods, but typically heavier weight.\index{tripod}
+	\item [\Gls{telescope} Portable Pier] --- Similar to a \gls{telescope} tripod, but much heavier, typically
+         with a larger center pier post. Still movable, and folds up similar to a photography tripod.\index{pier}
+	\item [\Gls{telescope} Pier] --- A wide variety, such as making a roughly 1.5 meter permanent cement post.
 \end{description} 
 \end{mdframed}
 \index{pier}
@@ -295,7 +300,7 @@ Tripod and similar options include:
 
 \section{Mounts}
 \label{sec:hardware-mounts}
-\index{mount}\index{track}
+\index{mount}\index{track}\index{tripod}
 For mounts, there are two main types: tracking or static.
 By the latter ``static'' mounts, it is meant that the
 camera, the tripod, and the mount all stay motionless.
@@ -317,70 +322,69 @@ Static mounting options include:
 \index{camera}\index{mount}
 
 Tracking mount options to consider include:
+\index{mount}\index{track}
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
-	\item [Sky-Watcher EQ6-R Pro] --- Telescope mount using {INDI}.
-	\item [Celestron] --- Wide variety of telescope mounts using {INDI}.
-	\item [iOptron] --- Telescope mount with (untested) satellite tracking.
-	\item [INDI Telescope Mounts] --- A wide variety of other \gls{INDI} compatible telescope mounts.
+	\item [Sky-Watcher EQ6-R Pro] --- \Gls{telescope} mount using \gls{INDI}.
+	\item [\gls{Celestron}] --- Wide variety of \gls{telescope} mounts using \gls{INDI}.
+	\item [iOptron] --- \Gls{telescope} mount with (untested) satellite tracking.
+	\item [\gls{INDI} \Gls{telescope} Mounts] --- A wide variety of other \gls{INDI} compatible \gls{telescope} mounts.
 	\item [Yaesu G-5500] --- Antenna \gls{rotator}.
 	\item [hamlib] --- Other hamlib compatible \glspl{rotator}.
-	\item [FLIR PTU-5] --- High Performance Pan-Tilt Unit designed for security cameras (untested, no drivers?).
-	\item [Misc PTZ] --- Other security camera pan/tilt mounts.
+	\item [\gls{Teledyne-FLIR} PTU-5] --- High Performance \gls{PTZ} Unit designed for security cameras (untested, no drivers?).
+	\item [Misc \gls{PTZ}] --- Other security camera \gls{PTZ} mounts.
 \end{description}
 \end{mdframed}
-\index{track}\index{mount}\index{Sky-Watcher}\index{INDI}\index{Celestron}
-\index{Yaesu}\index{rotator}\index{hamlib}\index{FLIR}\index{pan/tilt}
-\index{iOptron}
+\index{track}\index{mount}\index{Sky-Watcher}\index{Yaesu}\index{hamlib}\index{iOptron}
+\index{G-5500}
 
 Tracking mounts aren't widely used, but there is support for them in
-\texttt{stvid} when acquiring data.
+\texttt{\gls{stvid}} when acquiring data.
 The tracking needs to be set up independently of \texttt{stvid}.
-At present, I use KStars with Ekos to control a Sky-Watcher tracking
-mount.
-\index{KStars}\index{Ekos}\index{Sky-Watcher}\index{stvid}\index{track}
+At present, I use \gls{KStars} with Ekos to control a Sky-Watcher EQ6-R Pro
+tracking mount.
+\index{Ekos}\index{Sky-Watcher}\index{track}
 
 For tracking, there a few different ways to track:
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
 	\item [Static] --- No tracking, just point at one place in the sky.
-         Generates star trails.
+         Generates \glspl{star-trail}.
          Generates satellite trails.
 	\item [Sidereal tracking] --- Tracks stars.
          Generates stars as points.
          Generates satellite trails.
 	\item [Satellite tracking] --- Tracks satellites.
-         Generates stars as tracks.
+         Generates \glspl{star-trail}.
          Generates satellites as points or potentially larger images
          of the satellite structure.
 \end{description}
 \end{mdframed}
 
 \subsection{Sidereal Tracking Mounts}
-Sidereal tracking (``telescope tracking'') is what \gls{COTS} tracking ``GOTO''
-\glspl{telescope} from Celestron or Sky-Watcher do, for example. They tracks
+\index{track}\index{mount}
+Sidereal tracking (``telescope tracking'') is what \gls{COTS} tracking ``\gls{GoTo}''
+\glspl{telescope} from \gls{Celestron} or Sky-Watcher do, for example. They track
 the stars, countering the rotation of the Earth to keep the same view
-of the sky in the camera's \gls{FOV}. Stars remain as points, even after multi-minute
+of the sky in the camera's \gls{FoV}. Stars remain as points, even after multi-minute
 or multi-hour imaging. This is what is used for ``pretty'' pictures
 of stars, nebula, galaxies, etc. 
 This is the most common tracking set up, as it has been widely used in
 astronomy communities for decades.
 
-
 Within sidereal tracking mounts, there are yet more options:
 
-
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
 	\item [Fork] --- Fork mount.
-	\item [EQ fork] --- Fork on EQ mount.
-	\item [German EQ] --- Most common EQ mount.
-	\item [More] --- Endless variety of available telescope mounts.
+	\item [\gls{EQ} fork] --- Fork on \gls{EQ} mount.
+	\item [German \gls{EQ}] --- Most common \gls{EQ} mount.
+	\item [More] --- Endless variety of available \gls{telescope} mounts.
 \end{description}
 \end{mdframed}
-\index{German EQ}\index{fork} %XXX
+\index{German \gls{EQ}}\index{fork} %XXX
 \index{mount}\index{track}
  
 Also related to sidereal tracking is lunar and planetary
@@ -388,12 +392,13 @@ tracking, but for our uses all three will be included under sidereal tracking.
 
 To use a sidereal tracking mount for imaging satellites, the camera
 must ``leap frog'' the satellite.
-At present, my practice is to use a sidereal mount, point at a location with KStars,
-start stvid. Then stop stvid, move to new location using KStars,
-start stvid.
-\index{track}\index{KStars}\index{stvid}
+At present, my practice is to use a sidereal mount, point at a location with \gls{KStars},
+start \gls{stvid}. Then stop \gls{stvid}, move to new location using \gls{KStars},
+start \gls{stvid}.
+\index{track}\index{camera}
 
-See Software section XXX for information on using tracking mounts.
+See Software section \ref{sec:software-tracking}, \pageref{sec:software-tracking}
+for information on using tracking mounts.
 
 \subsection{Satellite Tracking Mounts}
 \index{track}\index{mount}
@@ -405,38 +410,37 @@ It requires, such as:
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
-	\item [Time] --- Accurate time, such as from \gls{GNSS}.
+	\item [Time] --- Accurate time, such as from \gls{GNSS} or \gls{NTP}.
 	\item [Location] --- Accurate location, also available from \gls{GNSS}.
-	\item [TLE] --- Need to know the \glspl{satellite}' orbit (accurately!).
+	\item [\gls{TLE}] --- Need to know the \glspl{satellite}' orbit (accurately!).
         \item [Variable speed tracking] --- \Glspl{satellite} are moving at different
          speeds above, the mount needs to be capable of that.
-	\item [Human guided] --- Some skilled amateurs track by hand.
 	\item [Alignment] --- On top of all the gear and software needed,
          the equipment needs to be accurately aligned.
 \end{description}
 \end{mdframed}
-\index{GNSS}\index{TLE}
+\index{alignment}\index{track}
 
 Most tracking equipment for \glspl{telescope},
-cameras, and antennas usually has just a few speeds, such as a slewing speed
+cameras, and \glspl{antenna} usually has just a few speeds, such as a \gls{slew} speed
 and a sidereal star tracking speed. Sometimes there will be a few steps
-of these speeds (e.g. slew speeds from 1-9), but not the finely tuned tracking
-speeds needed to track a satellite. Oftentimes the telescope tracking maximum
-speed will be too slow for satellite tracks.
+of these speeds (e.g. \gls{slew} speeds from 1-9), but not the finely tuned tracking
+speeds needed to track a satellite. Oftentimes the \gls{telescope} tracking maximum
+speed will be too slow for satellite tracking.
+\index{track}
 
 Variable speed tracking (XXX phrase?) is needed for tracking satellites if
 the goal is to keep the satellite in the (near) center of the image frame
-and leave star trails. The speed the mount moves needs to be calculated
-based upon a recent orbit calcuation, such as from a \gls{TLE}.
+and leave \glspl{star-trail}. The speed the mount moves needs to be calculated
+based upon a recent \gls{orbit} calcuation, such as from a \gls{TLE}.
 
 There are highly skilled amateur astronomers that have captured detailed
-pictures of artificial satellites, such as the ISS and astronauts doing
-space walks, using hand guided telescopes with low cost \gls{CCD} imagers.
-\index{CCD}\index{ISS}
+pictures of artificial satellites, such as the \gls{ISS} and astronauts doing
+space walks, using hand guided \glspl{telescope} with low cost \gls{CCD} imagers.
 % XXX ref
 
 There are few options for satellite tracking mounts.
-Some new iOptron telescope mount firmware supports tracking
+Some new iOptron \gls{telescope} mount \gls{firmware} supports tracking
 satellites. This has been largely untested so far, but at present
 is likely the best option, if a satellite tracking mount is wanted.
 \index{iOptron}\index{track}\index{mount}
@@ -444,8 +448,9 @@ is likely the best option, if a satellite tracking mount is wanted.
 
 \section{Future Designs}
 \label{sec:hardware-future}
-\index{RASA}\index{telescope}\index{astrograph}
-\index{rotator}\index{antenna}
+
+\index{track}
+\index{camera}
 
 There is some discussion of using much larger ``lenses'', such as
 a \gls{RASA} ``\gls{telescope}'' (See: \gls{astrograph}).

src/Identify.tex

@@ -11,8 +11,7 @@
 
 \section{Overview of Satellite Identification}
 \label{sec:overview-identify}
-\index{identify}\index{SIDLOC}\index{orbit}
-\index{SSA}
+\index{identify}\index{locate}
 
 The \gls{LSF} is developing a project called \gls{SIDLOC},
 for \gls{satellite} identification and localization. With the
@@ -22,11 +21,11 @@ for \gls{SSA}.
 
 \section{\texttt{stvid}'s \texttt{process.py} for Identification}
 \label{sec:process-identify}
-\index{identify}\index{FITS}\index{stvid}\index{process}
+\index{identify}\index{process}
 
 The best tool for identifying \glspl{satellite} from \gls{FITS} files
 is the \texttt{process.py}
-script from \texttt{stvid}, available here:
+script from \texttt{\gls{stvid}}, available here:
 
 * \url{https://github.com/cbassa/stvid}
 
@@ -36,17 +35,15 @@ My fork is here:
 
 
 \section{Identifying Satellites with \texttt{satid}}
-\index{satid}\index{sattools}\index{identify}
-\index{C}\index{Giza}
+\index{identify}\index{Giza}
 
-The deprecated C application, \texttt{satid} from the \texttt{\gls{sattools}}
+The deprecated \gls{C} application, \texttt{satid} from the \texttt{\gls{sattools}}
 package can help identify \glspl{satellite}.
 See figure \ref{fig:satid-giza-3}, page \pageref{fig:satid-giza-3}
 for output from my Giza port of \texttt{\gls{satid}}.%
 \footnote{\url{https://spacecruft.org/spacecruft/sattools/media/branch/spacecruft/img/satid-giza-3.png}}
 \index{Giza}
 
-
 * \url{https://github.com/cbassa/sattools}
 
 My fork is here:
@@ -57,28 +54,183 @@ My fork is here:
 	\begin{center}
 		\includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{satid-giza-3.png}
 		\caption{\texttt{satid} example.}
-		\index{satid}\index{sattools}
 		\label{fig:satid-giza-3}
 	\end{center}
 \end{figure}
 
 
 \section{Identification with stvid}
-\index{identify}\index{stvid}
+\index{identify}
 See section \ref{sec:satellite-detection}, page \pageref{sec:satellite-detection}
-for details on identification with stvid.
+for details on identification with \gls{stvid}.
 The detection and identification steps are both done in one script.
 
 See figure \ref{fig:stvid-process}, page \pageref{fig:stvid-process}
 for an example of from \gls{stvid} automated processing of an input \gls{FITS}
 file. The output image is in \gls{PNG} format.
 \gls{stvid} will also output other files with results, such as \gls{CSV} files.
-\index{stvid}\index{FITS}\index{PNG}\index{CSV}\index{process}
+\index{process}
 
 \begin{sidewaysfigure}[p!]
-        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{stvid-process-0.png}
-        \caption{Satellite images processed by stvid.}
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{stvid/2022-08-23T11:21:34.290.fits.png}
+        \caption{Example satellite image processed by \texttt{stvid}.}
         \label{fig:stvid-process}
-        \index{stvid}\index{process}
+        \index{process}
+\end{sidewaysfigure}
+
+\section{Review of Images}
+
+See the following subsections for example output from \gls{stvid}.
+
+
+\subsection{Unidentified Satellites}
+\index{unidentified}\index{identify}
+When \gls{stvid} runs the \texttt{process.py} (or new) script and
+it encounters a satellite it cannot identify, it gives it the 
+\gls{NORAD-ID} \texttt{90000}. If more unidentified satellites are
+detected in the same image, each detection is incremented by one.
+
+See figure \ref{fig:stvid-unidentified}, page \pageref{fig:stvid-unidentified},
+ for an example image, with three unidentified satellites.
+One is on the left, the other two on the right, next to each other.
+
+See figures \ref{fig:stvid-unidentified-90000}, \ref{fig:stvid-unidentified-90001}, and \ref{fig:stvid-unidentified-90002}, pages \pageref{fig:stvid-unidentified-90000}, \pageref{fig:stvid-unidentified-90001}, and \pageref{fig:stvid-unidentified-90002},
+to see an example of \texttt{\gls{stvid}} labelling three identified satellites
+with \glspl{NORAD-ID} \texttt{90000}, \texttt{90001}, \texttt{90002}.
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{id-new-sats/2022-08-23T11:18:12.531.fits.png}
+        \caption{stvid processed image, with three unidentified satellites.}
+        \label{fig:stvid-unidentified}
+        \index{unidentified}
+\end{sidewaysfigure}
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{id-new-sats/2022-08-23T11:18:12.531_90000_unid.png}
+        \caption{stvid processed image, with three unidentified satellites, the first labeled with NORAD ID \texttt{90000}.}
+        \label{fig:stvid-unidentified-90000}
+        \index{unidentified}
+\end{sidewaysfigure}
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{id-new-sats/2022-08-23T11:18:12.531_90001_unid.png}
+        \caption{stvid processed image, with three unidentified satellites, the second labeled with NORAD ID \texttt{90001}.}
+        \label{fig:stvid-unidentified-90001}
+        \index{unidentified}
+\end{sidewaysfigure}
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{id-new-sats/2022-08-23T11:18:12.531_90002_unid.png}
+        \caption{stvid processed image, with three unidentified satellites, the third labeled with NORAD ID \texttt{90002}.}
+        \label{fig:stvid-unidentified-90002}
+        \index{unidentified}
+\end{sidewaysfigure}
+
+
+\subsection{Airplanes}
+\index{airplane}\index{noise}
+Airplanes are noise in the data.
+
+Airplanes will appear not infrequently in images.
+See figure \ref{fig:stvid-airplane1}, page \pageref{fig:stvid-airplane1}
+for an example with an airplane in the left side, forming two parallel
+trails from the aircrafts' lights.
+
+In figure \ref{fig:stvid-airplane2}, page \pageref{fig:stvid-airplane2},
+is shown an example image with an airplane with a very distinct blinking light.
+ 
+In figure \ref{fig:stvid-airplane3}, page \pageref{fig:stvid-airplane3},
+airplane solid parallel trails can be seen with blinking lights.
+ 
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{airplane/2022-08-23T04:17:27.161.fits.png}
+        \caption{Airplane, bold left side, in stvid processed image.}
+        \label{fig:stvid-airplane1}
+        \index{airplane}
+\end{sidewaysfigure}
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{airplane/2022-08-24T03:05:30.370.fits.png}
+        \caption{Airplane, blinking, in stvid processed image.}
+        \label{fig:stvid-airplane2}
+        \index{airplane}
+\end{sidewaysfigure}
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{airplane/2022-08-24T09:18:02.277.fits.png}
+        \caption{Airplane, two solid lights plus blinking, in stvid processed image.}
+        \label{fig:stvid-airplane3}
+        \index{airplane}
+\end{sidewaysfigure}
+
+
+\subsection{Configuration and Setup Errors in Images}
+\index{process}\index{identify}
+
+See figure \ref{fig:stvid-misconfigured}, page \pageref{fig:stvid-misconfigured},
+for an example of an image processed by a mis-configured system.
+As can be seen, the plotted lines are offset from the actual images of satellites.
+This, and similar issues, can be addressed by checking:
+
+\begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
+\begin{itemize}
+  \item Recent \glspl{TLE} on both the processing workstation and the
+   \gls{embedded-system}.
+  \item Correct, \gls{NTP} (or better) synchronized time on on the processing
+   workstation and the \gls{embedded-system}.
+  \item Correct latitude, longitude, and altitude are set in configuration
+   files, typically based on \gls{GNSS} readings.
+   \index{latitude}\index{longitude}\index{altitude}
+\end{itemize}
+\end{mdframed}
+
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{stvid/2022-08-25T03\:40\:03.853.fits.png}
+        \caption{\texttt{stvid} processed image, showing mis-configured/setup system.}
+        \label{fig:stvid-misconfigured}
+        \index{airplane}
+\end{sidewaysfigure}
+
+\subsection{Image Processed with Bad TLE}
+In figure \ref{fig:stvid-process-bad-tle}, page \pageref{fig:stvid-process-bad-tle},
+can be seen a \gls{FITS} file that has been processed by stvid, but with \glspl{TLE}
+that are around two days old. As can be seen, the satellites don't quite line up
+where they should.
+
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{stvid/2022-09-04T03:40:07.923.fits.png}
+        \caption{\texttt{stvid} processed image, alignment off due to use of old TLE.}
+        \label{fig:stvid-process-bad-tle}
+\end{sidewaysfigure}
+
+\subsection{Image Acquired During Slew}
+\index{acquire}
+
+See figured \ref{fig:stvid-process-bad-slew}, page \pageref{fig:stvid-process-bad-slew},
+for an example image that is bad due to \gls{slew}[ing] during acquisition.
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{stvid/2022-09-04T04\:56\:37.072.fits.png}
+        \caption{\texttt{stvid} processed image, trails due to slewing during acquire.}
+        \label{fig:stvid-process-bad-slew}
+\end{sidewaysfigure}
+
+\subsection{Light Outside FoV Artifact}
+\index{acquire}
+
+See figured \ref{fig:stvid-light-fov}, page \pageref{fig:stvid-light-fov},
+for an example of an artifact, visible crossing the left and center,
+generated by light outside the \gls{FoV}, in
+this case the moon!%
+\footnote{Pierros in SatNOGS Optical Matrix}
+This is also an example image that detects classified satellites.
+This is how the main upstream \texttt{\gls{stvid}} works.
+
+\begin{sidewaysfigure}[p!]
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{stvid/stvid-light-fov.png}
+        \caption{\texttt{stvid} processed image, with classified satellites and light artifact.}
+        \label{fig:stvid-light-fov}
 \end{sidewaysfigure}
 

src/Introduction.tex

@@ -11,7 +11,6 @@
 
 The SatNOGS Optical Unofficial Guide documents how to set up and run an
 \gls{optical-ground-station} for the \gls{LSF}'s \gls{SatNOGS} network.
-\index{ground station}
 
 % https://network.satnogs.org/
 \begin{figure}[h!]
@@ -20,7 +19,6 @@ The SatNOGS Optical Unofficial Guide documents how to set up and run an
 	\includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{satnogs-network-web.png}
 	\caption{SatNOGS Network.}
 	\label{fig:satnogs-network-web}
-	\index{SatNOGS}
 	\end{framed}
 \end{figure}
 
@@ -28,42 +26,42 @@ The SatNOGS Optical Unofficial Guide documents how to set up and run an
 \section{Unofficial Guide Overview}
 First,  an overview of the this text, then the \gls{LSF}
 and some of it's key projects, such as the \gls{SatNOGS} network.
-A cursory review of \glspl{satellite} and existing \gls{RF} ground stations
+A cursory review of \glspl{satellite} and existing \gls{RF} \glspl{ground-station}
 will be followed by a big picture view of acquiring and processing
 images of \glspl{satellite}. Hardware is reviewed, then software to run
 on it, with many options, including what is best. Finally,
-what to do with the data (idk!).
+what to do with the data.
 The chapters that follow are listed below.
-\index{RF}
+
 
 % Perhaps more LaTeXy ref XXX
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
   \item [\Glspl{satellite}] --- What are we looking at?
-  \item [Ground Stations] --- How Earth talks to \glspl{satellite} and back.
-  \item [Toolchain and Process] --- The big picture of what
-   hardware and software is needed to set up an optical ground station
-   for use on the distributed network.
+  \item [\Glspl{ground-station}] --- How Earth talks to \glspl{satellite} and back.
+  \item [\Gls{toolchain} and Process] --- The big picture of what
+   hardware and software is needed to set up an \gls{optical-ground-station}
+   for use on the network.
   \item [Hardware] --- Details on appropriate hardware configurations,
    and example setups.
   \item [Software] --- A look at the myriad software related to \glspl{satellite},
-   and what works best at present for SatNOGS Optical.
-  \item [Acquire] --- Convert photons to bits. Pointing a camera at the
-   sky works.
+   and what works best at present for \gls{SatNOGS-Optical}.
+  \item [Acquire] --- Convert \glspl{photon} to bits. Pointing a camera at the
+   sky works.\index{camera}
   \item [Solve] --- Pictures of stars reveal the time and location of
-   the photo. Plate solvers reviewed.
-  \item [Detect] --- The plate solver says where the photo is,
-   now detect if are there moving tracks that aren't stars that could
+   the photo. \Glspl{plate-solver} reviewed.
+  \item [Detect] --- The \gls{plate-solver} says where the photo is,
+   now detect if are there moving trails that aren't \glspl{star-trail} that could
    be \glspl{satellite}.
   \item [Identify] --- With time, location, \gls{satellite} detection, \glspl{TLE}
-   are overlaid and compared with detected \glspl{satellite}.
+   are overlaid and compared with detected \glspl{satellite}.\index{identify}
    \Gls{satellite} identification by computers and humans.
-  \item [Upload] --- When ready, data will be pushed to the SatNOGS network.
+  \item [Upload] --- When ready, data will be pushed to the \gls{SatNOGS} network.
   \item [Support] --- Where development is occurring and questions answered!
 \end{description}
 \end{mdframed}
-\index{ground station}\index{process}\index{hardware}\index{software}
-\index{acquire}\index{solve}\index{detect}\index{identify}\index{upload}
+\index{process}\index{hardware}\index{software}
+\index{acquire}\index{detect}\index{identify}\index{upload}
 \index{support}
 
 
@@ -71,7 +69,6 @@ The chapters that follow are listed below.
 The \gls{LSF} supports
 ``free and accessible space for all, creating \gls{open-source} space technologies.''%
 \footnote{\url{https://libre.space}}
-\index{Open Source}
 
 \begin{figure}[h!]
 	\begin{framed}
@@ -79,7 +76,6 @@ The \gls{LSF} supports
 	\includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{lsf-web.png}
 	\caption{Libre Space Foundation Website.}
 	\label{fig:lsf-web}
-	\index{Libre Space Foundation}
 	\end{framed}
 \end{figure}
 
@@ -97,8 +93,7 @@ Select \gls{LSF} projects:
 
 
 \section{SatNOGS Network}
-SatNOGS is the \gls{LSF}'s global network of \gls{satellite} ground stations.
-\index{ground station}
+\gls{SatNOGS} is the \gls{LSF}'s global network of \gls{satellite} ground stations.
 
 \begin{figure}[h!]
 	\begin{framed}
@@ -106,20 +101,17 @@ SatNOGS is the \gls{LSF}'s global network of \gls{satellite} ground stations.
 	\includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{satnogs-web.png}
 	\caption{SatNOGS Website.}
 	\label{fig:satnogs-web}
-	\index{SatNOGS}
 	\end{framed}
 \end{figure}
 
 
-\section{Network Status}
-\index{RF}
-The SatNOGS \gls{RF} network has been running successfully for years.
-Adding an optical network is a new development. At present there
+\section{Optical Network Status}
+The \gls{SatNOGS} \gls{RF} network has been running successfully for years.
+Adding a \gls{SatNOGS-Optical} network is a new development. At present there
 are zero nodes on the network.
 
 Some software already exists,
 some is being ported from \gls{C} to \gls{Python}, and other parts remain to be done.
 There is software available for acquiring optical data of \glspl{satellite}.
 There is no facility at present for pushing data back to the network.
-\index{C}\index{Python}
 

src/Makefile

@@ -1,6 +1,29 @@
 # Makefile
 
 all:
+	xelatex								\
+		-halt-on-error						\
+		-shell-escape						\
+		-interaction=nonstopmode				\
+		-no-pdf							\
+		SNOUG.tex
+	biber SNOUG
+	#makeglossaries SNOUG
+	bib2gls SNOUG
+	xelatex								\
+		-halt-on-error						\
+		-shell-escape						\
+		-interaction=nonstopmode				\
+		-no-pdf							\
+		SNOUG.tex
+	bib2gls SNOUG
+	xelatex								\
+		-halt-on-error						\
+		-shell-escape						\
+		-interaction=nonstopmode				\
+		-no-pdf							\
+		SNOUG.tex
+	bib2gls SNOUG
 	xelatex								\
 		-halt-on-error						\
 		-shell-escape						\
@@ -21,7 +44,6 @@ all:
 		-no-pdf							\
 		SNOUG.tex
 	makeindex SNOUG
-	biber SNOUG
 	xelatex								\
 		-halt-on-error						\
 		-shell-escape						\
@@ -34,9 +56,18 @@ all:
 		-interaction=nonstopmode				\
 		SNOUG.tex
 
+cover:
+	xelatex								\
+		-halt-on-error						\
+		-shell-escape						\
+		-interaction=nonstopmode				\
+		Cover.tex
+
 clean:
 	rm -fr _minted-*
 	rm -f *.aux
+	rm -f *.bib.bak
+	rm -f *.bib.sav.tmp
 	rm -f *.bbl
 	rm -f *.bcf
 	rm -f *.blg

src/SNOUG.bib

@@ -334,4 +334,293 @@
   year             = {2021},
 }
 
+@Misc{enwiki:OpenCV,
+  author           = {{Wikipedia contributors}},
+  title            = {OpenCV --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=OpenCV&oldid=1106133881}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:19:29},
+  year             = {2022},
+}
+
+@Misc{enwiki:KStars,
+  author           = {{Wikipedia contributors}},
+  title            = {KStars --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=KStars&oldid=1076667045}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:22:15},
+  year             = {2022},
+}
+
+@Misc{enwiki:GPhoto,
+  author           = {{Wikipedia contributors}},
+  title            = {GPhoto --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=GPhoto&oldid=1097546275}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:24:39},
+  year             = {2022},
+}
+
+@Misc{enwiki:Raspberry_Pi,
+  author           = {{Wikipedia contributors}},
+  date             = {2022},
+  title            = {Raspberry Pi --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Raspberry_Pi&oldid=1107949674}},
+  note             = {[Online; accessed 2-September-2022]},
+  creationdate     = {2022-09-02T16:27:31},
+  modificationdate = {2022-09-02T16:28:44},
+}
+
+@Misc{enwiki:Celestron,
+  author           = {{Wikipedia contributors}},
+  title            = {Celestron --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Celestron&oldid=1091418493}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:30:20},
+  year             = {2022},
+}
+
+@Misc{enwiki:Amateur_radio,
+  author           = {{Wikipedia contributors}},
+  title            = {Amateur radio --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Amateur_radio&oldid=1106068703}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:32:33},
+  year             = {2022},
+}
+
+@Misc{enwiki:Firmware,
+  author           = {{Wikipedia contributors}},
+  title            = {Firmware --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Firmware&oldid=1099439511}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:34:39},
+  year             = {2022},
+}
+
+@Misc{enwiki:Gpsd,
+  author           = {{Wikipedia contributors}},
+  title            = {Gpsd --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Gpsd&oldid=1076207218}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:37:29},
+  year             = {2022},
+}
+
+@Misc{enwiki:Star_catalogue,
+  author           = {{Wikipedia contributors}},
+  title            = {Star catalogue --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Star_catalogue&oldid=1107326057}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:41:17},
+  year             = {2022},
+}
+
+@Misc{enwiki:Star_chart,
+  author           = {{Wikipedia contributors}},
+  title            = {Star chart --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Star_chart&oldid=1106250278}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:42:48},
+  year             = {2022},
+}
+
+@Misc{enwiki:Astronomical_catalog,
+  author           = {{Wikipedia contributors}},
+  title            = {Astronomical catalog --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Astronomical_catalog&oldid=1035999452}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:45:11},
+  year             = {2021},
+}
+
+@Misc{enwiki:Unix,
+  author           = {{Wikipedia contributors}},
+  title            = {Unix --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Unix&oldid=1105826457}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:47:07},
+  year             = {2022},
+}
+
+@Misc{enwiki:Appropriate_technology,
+  author           = {{Wikipedia contributors}},
+  title            = {Appropriate technology --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Appropriate_technology&oldid=1104787534}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:50:21},
+  year             = {2022},
+}
+
+@Misc{enwiki:Linux_distribution,
+  author           = {{Wikipedia contributors}},
+  title            = {Linux distribution --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Linux_distribution&oldid=1107830099}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:53:59},
+  year             = {2022},
+}
+
+@Misc{enwiki:Lagrange_point,
+  author           = {{Wikipedia contributors}},
+  title            = {Lagrange point --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Lagrange_point&oldid=1102894784}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:56:19},
+  year             = {2022},
+}
+
+@Misc{enwiki:GoTo_telescopes,
+  author           = {{Wikipedia contributors}},
+  title            = {GoTo (telescopes) --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=GoTo_(telescopes)&oldid=841595201}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T16:59:02},
+  year             = {2018},
+}
+
+@Misc{enwiki:Slewing,
+  author           = {{Wikipedia contributors}},
+  title            = {Slewing --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Slewing&oldid=1061997651}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T17:02:10},
+  year             = {2021},
+}
+
+@Misc{enwiki:Toolchain,
+  author           = {{Wikipedia contributors}},
+  title            = {Toolchain --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Toolchain&oldid=1094527160}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T17:11:55},
+  year             = {2022},
+}
+
+@Misc{enwiki:Pipeline_computing,
+  author           = {{Wikipedia contributors}},
+  title            = {Pipeline (computing) --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Pipeline_(computing)&oldid=1096885455}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T17:14:10},
+  year             = {2022},
+}
+
+@Misc{enwiki:Embedded_system,
+  author           = {{Wikipedia contributors}},
+  title            = {Embedded system --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Embedded_system&oldid=1106874216}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T17:19:17},
+  year             = {2022},
+}
+
+@Misc{enwiki:Star_trail,
+  author           = {{Wikipedia contributors}},
+  title            = {Star trail --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Star_trail&oldid=1075094531}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T17:30:14},
+  year             = {2022},
+}
+
+@Misc{enwiki:Satellite_flare,
+  author           = {{Wikipedia contributors}},
+  title            = {Satellite flare --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Satellite_flare&oldid=1104678552}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T17:34:00},
+  year             = {2022},
+}
+
+@Misc{enwiki:Photon,
+  author           = {{Wikipedia contributors}},
+  title            = {Photon --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Photon&oldid=1104709214}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T17:43:30},
+  year             = {2022},
+}
+
+@Misc{enwiki:Software_repository,
+  author           = {{Wikipedia contributors}},
+  title            = {Software repository --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Software_repository&oldid=1081326130}},
+  note             = {[Online; accessed 2-September-2022]},
+  modificationdate = {2022-09-02T17:55:58},
+  year             = {2022},
+}
+
+@Misc{enwiki:Upstream,
+  author           = {{Wikipedia contributors}},
+  title            = {Upstream (software development) --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Upstream_(software_development)&oldid=1066370459}},
+  note             = {[Online; accessed 3-September-2022]},
+  modificationdate = {2022-09-02T18:05:06},
+  year             = {2022},
+}
+
+@Misc{enwiki:Daemon,
+  author           = {{Wikipedia contributors}},
+  title            = {Daimon (disambiguation) --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Daimon_(disambiguation)&oldid=1069803376}},
+  note             = {[Online; accessed 3-September-2022]},
+  modificationdate = {2022-09-02T18:16:56},
+  year             = {2022},
+}
+
+@Misc{enwiki:Operating_system,
+  author           = {{Wikipedia contributors}},
+  title            = {Operating system --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Operating_system&oldid=1104687084}},
+  note             = {[Online; accessed 3-September-2022]},
+  modificationdate = {2022-09-02T18:19:06},
+  year             = {2022},
+}
+
+@Misc{enwiki:Teledyne_FLIR,
+  author           = {{Wikipedia contributors}},
+  title            = {Teledyne FLIR --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Teledyne_FLIR&oldid=1102704879}},
+  note             = {[Online; accessed 3-September-2022]},
+  modificationdate = {2022-09-02T22:23:54},
+  year             = {2022},
+}
+
+@Misc{enwiki:Ultrasonic_motor,
+  author           = {{Wikipedia contributors}},
+  title            = {Ultrasonic motor --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Ultrasonic_motor&oldid=1099892445}},
+  note             = {[Online; accessed 4-September-2022]},
+  modificationdate = {2022-09-03T19:30:07},
+  year             = {2022},
+}
+
+@Misc{enwiki:Satellite_Catalog_Number,
+  author           = {{Wikipedia contributors}},
+  title            = {Satellite Catalog Number --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Satellite_Catalog_Number&oldid=1100318368}},
+  note             = {[Online; accessed 4-September-2022]},
+  modificationdate = {2022-09-03T20:57:59},
+  year             = {2022},
+}
+
+@Misc{enwiki:Docker,
+  author           = {{Wikipedia contributors}},
+  title            = {Docker (software) --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Docker_(software)&oldid=1108127182}},
+  note             = {[Online; accessed 4-September-2022]},
+  modificationdate = {2022-09-04T17:25:07},
+  year             = {2022},
+}
+
+@Misc{enwiki:Pixel_binning,
+  author           = {{Wikipedia contributors}},
+  title            = {Pixel binning --- {Wikipedia}{,} The Free Encyclopedia},
+  howpublished     = {\url{https://en.wikipedia.org/w/index.php?title=Pixel_binning&oldid=1085651660}},
+  note             = {[Online; accessed 4-September-2022]},
+  modificationdate = {2022-09-04T17:53:02},
+  year             = {2022},
+}
+
 @Comment{jabref-meta: databaseType:biblatex;}

src/SNOUG.tex

@@ -79,7 +79,6 @@ leftmargin=1cm,rightmargin=1cm
 \setmonofont{LMMono12-Regular}
 % Linux Biolinum
 \setsansfont[Ligatures=TeX]{Linux Biolinum O}
-
 %%% END PREAMBLE FONTS %%%
 
 %%% MISC %%%
@@ -216,11 +215,137 @@ leftmargin=1cm,rightmargin=1cm
 %%% END INDEX %%%
 
 %%% GLOSSARY %%%
-\usepackage[toc,indexcrossrefs,translate=babel,nopostdot=true,nonumberlist,nogroupskip]{glossaries-extra}
-\GlsXtrLoadResources
-\setabbreviationstyle[acronym]{short-long}
-\loadglsentries{Glossary}
-\makenoidxglossaries
+\let\printindex\relax % or conflicts with memoir
+
+\usepackage[
+	automake, % Automatically create glossary files when compiling
+	acronyms, % Allow the use of acronyms as a separate glossary type
+	abbreviations, % Allow the use of abbreviations as a separate glossary type
+	nonumberlist,record=hybrid,index,toc,indexcrossrefs,translate=babel, % TODO comment what each of these does
+]{glossaries-extra}
+
+%%% Multiple Columns (Abbreviations)
+\usepackage{glossary-mcols}
+
+\renewcommand{\abbreviationsname}{List of Abbreviations} % Change the default name of the abbreviations
+
+\makeindex
+
+% Specify the in-text glossary abbreviation style for each glossary type
+\setabbreviationstyle{long-short}
+\setabbreviationstyle[acronym]{long-short} % The first time an acronym is used in text, display it as <long> (<short>), e.g. "Network Time Protocol (NTP)"
+
+% Load all glossary type entries from separate .bib files. Acronyms and abbreviations are input using @dual<acronym/abbreviation> entries which the code below duplicates and puts into 2 separate glossary types: 1) acronym/abbreviation and 2) main. The former populate the acronyms/abbreviations and the latter populates the main glossary.
+% Main glossary
+\GlsXtrLoadResources[
+	src={Glossary.bib},
+	sort={en-US}, % Default sorting
+	type=main, % Glossary type of main (primary) entries (e.g. @entry)
+	dual-sort={combine}, % TODO this should be working but it's not >_< it also doesn't work in \GlsXtrLoadResources for the main glossary where it might need to go instead
+	dual-sort-field={sort}, % TODO not working
+]
+% Acronyms
+\GlsXtrLoadResources[
+	src={Acronyms.bib}, % Source bib file containing acronym entries
+	sort={letter-nocase}, % Default sorting
+	type=acronym, % Glossary type of main (primary) entries (e.g. @acronym)
+	dual-type=main, % Glossary type of dual (secondary) entries, dual entries are only created with @dual* entries in the .bib file
+	dual-abbrv-map={{long}, {name}}, % Map the long field in the @dualacronym entry to the name field used in the main glossary
+	abbreviation-sort-fallback={name}, % Sort entries by the long field (check this in .glstex by looking at the dual entry sort= values)
+	dual-sort={combine}, % TODO this should be working but it's not >_< it also doesn't work in \GlsXtrLoadResources for the main glossary where it might need to go instead
+	dual-sort-field={sort}, % TODO not working
+]
+% Abbreviations
+\GlsXtrLoadResources[
+	src={Abbreviations.bib}, % Source bib file containing abbreviations entries
+	sort={letter-nocase}, % Default sorting
+	type=abbreviations, % Glossary type of main (primary) entries (e.g. @abbreviation)
+	dual-type=main, % Glossary type of dual (secondary) entries, dual entries are only created with @dual* entries in the .bib file
+	dual-abbrv-map={{long}, {name}}, % Map the long field in the @dualabbreviation entry to the name field used in the main glossary
+	abbreviation-sort-fallback={name}, % Sort entries by the long field (check this in .glstex by looking at the dual entry sort= values)
+	dual-sort={combine}, % TODO this should be working but it's not >_< it also doesn't work in \GlsXtrLoadResources for the main glossary where it might need to go instead
+	dual-sort-field={sort}, % TODO not working
+]
+% Another approach that uses just the normal @abbreviation and @acronym entries but doesn't format entries in the main glossary correctly
+%\GlsXtrLoadResources[
+%	src={Glossary.bib},
+%	sort={en-US}, % Default sorting
+%	type=main, % Glossary type of main (primary) entries (e.g. @entry)
+%]
+%% Acronyms
+%\GlsXtrLoadResources[
+%	src={Acronyms.bib}, % Source bib file containing acronym entries
+%	sort={letter-nocase}, % Default sorting
+%	type=acronym, % Glossary type of main (primary) entries (e.g. @acronym)
+%	secondary={en-US:long:main},
+%]
+%% Abbreviations
+%\GlsXtrLoadResources[
+%	src={Abbreviations.bib}, % Source bib file containing abbreviations entries
+%	sort={letter-nocase}, % Default sorting
+%	type=abbreviations, % Glossary type of main (primary) entries (e.g. @abbreviation)
+%	secondary={en-US:long:main},
+%]
+
+\GlsXtrEnableIndexFormatOverride
+
+\glsdefpostname{acronym}{ (\glsentryshort{\glscurrententrylabel})} % Add " (<short>) to acronym entries in the main glossary
+\glsdefpostname{abbreviation}{ (\glsentryshort{\glscurrententrylabel})} % Add " (<short>) to abbreviation entries in the main glossary
+
+% Define a new glossary style that outputs short and long fields from glossary entries in a description list environment
+\newglossarystyle{shortlongglossary}{%
+	% Put glossary entries into a description environment
+	\renewenvironment{theglossary}{
+		\begin{multicols}{2}
+		\begin{description}
+	}{
+		\end{description}
+		\end{multicols}
+	}%
+	% Define which fields are output for each glossary entry
+	\renewcommand*{\glossentry}[2]{%
+		\item[\glstarget{##1}{\glsentryshort{##1}}] \glsentrylong{##1} % Each glossary entry is output as a description item in the format: \item[<short>] <long>
+	}%
+}
+
+% Adds acronym to index like:
+% World Coordinate System (WCS), 67, 116
+% Adds glossary to index like:
+% photon, xii
+\renewcommand*{\glsxtrautoindexentry}[1]{%
+  \ifglshasshort{#1}%
+  {\string\glsentrylong{#1} (\glsentryshort{#1})}%
+  {\string\glsentrylong{#1}}%
+}
+
+% use long form for the sort value in the index, if provided:
+\renewcommand*{\glsxtrautoindexassignsort}[2]{%
+  \ifglshaslong{#2}%
+  {\glsletentryfield{#1}{#2}{long}}%
+  {\glsletentryfield{#1}{#2}{sort}}%
+}
+
+% OK, ACRONYM shows description, then short.
+% Showshort first better.
+% Shows both when desc=long, only one needed...
+% OK, but me. XXX borken?
+%\glsdefpostname{acronym}{TEST} % This outputs something after the name, e.g. NTPTEST
+%\renewcommand*{\glsxtrpostdescacronym}{\glsentrylong{\glscurrententrylabel}} % This outputs something after the description
+
+% crossref for see:
+\renewcommand*{\glsxtrpostdescgeneral}{%
+\ifglshasfield{see}{\glscurrententrylabel}
+{, \glsxtrusesee{\glscurrententrylabel}}%
+{}%
+}
+
+% Index glossary, abbreviations, acronyms
+\glssetcategoryattribute{general}{dualindex}{hyperpage}
+\glssetcategoryattribute{abbreviation}{dualindex}{hyperpage}
+\glssetcategoryattribute{acronym}{dualindex}{hyperpage}
+
+% First letter upper
+%\glssetcategoryattribute{general}{glossname}{firstuc}
 %%% END GLOSSARY %%%
 
 %%% DEBUG %%%
@@ -333,6 +458,10 @@ leftmargin=1cm,rightmargin=1cm
 %\include{Acknowledgements}
 %%% END ACKNOWLEDGEMENTS PAGE %%%
 
+%%% ACRONYM %%%
+\printunsrtglossary[type={acronym}, style={shortlongglossary}]
+%%% END ACRONYM %%%
+
 % Format:
 % \chapterconf{Name of file to include}{Title of Chapter}
 \chapterconf{Introduction}{Introduction}{SatNOGS Optical}
@@ -361,11 +490,10 @@ leftmargin=1cm,rightmargin=1cm
 \chapterconf{Solve}{Plate Solvers}{Place from Pixels}
 \chapterconf{Detect}{Detect}{Find Satellites}
 \chapterconf{Identify}{Identify}{More Than Just Old Rocket Bodies}
-\chapterconf{Upload}{Upload}{Send Data to the SatNOGS Network}
+\chapterconf{Upload}{Upload \& Share}{Send Data to the SatNOGS Network}
 \chapterconf{Support}{Support}{Help!}
 \chapterconf{Contact}{Contact}{Email, Chat, Forum}
 %% END MAINMATTER CHAPTERS %%%
-% Hardware, Software, Acquire, Plate Solver, Detect, Identify
 
 %%% END MAINMATTER %%%
 
@@ -377,11 +505,12 @@ leftmargin=1cm,rightmargin=1cm
 %\chapterconf{Appendix}{Appendix}{Even More for Free}
 %%% END APPENDIX %%%
 
+%%% ABBREVIATIONS %%%
+\printunsrtglossary[type={abbreviations}, style={shortlongglossary}]
+%%% END ABBREVIATIONS %%%
+
 %%% GLOSSARY %%%
-% Set font for glossary word.
-%\renewcommand*{\glsnamefont}[1]{\fontspec{GemunuLibre-Bold.otf}{#1}}
-\clearpage
-\printnoidxglossaries
+\printunsrtglossary[type={main}, style={indexgroup}]
 %%% END GLOSSARY %%%
 
 %%% BIBLIOGRAPHY %%%

src/SatNOGS_Optical.tex

@@ -12,16 +12,15 @@
 \label{sec:optical-howto}
 
 \gls{SatNOGS-Optical} is the nascent distributed network of optical
-ground stations.
+\glspl{ground-station}.
 
 This chapter gives a top level review what is needed in terms of hardware and
-software to build an operating optical ground station.
-\index{hardware}\index{software}\index{ground station}
+software to build an operating optical \gls{ground-station}.
+\index{hardware}\index{software}
 
 
 \section{Toolchain}
 \label{sec:toolchain}
-\index{toolchain}
 
 See below for a \gls{SatNOGS-Optical} Process Overview.%
 \footnote{\url{https://spacecruft.org/spacecruft/SNOPO}}
@@ -29,7 +28,7 @@ See figure \ref{fig:snopo}, page \pageref{fig:snopo}, described below.
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
-  \item [Hardware] --- Hardware, such as cameras and computers, is to be selected and set up.
+  \item [Hardware] --- Hardware, such as cameras and \glspl{embedded-system}, is to be selected and set up.
   \item [Software] --- The best currently available software is to be downloaded, installed, and configured.
   \item [Acquire] --- Data samples, typically in the form of \gls{FITS} file photographs, need to be acquired by running a camera outside at night taking pictures of the sky.
   \item [\Gls{plate-solver}] --- Acquired data samples in \gls{FITS} files need to be processed by a \gls{plate-solver}. See section \ref{sec:plate-solver}, page \pageref{sec:plate-solver}.
@@ -38,11 +37,12 @@ See figure \ref{fig:snopo}, page \pageref{fig:snopo}, described below.
 \end{description}
 \end{mdframed}
 \index{hardware}\index{software}\index{acquire}\index{detect}\index{identify}
+\index{camera}
 
 \begin{sidewaysfigure}[p!]
 	\begin{center}
 	\includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{SNOPO.png}
-	\caption{SatNOGS Optical Process Overview}
+	\caption{\gls{SatNOGS-Optical} Process Overview}
 	\label{fig:snopo}
 	\index{process}
 	\end{center}
@@ -55,8 +55,9 @@ See figure \ref{fig:snopo}, page \pageref{fig:snopo}, described below.
 Discussed in this section are some of the hardware options to be
 explored. More explicit instructions of a particular hardware installation
 can be see in section \ref{sec:hardware-overview}, page \pageref{sec:hardware-overview}.
-Discussed below are camera options, for details on computers and other parts,
+Discussed below are camera options, for details on \glspl{embedded-system} and other parts,
 also see hardware in section \ref{sec:hardware-overview}, page \pageref{sec:hardware-overview}
+\index{camera}
 
 For the purposes here, there are three main categories of hardware. Depending which
 category of equipment is selected, it impacts everything else, such as the
@@ -74,7 +75,7 @@ software used. Main categories:
 Different types of equipment can be used in different categories.
 Some can be used in multiple setups, most just in one.
 If available, using motion video cameras will work best for
-detecting \glspl{satellite} with the developing \gls{SatNOGS} toolchain.
+detecting \glspl{satellite} with the developing \gls{SatNOGS} \gls{toolchain}.
 Examples of motion video camera sources that could be used:
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
@@ -82,24 +83,22 @@ Examples of motion video camera sources that could be used:
   \item [The Imaging Source Cameras based on IMX174] --- Known to work. Recommended.
    High quality cameras, believed to be usable following \gls{DFSG}.
   \item [ZWO ASI based on IMX174] --- Known to work. Not \gls{DFSG} compatible.
-   Uses proprietary SDK. Currently in prototype development.
-  \item [UVC/Video4Linux2] --- ``Any'' video camera that works with the \gls{Linux} kernel.
+   Uses proprietary \gls{SDK}. Currently in prototype development. \index{proprietary}
+  \item [\gls{UVC}/\gls{V4L2}] --- ``Any'' video camera that works with the \gls{Linux} kernel.
    Typically, the device will appear similar to \texttt{/dev/video0}. A camera
    that works with the software isn't necessarily sensitive enough to detect
    satellites, however, as most are designed for brighter environments.
-  \item [OpenCV] --- Devices that work with OpenCV can be used, same as UVC.
+  \item [\gls{OpenCV}] --- cameras that work with \gls{OpenCV} can be used, same as \gls{UVC}.
    To work well, they need to be sensitive.
-  \item [Raspberry Pi] --- The PiCamera can be used. A good lower cost option.
-   Recommended. Many non-Raspberry Pi devices, such as Odroid are also compatible with the Pi
-   MIPI interface.
+  \item [\gls{Raspberry-Pi}] --- The PiCamera can be used. A good lower cost option.
+   Recommended. Many non-\gls{Raspberry-Pi} devices, such as Odroid are also compatible with the Pi
+   \gls{MIPI} interface.\index{PiCamera}\index{Odroid}
 \end{description}
 \end{mdframed}
-\index{The Imaging Source}\index{ZWO ASI}\index{UVC}\index{V4L2}\index{OpenCV}
-\index{Raspberry Pi}\index{Odroid}\index{MIPI}
+\index{The Imaging Source}\index{ZWO ASI}
 
-Still cameras can also be used productively. The current \gls{Python} toolchain
+Still cameras can also be used productively. The current \gls{Python} \gls{toolchain}
 is in very early development and not completely usable yet.
-\index{Python}
 
 See the list below for still camera options:
 
@@ -107,7 +106,7 @@ See the list below for still camera options:
 \begin{description}
   \item [\Glspl{telescope}] --- Can definitely take images of \glspl{satellite}.
   Not the best tool at present, as it isn't well integrated into the \gls{SatNOGS-Optical} toolchain.
-  The \gls{FOV} is generally too small. The mounts are optimized for
+  The \gls{FoV} is generally too small. The mounts are optimized for
   different types of tracking than satellites. This is changing, and longer
   term could be well-supported. Using \gls{RASA} style \glspl{astrograph}
   is likely the best option.
@@ -116,17 +115,17 @@ See the list below for still camera options:
   Cannot be used directly with the current developing \gls{SatNOGS} toolchain.
   It is not seen as the future path forward as it isn't well optimized for
   \gls{SatNOGS-Optical} usage. That said, it is very useful at present for
-  running a tracking mount with KStars and Ekos, for example,
+  running a tracking mount with \gls{KStars} and Ekos, for example,
   in lieu of a better option. Camera software in the \gls{INDI} platform typically
   produce image \gls{FITS} files.
-  \item [gphoto] --- The \gls{Linux} kernel recognizes many cameras that can be
-  used with gphoto tools and drivers, available in \gls{Debian}.
+  \item [\gls{gPhoto}] --- The \gls{Linux} kernel recognizes many cameras that can be
+  used with \gls{gPhoto} tools and drivers, available in \gls{Debian}.
   This is the recommended option at present for still cameras.
   \gls{DSLR} cameras, such as from major manufacturers Canon and Nikon, are
-  used with gphoto.
+  used with \gls{gPhoto}.
 \end{description}
 \end{mdframed}
-\index{telescope}\index{INDI}\index{gphoto}\index{DSLR}
+\index{Ekos}\index{track}\index{mount}\index{Canon}\index{Nikon}
 
 Considering the hardware options above, they need to be matched with
 corresponding software. Not all options work (at all), and some cannot be
@@ -137,7 +136,7 @@ There are also broader ``paths'' that need to be considered:
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
   \item [\gls{sattools}] --- Deprecated because it is in \gls{C}, and the
-    decision was made to move forward with applications primarily
+    decision by upstream and the \gls{LSF} was made to move forward with applications primarily
     written in \gls{Python}. \Gls{sattools} is the most complete toolkit,
     however, so no matter what path is chosen, some parts of it will likely
     be used for now. It can be used with motion video cameras and
@@ -151,19 +150,18 @@ There are also broader ``paths'' that need to be considered:
     \gls{SatNOGS-Optical} project will likely use in the future
     for still cameras.
     It is in very early development, but can acquire data (take photos)
-    with gphoto-compatible cameras.
+    with \gls{gPhoto}-compatible cameras.
   \item [\texttt{asm}] --- All Sky Monitor for taking pictures of all, or nearly all
     of the sky, such as with a 150 or 180 degree view. The \texttt{asm}
     application is in pre-development, but is in \gls{Python} and could be
     the basis for future \gls{SatNOGS-Optical} development.
     The difficulty with all sky cameras is the \gls{plate-solver} isn't
     written to use images from the ``fish-eye'' view of an all sky camera. 
-  \item [Other] --- There are many other satellite and telescope software
+  \item [Other] --- There are many other satellite and \gls{telescope} software
     packges freely available on the Internet. Perhaps some could be adapted for
     usage.
 \end{description}
 \end{mdframed}
-\index{sattools}\index{Python}\index{C}\index{stvid}\index{motion video}
+\index{motion video}
 \index{still camera}\index{allsky}\index{stphot}\index{allsky}
-\index{plate solver}
 

src/Satellites.tex

@@ -11,64 +11,60 @@
 
 \section{Overview of Satellites}
 \label{sec:overview-satellite}
-\index{satellite}\index{RF}
+
 This chapter gives a brief overview of \glspl{satellite}, with particular
-antention to ones using amateur \gls{RF} bands.
+antention to ones using \gls{amateur-radio} bands.
 
 
 \section{SatNOGS DB}
 \label{sec:satnogs-db}
 
-The \gls{SatNOGS DB} is a database that lists \glspl{satellite},
-many of which can be tracked by ground station operators on the
+The \gls{SatNOGS-DB} is a database that lists \glspl{satellite},
+many of which can be tracked by \gls{ground-station} operators on the
 \gls{SatNOGS} network.
 
 \begin{figure}[h!]
 	\begin{framed}
 	\centering
-        \includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{satnogs-db-web.png}
-        \caption{SatNOGS DB website.}
+        \includegraphics[keepaspectratio=true,height=0.80\textheight,width=0.80\textwidth,angle=0]{satnogs-db-web.png}
+        \caption{\gls{SatNOGS-DB} website.}
         \label{fig:satnogs-db-web}
-        \index{SatNOGS DB}
 	\end{framed}
 \end{figure}
 
 Individual \glspl{satellite} can be viewed, such as the RamSat \Gls{cubesat}.
-\index{RamSat}\index{CubeSat}
+\index{RamSat}
 
 % https://db.satnogs.org/satellite/YJWC-7364-7085-7563-0113
 \begin{figure}[h!]
 	\begin{framed}
 	\centering
         \includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{satnogs-db-ramsat-web.png}
-        \caption{SatNOGS DB RamSat CubeSat web page.}
+        \caption{\gls{SatNOGS-DB} RamSat \gls{cubesat} web page.}
         \label{fig:satnogs-db-ramsat-web}
         \index{RamSat}
 	\end{framed}
 \end{figure}
 
-
 For some \glspl{satellite}, \gls{telemetry} is available in a \gls{Grafana} dashboard.
 See the RamSat \gls{telemetry} dashboard.
-\index{RamSat}\index{telemetry}\index{Grafana}\index{dashboard}
+\index{RamSat}\index{dashboard}
 
 % https://dashboard.satnogs.org/d/XZQTCYznz/ramsat?orgId=1&refresh=30s&var-suid=48850
-\begin{figure}[h!]
-	\begin{framed}
+\begin{sidewaysfigure}[p!]
 	\centering
-        \includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{satnogs-telemetry-ramsat-web.png}
-        \caption{SatNOGS DB RamSat CubeSat telemetry web page.}
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{satnogs-telemetry-ramsat-web.png}
+        \caption{\gls{SatNOGS-DB} RamSat \gls{cubesat} \gls{telemetry} web page.}
         \label{fig:satnogs-telemetry-ramsat-web}
         \index{RamSat}
-	\end{framed}
-\end{figure}
+\end{sidewaysfigure}
 
 \section{Libre Satellites}
 \label{sec:libre-satellites}
 
 Below are \glspl{satellite} in \gls{orbit}, decayed, or designs on Earth that generally support the \gls{libre} way.
 These are some select \gls{libre} \glspl{satellite}:
-\index{orbit}\index{decay}
+\index{decay}
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
@@ -82,7 +78,7 @@ These are some select \gls{libre} \glspl{satellite}:
 \begin{figure}[h!]
 	\begin{framed}
 	\centering
-        \includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{upsat-web.png}
+        \includegraphics[keepaspectratio=true,height=0.80\textheight,width=0.80\textwidth,angle=0]{upsat-web.png}
         \caption{UPSat Website.}
         \label{fig:upsat-web}
         \index{UPSat}
@@ -93,37 +89,34 @@ These are some select \gls{libre} \glspl{satellite}:
 See figure \ref{fig:satnogs-obs-list-ramsat-web}, page \pageref{fig:satnogs-obs-list-ramsat-web}
 for a example list of observations of the RamSat \Gls{cubesat}.%
 \footnote{\url{https://network.satnogs.org/observations/?future=0&norad=48850&observer=&station=&start=&end=&transmitter_mode=&page=2}}
-\index{RamSat}\index{CubeSat}\index{RF}
+\index{RamSat}\index{observation}\index{schedule}
 
 \begin{figure}[h!]
 	\begin{framed}
 	\centering
-        \includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{satnogs-obs-list-ramsat-web.png}
-        \caption{List of observations of the RamSat CubeSat, example.}
+        \includegraphics[keepaspectratio=true,height=0.80\textheight,width=0.80\textwidth,angle=0]{satnogs-obs-list-ramsat-web.png}
+        \caption{List of observations of the RamSat \gls{cubesat}, example.}
         \label{fig:satnogs-obs-list-ramsat-web}
-        \index{RamSat}\index{observation}\index{CubeSat}
+        \index{RamSat}\index{observation}
 	\end{framed}
 \end{figure}
 
-Individual \gls{RF} observations are uploaded to the SatNOGS network,
-as can be seen in the example observation of the RamSat by SatNOGS
-ground station ``2380 - Piszkesteto UHF'' run by volunteer bcsak (username).
-\index{RF}\index{RamSat}
+Individual \gls{RF} observations are uploaded to the \gls{SatNOGS} network,
+as can be seen in the example observation of the RamSat \gls{cubesat} by \gls{SatNOGS}
+\gls{ground-station} ``2380 - Piszkesteto \gls{UHF}'' run by volunteer bcsak (username).
+\index{RamSat}\index{bcsak}
 
-\begin{figure}[h!]
-	\begin{framed}
+\begin{sidewaysfigure}[p!]
 	\centering
-        \includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{satnogs-obs-6401760-web.png}
-        \caption{Sample observation of RamSat CubeSat on SatNOGS website.}
+        \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{satnogs-obs-6401760-web.png}
+        \caption{Sample observation of RamSat \gls{cubesat} on SatNOGS website.}
         \label{fig:satnogs-obs-6401760-web}
-        \index{RamSat}\index{observation}\index{CubeSat}
-	\end{framed}
-\end{figure}
+        \index{RamSat}\index{observation}
+\end{sidewaysfigure}
 
 
 \section{Satellite Orbits}
 \label{sec:satellite-orbits}
-\index{orbit}\index{SGP}\index{SDP}\index{TLE}
 
 Satellite \glspl{orbit}.
 See \gls{SGP} and \gls{SDP}.

src/Software.tex

@@ -26,26 +26,32 @@ for a diagram with an overview of the software process.
                         back arrow distance=0.75,
                 }
                 \smartdiagram[flow diagram:horizontal]{Acquire, Process, Analyze, Upload}
-                \caption{SatNOGS Optical Operation Pipeline}
+                \caption{\gls{SatNOGS-Optical} Operation Pipeline}
                 \label{fig:operation}
                 \index{operation}
 %	\end{framed}
         \end{figure}
 \end{center}
+\index{acquire}\index{process}\index{analyze}\index{upload}
 
 \section{Setup Optical Ground Station Software}
 \label{sec:software-setup}
 \index{software}
 HOWTO set up and configure a \gls{SatNOGS-Optical} \gls{ground-station} prototype.
-Note: the SatNOGS network is not yet ready for optical data.
+Note: the \gls{SatNOGS} network is not yet ready for optical data.
 
-Setup an embedded computer, such as an Odroid N2, with \gls{Debian} stable
-(11/Bullseye) or testing (Bookworm).
-\index{embedded computer}\index{Odroid}\index{Debian}
+For a description of installation using \gls{Docker}, see
+section \ref{sec:software-docker}, page \pageref{sec:software-docker}.
+For a ``manual'' install, see immediately below.
 
-See each repository for latest documentation.
+Setup an \gls{embedded-system}, such as a \gls{Raspberry-Pi} or an Odroid N2,
+with \gls{Debian} stable (11/Bullseye) or testing (Bookworm).
+\index{Odroid}
 
-Install dependencies from \gls{Debian} repository:
+See each \gls{software-repository} for latest documentation.
+\index{repository}
+
+Install dependencies from the \gls{Debian} \gls{software-repository}:
 
 \begin{minted}{sh}
 sudo apt update
@@ -56,9 +62,10 @@ sudo apt install python3-virtualenv python3-pip python3-dev \
     astrometry-data-tycho2-08 astrometry-data-tycho2-09 \
     astrometry-data-tycho2-10-19
 \end{minted}
+\index{virtualenv}\index{PIP}
+\index{Giza}\index{Source Extractor}
 
 Next, install the \texttt{\gls{hough3d-code}} dependency.
-\index{hough3d-code}
 
 \begin{minted}{sh}
 git clone https://gitlab.com/pierros/hough3d-code
@@ -67,8 +74,9 @@ make all
 sudo cp -p hough3dlines /usr/local/bin/hough3dlines
 \end{minted}
 
-Install \texttt{\gls{satpredict}} from using either the cbassa or spacecruft repo.
-\index{satpredict}
+Install \texttt{\gls{satpredict}} from using either the cbassa or spacecruft
+\gls{software-repository}.
+\index{repository}
 
 \begin{minted}{sh}
 cd ../
@@ -80,10 +88,10 @@ make
 sudo make install
 \end{minted}
 
-Now install \texttt{stvid}, the main acquisition and processing
+Now install \texttt{\gls{stvid}}, the main acquisition and processing
 application. It is written in \gls{Python}. Either use the spacecruft
-\texttt{git} repository or the cbassa one.
-\index{stvid}\index{Python}
+\texttt{git} \gls{software-repository} or the cbassa one.
+\index{acquire}
 
 \begin{minted}{sh}
 cd ../
@@ -92,8 +100,8 @@ git clone https://spacecruft.org/spacecruft/stvid
 #git clone https://github.com/cbassa/stvid
 \end{minted}
 
-Optionally, set up a \gls{Python} virtual environment:
-\index{Python}\index{virtualenv}
+Optionally, set up a \gls{Python} virtual environment and use \gls{PIP}:
+\index{virtualenv}
 
 \begin{minted}{sh}
 cd stvid
@@ -112,7 +120,7 @@ pip install --upgrade -r requirements.txt
 \index{numpy}
 
 If the system \texttt{python3-numpy} conflicts, you could try installing
-numpy in the virtualenv thusly:
+numpy with \gls{PIP} in the virtualenv thusly:
 
 \begin{minted}{sh}
 pip install --upgrade --ignore-installed numpy
@@ -121,7 +129,7 @@ pip install --upgrade --ignore-installed numpy
 \gls{Debian} in bug \texttt{\#941466} changed the name of the
 \texttt{sextractor} dependency to \texttt{source-extractor},
 so a symlink is needed for now:
-\index{Debian}\index{Source Extractor}
+\index{Source Extractor}\index{SExtractor}
 
 \begin{minted}{sh}
 sudo ln -s /usr/bin/source-extractor /usr/local/bin/sextractor
@@ -129,7 +137,7 @@ sudo ln -s /usr/bin/source-extractor /usr/local/bin/sextractor
 
 \section{Configure Software}
 \label{sec:software-configure}
-Configure the embedded computer.
+Configure the \gls{embedded-system}.
 
 \begin{minted}{sh}
 cd stvid/
@@ -139,7 +147,7 @@ cp -p configuration.ini-dist configuration.ini
 # Set:
 vi configuration.ini
 \end{minted}
-\index{stvid}\index{configuration.ini}
+\index{configuration.ini}
 
 Edit various \texttt{configuration.ini} fields:
 \begin{minted}{sh}
@@ -160,6 +168,7 @@ st-password = bar
 # Path to source-extractor
 sex_config = /usr/share/source-extractor/default.sex
 \end{minted}
+\index{Source Extractor}\index{COSPAR}\index{TLE}
 
 Store downloads here:
 
@@ -177,27 +186,25 @@ export ST_TLEDIR=$HOME/TLE
 export ST_OBSDIR=$HOME/satobs
 export ST_LOGIN="identity=foo@no:pass"
 \end{minted}
-\index{sattools}\index{TLE}
 
-Set \texttt{astrometry.net} to run in parallel, assuming you have enough RAM:
+Set \texttt{astrometry.net} to run in parallel, assuming you have enough \gls{RAM}:
 (This doesn't appear to work? Breaks?).
-\index{astrometry.net}
 
 \begin{minted}{sh}
 sudo vim /etc/astrometry.cfg
 # Uncomment:
 inparallel
 \end{minted}
+\index{astrometry.net}
 
 
 \section{skymap}
 \label{sec:skymap}
-\index{skymap}\index{orbit}\index{sattools}
 
-Use \gls{skymap} for viewing \gls{satellite} \glspl{orbit} tracks
-projected on a map of of the sky. Skymap is part of \gls{sattools}.
-\Gls{skymap} isn't a required part of the toolchain, but it is useful
-to see what \glspl{satellite} are visibile at a particular time and
+Use \gls{skymap} for viewing \gls{satellite} \glspl{orbit} trails
+projected on a map of of the sky. \Gls{skymap} is part of \gls{sattools}.
+\Gls{skymap} isn't a required part of the \gls{toolchain}, but it is useful
+to see what \glspl{satellite} are visible at a particular time and
 location.
 
 Source:
@@ -211,26 +218,24 @@ My fork:
 \begin{sidewaysfigure}[p!]
         \begin{center}
                 \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{skymap-giza-21.png}
-                \caption{\texttt{skymap} example screenshot.}
-                \index{skymap}\index{sattools}
-                \label{fig:skymap-giza-21}
+                \caption{\texttt{\gls{skymap}} example screenshot.}
+		\label{fig:skymap-giza-21}
         \end{center}
 \end{sidewaysfigure}
 
 \fbox{
         \parbox{\linewidth}{
                 \textcolor{red}{NOTICE:} \\
-                The main upstream sattools package requires non-\gls{libre} \texttt{pgplot} on host computer which is not \gls{DFSG} compatible.
-                \index{proprietary}\index{DFSG}\index{pgplot}
+                The main upstream \gls{sattools} package requires non-\gls{libre} \texttt{pgplot} on the host computer which is not \gls{DFSG} compatible.
+                \index{proprietary}\index{pgplot}
         }
 }
 
-
 Described below is how to build and install my fork of \gls{sattools} to use
-\gls{skymap} instead of upstream. Upstream requires non-libre software which
+\gls{skymap} instead of upstream. \Gls{upstream} requires non-\gls{libre} software which
 also happens to be very difficult for most users to compile. My fork uses the
 Giza library which replaces pgplot. It is much easier to build.
-\index{fork}\index{sattools}\index{skymap}\index{Giza}
+\index{fork}\index{Giza}\index{pgplot}
 
 \begin{minted}{sh}
 # Install dependencies
@@ -261,7 +266,7 @@ sudo make uninstall
 \end{minted}
 
 See below for \gls{skymap} (fork) usage:
-\index{TLE}
+
 
 \begin{minted}{sh}
 tleupdate
@@ -301,7 +306,7 @@ Visualize satellites on a map of the sky.
 
 \section{Tracking Software}
 \label{sec:software-tracking}
-\index{track}\index{software}
+\index{track}\index{software}\index{mount}
 The tracking software used depends upon the tracking mount.
 
 See section \ref{sec:hardware-tracking-ground-station},
@@ -313,42 +318,93 @@ software:
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
-        \item [Telescope] --- Controlling \glspl{telescope} remotely.
-        \item [Antenna] --- Controlling \glspl{antenna} remotely with hamlib.
-        \item [Cameras] --- Controlling PTZ cameras remotely.
+        \item [\Glspl{telescope}] --- Controlling \glspl{telescope} remotely.
+        \item [\Glspl{antenna}] --- Controlling \glspl{antenna} remotely with hamlib.
+        \item [Cameras] --- Controlling \gls{PTZ} cameras remotely.
 \end{description}
 \end{mdframed}
-\index{telescope}\index{antenna}
+\index{hamlib}
+\index{camera}
 
 
 \subsection{Telescope Tracking Software}
-Software that can be used with telescope tracking mounts:
+Software that can be used with \gls{telescope} tracking mounts:
+\index{mount}\index{track}
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
-        \item [INDI] --- Main client/server used by other applications.
-        \item [KStars] --- Sky charts, INDI control.
-	\item [Ekos] --- Application used within KStars for remote control
+        \item [\gls{INDI}] --- Main client/server used by other applications.
+        \item [\gls{KStars}] --- \Glspl{sky-chart}, \gls{INDI} control.
+	\item [Ekos] --- Application used within \gls{KStars} for remote control
          of \glspl{telescope} and related hardware via \gls{INDI}.
-        \item [Stellarium] --- Sky charts, has \gls{INDI} plugin.
-	\item [Other INDI] --- Many more applications work with \gls{INDI}.
-	\item [INDIGO] --- Positions itself as a next-generation INDI (?).
+        \item [Stellarium] --- \Glspl{sky-chart}, has \gls{INDI} plugin.
+	\item [Other \gls{INDI}] --- Many more applications work with \gls{INDI}.
+	\item [INDIGO] --- Positions itself as a next-generation \gls{INDI} (?).
 \end{description}
 \end{mdframed}
-\index{telescope}\index{INDI}\index{KStars}\index{Ekos}\index{Stellarium}
+\index{Ekos}\index{Stellarium}
 \index{INDIGO}
 
-Using \gls{INDI} with KStars and Ekos on a Sky-Watcher or Celestron
-telescope mount is a known working solution.
-\index{Sky-Watcher}\index{Celestron}
+Using \gls{INDI} with \gls{KStars} and Ekos on a Sky-Watcher or \gls{Celestron}
+\gls{telescope} mount is a known working solution.
+\index{Sky-Watcher}\index{Ekos}
 
+\gls{Celestron} \glspl{telescope} are widely used and available for many years.
+There is a variety of software written to control the mounts. The below list
+covers the drivers (e.g. \gls{INDI}), not the software on top (e.g \gls{KStars}).
+
+\gls{Celestron} Nexstar \gls{telescope} tracking mount drivers:%
+\footnote{\url{https://www.indilib.org/telescopes/celestron.html}}%
+\footnote{\url{https://github.com/indigo-astronomy/libnexstar}}%
+\footnote{\url{https://github.com/indigo-astronomy/indigo/blob/master/indigo_drivers/mount_nexstar/README.md}}
+\begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
+\begin{description}
+  \item [Celestron INDI] --- \gls{Celestron} \gls{INDI}
+  \item [libnexstar INDIGO] --- libnexstar INDIGO.
+\end{description}
+\end{mdframed}
+
+Sky-Watcher EQ6-R Pro \gls{telescope} tracking mount drivers:%
+\footnote{\url{https://www.indilib.org/telescopes/skywatcher.html}}%
+\footnote{\url{https://www.indilib.org/telescopes/skywatcher/eqmod.html}}%
+\footnote{\url{https://www.indilib.org/telescopes/skywatcher/synscan-telescope.html}}
+\begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
+\begin{description}
+  \item [EQMod Mount INDI] --- Drives Sky-Watcher protocol.
+  \item [Synscan INDI] --- Drives Synscan hand controller.
+   \gls{INDI} recommends using EQMod Mount over Synscan.
+  \item [libnexstar INDIGO] --- libnexstar INDIGO.
+\end{description}
+\end{mdframed}
+
+\subsection{INDI}
+\gls{INDI} does much, \gls{KStars}, etc.
+
+One option to consider is making \gls{stvid} an \gls{INDI} client.
+
+
+\subsection{INDIGO}
+INDIGO%
+\footnote{\url{https://www.indigo-astronomy.org/}}
+works with libnexstar, which supports many mounts:%
+\footnote{\url{https://github.com/indigo-astronomy/libnexstar}}
+
+\begin{quote}
+This library implements the serial commands supported by the Celestron
+NexStar hand control (HC) and SkyWatcher/Orion SynScan HC. This applies
+to the Celestron: NexStar GPS, NexStar GPS-SA, NexStar iSeries, NexStar
+SE Series, NexStar GT, CPC, SLT, Advanced-VX, Advanced-GT, CGE, CGEM etc.
+SkyWatcher: EQ5, HEQ5, EQ6 (Pro), AZ-EQ5 GT, AZ-EQ6 GT, EQ8 etc. and the
+corresponding Orion mounts.
+\end{quote}
 
 \subsection{Antenna Tracking Software}
 At present, for the \gls{SatNOGS} network \gls{RF} \glspl{ground-station},
 hamlib is typically used for tracking, if directional \glspl{antenna} are
-used. Hamlib was originally created for amateur radio equipment, but has
-expanded to control many more devices.
-\index{hamlib}\index{antenna}\index{RF}\index{amateur radio}
+used. Hamlib was originally created for \gls{amateur-radio} equipment, but has
+expanded to control many more devices. Hamlib can be used for some
+telescope mounts.
+\index{hamlib}
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
@@ -356,19 +412,32 @@ expanded to control many more devices.
 \end{description}
 \end{mdframed}
 
-I don't know of anyone prototying a satellite tracking mount with hamlib,
+\subsection{Hamlib}
+I don't know of anyone prototyping a satellite tracking mount with hamlib,
 but it should be possible using the ``leap frog'' method, perhaps on the
 same mount as existing \gls{SatNOGS} \glspl{antenna}. The mount may not
 be steady enough.
+\index{hamlib}\index{mount}\index{track}
+
+Hamlib lists support for the following tracking mounts, usually
+used with \glspl{telescope}.%
+\footnote{Output from version 4.3.1 of \texttt{rotctl --list}}
+
+\begin{minted}{sh}
+  1401  Celestron              NexStar                 20110821.0      Untested      ROT_MODEL_NEXSTAR
+  1801  Meade                  LX200/Autostar          20200610.0      Stable        ROT_MODEL_MEADE
+  1901  iOptron                iOptron                 20191209.0      Alpha         ROT_MODEL_IOPTRON
+\end{minted}
 
 
 \subsection{Camera Tracking Software}
-There are applications for using PTZ control of cameras, such as used in
+
+There are applications for using \gls{PTZ} control of cameras, such as used in
 ``security'' cameras.
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{description}
-	\item [motion] --- PTZ camera control. XXX check
+	\item [motion] --- \gls{PTZ} camera control. XXX check
 \end{description}
 \end{mdframed}
 
@@ -378,31 +447,29 @@ at present.
 
 \section{GNSS with \texttt{gpsd}}
 \label{sec:software-gnss}
-\index{GNSS}\index{GPS}\index{Galileo}\index{GLONASS}\index{Beidou}
-\index{gpsd}
+\index{Galileo}
 
-\gls{GNSS} is used for time synchornization and for (somewhat)
+\gls{GNSS} is used for time synchronization and for (somewhat)
 accurately determining the location of the observation.
 
 \gls{GNSS} collectively includes the USA \gls{GPS}, Europe's Galileo,
-Russia's GLONASS, and China's Beidou, as well as other
+Russia's \gls{GLONASS}, and China's \gls{BDS}, as well as other
 regional systems.
-\index{GPS}\index{Galileo}\index{GLONASS}\index{Beidou}
+\index{Galileo}
+\index{USA}\index{Europe}\index{Russia}\index{China}
 
-A basic, widely available \gls{COTS} USB \gls{GNSS} device
-with a basic (or no!) \gls{antenna} plugged into the embedded
-computer can get time and location accurate enough for the
+A basic, widely available \gls{COTS} \gls{USB} \gls{GNSS} device
+with a basic (or no!) \gls{antenna} plugged into the \gls{embedded-system}
+can get time and location accurate enough for the
 purposes here. See various U-Blox devices, for example.
-\index{COTS}\index{USB}\index{U-Blox}
+\index{U-Blox}
 
-In \gls{Debian} \gls{GNSS} service with a USB device can be provided
-by the \texttt{gpsd} application.
-\index{Debian}
+In \gls{Debian} \gls{GNSS} service with a \gls{USB} device can be provided
+by the \texttt{\gls{gpsd}} application.
 
 \begin{minted}{sh}
 sudo apt install gpsd gpsd-tools
 \end{minted}
-\index{gpsd}
 
 Edit the configuration file, \texttt{/etc/default/gpsd} like:
 
@@ -412,26 +479,28 @@ GPSD_OPTIONS="-Gn"
 USBAUTO="false"
 \end{minted}
 
-This will start a \texttt{gpsd} daemon listening on all interfaces,
+This will start a \texttt{\gls{gpsd}} \gls{daemon} listening on all interfaces,
 so it can be used by other computers on the network (such as if
 acquire and process are on different machines). Using the
 device \texttt{/dev/ttyACM0} can be problematic if there are multiple
 \texttt{/dev/ttyACM*} devices. Perhaps something like this could be
 used in that case:
+\index{/dev/ttyACM}
 
 \begin{minted}{sh}
 DEVICES="/dev/serial/by-id/usb-u-blox_AG_-_www.u-blox.com_u-blox_GNSS_receiver-if00"
 \end{minted}
 
-Even with \texttt{gpsd} configuration listening on all IPs,
+Even with \texttt{\gls{gpsd}} configuration listening on all \glspl{IP},
 don't think \texttt{systemd} won't do what it likes. So
 you may have to do:
 
 \begin{minted}{sh}
 systemctl edit --full gpsd.socket
 \end{minted}
+\index{systemd}
 
-And create a configuration like this (I have IPv6 disabled, in this case):
+And create a \gls{gpsd} configuration like this (I have \gls{IPv6} disabled, in this case):
 
 \begin{minted}{sh}
 [Unit]
@@ -447,12 +516,14 @@ BindIPv6Only=no
 [Install]
 WantedBy=sockets.target
 \end{minted}
+\index{systemd}
 
 (Re)start:
 
 \begin{minted}{sh}
 sudo systemctl restart gpsd.service gpsd.socket
 \end{minted}
+\index{systemctl}
 
 Test all is good:
 
@@ -468,6 +539,7 @@ Enable to start on boot:
 \begin{minted}{sh}
 sudo systemctl enable gpsd.service gpsd.socket
 \end{minted}
+\index{systemctl}
 
 See below for sample output from \texttt{cgps}.
 
@@ -502,19 +574,18 @@ See below for sample output from \texttt{cgps}.
 
 \section{NTP}
 \label{sec:software-ntp}
-\index{NTP}
-With all the above, time still needs to be configured.
-Configuring \texttt{gpsd} isn't enough for correct system time.
-The main system on the Internet used for time synchronization is NTP.
-In \gls{Debian} there are a few options for NTP.
-The best is to use a hardware GPS, with PPS for improved
-accuracy. The easiest is to just use NTP.
-\index{PPS}
 
-All systems in the chain need to have the correct time and
-location. It is best if they all pull from the same NTP
+With all the above, time still needs to be configured.
+Configuring \texttt{\gls{gpsd}} isn't enough for correct system time.
+The main system on the Internet used for time synchronization is \gls{NTP}.
+In \gls{Debian} there are a few options for \gls{NTP}.
+The best is to use a hardware \gls{GNSS} (\gls{GPS}), with \gls{PPS} for improved
+accuracy. The easiest is to just use \gls{NTP}.
+
+All systems in the \gls{pipeline} need to have the correct time and
+location. It is best if they all pull from the same \gls{NTP}
 server, or even better than best if they all run \gls{GNSS}
-hardware with PPS enabled.
+hardware with \gls{PPS} enabled.
 
 Some quick and dirty time synchronization commands.
 The \texttt{ntpd} daemon can have slow startup synchronization
@@ -532,43 +603,51 @@ sudo ntpdate time.mit.edu
 # Get time from local server, such as router (made up IP):
 sudo ntpdate 192.168.1.1
 
+# If above complains, to do an initial sync at boot (force ntpdate):
+sudo ntpdate -b 192.168.1.1
+
 # Restart daemon
 sudo systemctl start ntp
 \end{minted}
+\index{ntpd}\index{ntpdate}
 
-Go through each of the systems used in the toolchain and make
-sure they all have accurate time or everything will be off.
+Go through each of the systems used in the \gls{toolchain} and make
+sure they all have accurate time or processing will be off.
 
 
-\section{KStars}
+\section{KStars with Tracking Mount}
 \label{sec:software-kstars}
-\index{software}\index{KStars}\index{Debian}
-KStars is an application that has been used for years in the astronomy
-community. It is well established, well supported and included in \gls{Debian}.
+\index{software}\index{track}\index{mount}
+\index{Ekos}
+\gls{KStars} is an application that has been used for years in the astronomy
+community. It is well established, well supported, and included in \gls{Debian}.
 
-KStars has multiple uses for imaging \glspl{satellite}.
-One main use is to control a telescope tracking mount, such as the
+\gls{KStars} has multiple uses for imaging \glspl{satellite}.
+One main use is to control a \gls{telescope} tracking mount, such as the
 hardware described in section \ref{sec:hardware-mounts}, page \pageref{sec:hardware-mounts}.
+\index{track}\index{mount}
 
-For the purposes here, described below will be using KStars with a
-Sky-Watcher tracking mount with INDI and Ekos.
+For the purposes here, described below will be using \gls{KStars} with a
+Sky-Watcher tracking mount with \gls{INDI} and Ekos.
 See figure \ref{fig:video-enclosure-mount-tripod}, page \pageref{fig:video-enclosure-mount-tripod}
-for a photo of the setup used with KStars below.
+for a photo of the setup used with \gls{KStars} below.
+\index{Ekos}
 
-The telescope mount will be used in sidereal tracking mode,
+The \gls{telescope} mount will be used in sidereal tracking mode,
 where the stars will appear as
 ``points'', and the \glspl{satellite} will appear as trails.
 The mount is not used in a satellite tracking mode.
 Sidereal is the ``standard'' tracking mode of \glspl{telescope}.
-\index{Sky-Watcher}\index{INDI}\index{Ekos}
+\index{Sky-Watcher}\index{Ekos}
 
-KStars is the ``main'' application, but it depends on other key parts.
-\gls{INDI} is the protocol that KStars uses for telescope control.
+\gls{KStars} is the ``main'' application, but it depends on other key parts.
+\gls{INDI} is the protocol that \gls{KStars} uses for \gls{telescope} control.
 \gls{INDI} itself is a collection of applications.
-While KStars has the main sky chart and Ekos is launched within it,
+While \gls{KStars} has the main \gls{sky-chart} and Ekos is launched within it,
 the actual mount control is done with the Ekos application.
 While it may sound complex, all of this is set up pretty easily in
 \gls{Debian}.
+\index{Ekos}\index{mount}
 
 \begin{minted}{sh}
 # Quick and dirty from memory, something like:
@@ -576,80 +655,80 @@ sudo apt update
 sudo apt install kstars indi-bin indi-eqmod indi-gpsd
 \end{minted}
 
-KStars has a sky chart, as can be see in figure \ref{fig:kstars-skychart},
+\gls{KStars} has a \gls{sky-chart}, as can be see in figure \ref{fig:kstars-skychart},
 page \pageref{fig:kstars-skychart}.
-When mount control is functioning, a location on the sky chart, such as a star,
- can be clicked on and the mount will go to that location and optionally track it.
-Using this, a telescope mount can be used to easily point the camera at a location
-and track it to observe telescopes. It should also provide a superior \gls{FITS} file
-for extracting data than using a static mount (XXX made up).
-\index{KStars}\index{sky chart}\index{GOTO}\index{mount}\index{track}
+When mount control is functioning, a location on the \gls{sky-chart}, such as a star,
+ can be clicked on and the mount will \gls{GoTo} that location and optionally track it.
+Using this, a \gls{telescope} mount can be used to easily point the camera at a location
+and track it to observe \glspl{satellite}. It should also provide a superior \gls{FITS} file
+for extracting data than using a static mount with \glspl{star-trail} (XXX made up).
+\index{mount}\index{track}
+\index{camera}
 
-To use a telescope tracking mount for use with \texttt{stvid}, the following steps need to be performed in
+To use a \gls{telescope} tracking mount for use with \texttt{\gls{stvid}}, the following steps need to be performed in
 roughly this order, assuming everything has been configured.
-A brief overview of steps:
-\index{stvid}
+An overview of steps:
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{enumerate}
         \item Physically mount all hardware.
 	\item Plug in and power everything up.
 	\item Confirm all hardware looks ok (e.g. \texttt{lsusb}).
-	\item Confirm GNSS time and location are ok (e.g. \texttt{cgps -u m}).
+	\item Confirm \gls{GNSS} time and location are ok (e.g. \texttt{cgps -u m}).
          See section \ref{sec:software-gnss}, page \pageref{sec:software-gnss}.
-	\item Confirm time is correct on all systems in toolchain (e.g. \texttt{date}). 
-         See section \ref{sec:software-ntp}, page \pageref{sec:software-ntp}.
+	\item Confirm time is correct on all systems in the \gls{toolchain}
+         (e.g. \texttt{date}). 
+         See section \ref{sec:software-ntp}, page \pageref{sec:software-ntp},
+	for information about \gls{NTP}.
 	\item Run camera configuration script (e.g. \texttt{v4l2-ctl} commands).
-	\item Start \texttt{indiserver} on the embedded computer, using scripts to
+	\item Start \texttt{indiserver} on the \gls{embedded-system}, using scripts to
          include a camera (such as \texttt{indi\_v4l2\_ccd}.
-	\item Start KStars on the workstation.
-	\item Launch Ekos within KStars, under \texttt{Tools}.
-	\item In Ekos, select a configuration with the EQ Mount for the Sky-Watcher,
-         and \texttt{V4L2} for the CCD, which will work with The Imaging Source
+	\item Start \gls{KStars} on the workstation.
+	\item Launch Ekos within \gls{KStars}, under \texttt{Tools}.
+	\item In Ekos, select a configuration with the \gls{EQ} Mount for the Sky-Watcher,
+         and \texttt{\gls{V4L2}} for the \gls{CCD}, which will work with The Imaging Source
          camera used in this example. Alternatively, the ZWO ASI could be used with a similar configuration.
 	\item The Ekos configuration should also be set to use the remote \texttt{indiserver}
-         IP address of the embedded computer USB connected to the Sky-Watcher mount.
-	\item Hit the start button to start Ekos/INDI.
+	\gls{IP} address of the \gls{embedded-system} \gls{USB} connected to the Sky-Watcher mount.
+	\item Hit the start button to start Ekos/\gls{INDI}.
 	\item On the screen that pops up, confirm all the tabs are good.
 	\item Check the last configuration tab for the camera, it often
          resets the size.
-	\item Hit close on the screen with the INDI devices.
+	\item Hit close on the screen with the \gls{INDI} devices.
 	\item Click the mount icon, and start tracking.
-	\item Perhaps do some focusing... XXX
+	\item Perhaps do some focusing... XXX \index{focus}
 	\item Click the solver icon.
 	\item Click the Sync radio button.
 	\item Click Capture and Solve. XXX what is it.
 	\item If everything is tracking happily, good.
-	\item If not, do all the alignment steps.
+	\item If not, do all the alignment steps. \index{alignment}
 	\item When alignment is good and tracking is accurate, stop Ekos and close it.
-	\item Stop the \texttt{indiserver} running on the embedded computer.
-	\item Start the \texttt{indiserver} on the embedded computer, but without using a camera
-         (e.g. remove \texttt{indi\_v4l2\_ccd}.
-	\item Select the INDI configuration with a remote \texttt{indiserver},
-         the EQ Mount, and the Simulated \gls{CCD}.
-	\item Hit start in Ekos to get INDI connections going.
+	\item Stop the \texttt{indiserver} running on the \gls{embedded-system}.
+	\item Start the \texttt{indiserver} on the \gls{embedded-system},
+	 but without using a camera (e.g. remove \texttt{indi\_v4l2\_ccd}.
+	\item Select the \gls{INDI} configuration with a remote \texttt{indiserver},
+         the \gls{EQ} Mount, and the Simulated \gls{CCD}.
+	\item Hit start in Ekos to get \gls{INDI} connections going.
 	\item Confirm all is ok in hardware tabs, then hit close.
-	\item Now in the KStars sky chart window there is control of the mount without
-         interfering with the camera.
-	\item Start \texttt{stvid}. See XXX for more info.
-	\item When done capturing that part of the sky with \texttt{stvid},
-         stop \texttt{stvid}
-	\item Go to the KStars sky chart and right-click on the new location,
-         and slew to it.
-	\item Start \texttt{stvid} again, pointing at the new location.
+	\item Now in the \gls{KStars} \gls{sky-chart} window there is
+         control of the mount without interfering with the camera.
+	\item Start \texttt{\gls{stvid}}. See XXX for more info.
+	\item When done capturing that part of the sky with \texttt{\gls{stvid}},
+         stop \texttt{\gls{stvid}}
+	\item Go to the \gls{KStars} \gls{sky-chart} and right-click
+         on the new location, and \gls{slew} to it.
+	\item Start \texttt{\gls{stvid}} again, pointing at the new location.
 	\item Repeat the last few steps each time a new sky location is desired.
 \end{enumerate}
 \end{mdframed}
-\index{v4l2-ctl}\index{mount}\index{KStars}\index{telescope}\index{track}
-\index{lsusb}\index{cgps}\index{GNSS}\index{NTP}\index{indiserver}
-\index{Ekos}\index{Sky-Watcher}\index{V4L2}\index{The Imaging Source}
-\index{stvid}
+\index{v4l2-ctl}\index{mount}\index{track}
+\index{lsusb}\index{cgps}\index{indiserver}
+\index{Ekos}\index{Sky-Watcher}\index{The Imaging Source}
 
 \begin{sidewaysfigure}[p!]
         \begin{center}
                 \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{kstars-skychart.png}
-                \caption{KStars sky chart, example screenshot.}
-                \index{KStars}\index{sky chart}
+                \caption{\gls{KStars} \gls{sky-chart}, example screenshot.}
                 \label{fig:kstars-skychart}
         \end{center}
 \end{sidewaysfigure}
@@ -657,8 +736,7 @@ A brief overview of steps:
 \begin{sidewaysfigure}[p!]
         \begin{center}
                 \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{kstars-profile-edit-v4l2.png}
-                \caption{KStars using V4L2, example screenshot.}
-                \index{KStars}\index{V4L2}
+                \caption{\gls{KStars} using \gls{V4L2}, example screenshot.}
                 \label{fig:kstars-profile-edit-v4l2}
         \end{center}
 \end{sidewaysfigure}
@@ -666,13 +744,12 @@ A brief overview of steps:
 \begin{sidewaysfigure}[p!]
         \begin{center}
                 \includegraphics[keepaspectratio=true,height=1.00\textheight,width=1.00\textwidth,angle=0]{kstars-profile-edit-simulator.png}
-                \caption{KStars using simulated CCD, example screenshot.}
-                \index{KStars}\index{CCD}
+                \caption{\gls{KStars} using simulated \gls{CCD}, example screenshot.}
                 \label{fig:kstars-profile-edit-simulator}
         \end{center}
 \end{sidewaysfigure}
 
-If the camera and mount are connected to the embedded computer OK, it will
+If the camera and mount are connected to the \gls{embedded-system} OK, it will
 look like below, in this case with The Imaging Source camera and Sky-Watcher
 mount:
 
@@ -685,11 +762,13 @@ Bus 001 Device 003: ID 067b:23d3 Prolific Technology, Inc. USB-Serial Controller
 Bus 001 Device 002: ID 05e3:0610 Genesys Logic, Inc. Hub
 Bus 001 Device 001: ID 1d6b:0002 Linux Foundation 2.0 root hub
 \end{minted}
+\index{The Imaging Source}\index{Sky-Watcher}
 
 Note the \texttt{The Imaging Source Europe GmbH DMK 33UX174} device is the
 camera and the
-\texttt{Prolific Technology, Inc. USB-Serial Controller} is the telescope
-mount. Other views of the devices:
+\texttt{Prolific Technology, Inc. USB-Serial Controller} is the
+Sky-Watcher \gls{telescope} mount. Other views of the devices:
+\index{Sky-Watcher}
 
 \begin{minted}{sh}
 jebba@odroid-01:~$ ls -l /dev/bus/usb/002/003 /dev/bus/usb/001/003 /dev/video* /dev/ttyUSB0
@@ -700,9 +779,27 @@ crw-rw---- 1 root video    81,   0 Sep  1 20:08 /dev/video0
 crw-rw---- 1 root video    81,   1 Sep  1 20:08 /dev/video1
 crw-rw---- 1 root video    81,   2 Sep  1 20:08 /dev/video2
 \end{minted}
+\index{/dev/video}\index{/dev/ttyUSB}
 
 Side note: you need to be in the \texttt{plugdev, video, dialout} groups.
 Side note: on the Odroid N2, there is another \texttt{/dev/video} device,
 so three devices are appearing. The The Imaging Source camera appears
 as two \texttt{/dev/video} devices.
+\index{Odroid}\index{The Imaging Source}
+
+
+\section{\texttt{stvid} with Docker}
+\label{sec:software-docker}
+\index{Ekman, Daniel}
+
+Daniel Ekman has created a \gls{Docker} setup for easier installation
+and configuration.
+
+The \gls{Docker} source code repo is available here:
+
+* \url{https://github.com/kng/stvid-docker}
+
+The \gls{Docker} itself is here:
+
+* \url{https://hub.docker.com/repository/docker/knegge/stvid}
 

src/Solve.tex

@@ -11,31 +11,32 @@
 
 \section{Plate Solver}
 \label{sec:plate-solver}
-\index{plate solver}\index{FITS}
 
-A ``plate solver'' will take an image of stars and detect the time and place
+A ``\gls{plate-solver}'' will take an image of stars and detect the time and place
 of the picture. There are two main steps:
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{enumerate}
- \item Extract stars from an image, such as a \gls{FITS} file generated by \texttt{stvid}.
- \item ``Solve'' the image of the stars in the image against vast databases of star images.
+ \item Extract stars from an image, such as a \gls{FITS} file generated by \texttt{\gls{stvid}}.
+ \item ``Solve'' the image of the stars in the image against vast databases in a
+  \gls{star-catalogue}.
 \end{enumerate}
 \end{mdframed}
 
 See below for a list of software tools that detect/extract stars from
 images (e.g. \gls{FITS}).
+\index{detect}
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{itemize}
  \item Source Extractor.
- \item KStars with ekos adds \texttt{Internal SEP}.
- \item KStars with ekos adds \texttt{Builtin method for solver}.
+ \item \gls{KStars} with Ekos adds \texttt{Internal SEP}.
+ \item \gls{KStars} with Ekos adds \texttt{Builtin method for solver}.
 \end{itemize}
 \end{mdframed}
-\index{Source Extractor}\index{KStars}\index{ekos}
+\index{Source Extractor}\index{Ekos}
 
-See below for a list of plate solvers that can be used.
+See below for a list of \glspl{plate-solver} that can be used.
 
 \begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
 \begin{itemize}
@@ -45,7 +46,7 @@ See below for a list of plate solvers that can be used.
  \item Watney.
 \end{itemize}
 \end{mdframed}
-\index{astrometry.net}\index{astap}\index{Watney}
+\index{astap}\index{Watney}\index{astrometry.net}
 
 
 \section{Source Extractor}
@@ -60,10 +61,10 @@ widely used for many years.
 
 
 \section{astrometry.net}
-\index{astrometry.net}
+
 Astrometry.net is a website and software that can be run locally to solve
 a plate of stars that has been extracted from \texttt{Source Extractor}. XXX
-\index{Source Extractor}
+\index{Source Extractor}\index{astrometry.net}
 
 % https://nova.astrometry.net/
 \begin{figure}[h!]
@@ -72,49 +73,41 @@ a plate of stars that has been extracted from \texttt{Source Extractor}. XXX
         \includegraphics[keepaspectratio=true,height=0.60\textheight,width=0.60\textwidth,angle=0]{astrometry-web.png}
         \caption{nova.astrometry.net website.}
         \label{fig:astrometry-web-web}
-        \index{astrometry.net}
 	\end{framed}
 \end{figure}
 
-
 \fbox{
         \parbox{\linewidth}{
                 \textcolor{red}{NOTICE:} \\
-                Using astrometry.net online requires an account with non-libre services.
+                Using astrometry.net online requires an account with non-\gls{libre} services.
 		The astrometry.net software can be installed locally to avoid this.
-                \index{proprietary}
+                \index{proprietary}\index{astrometry.net}
         }
 }
 
 
 \section{Star Catalogues}
 \label{sec:star-catalogues}
-\index{star catalogue}\index{plate solver}\index{stvid}
-
-To use a plate solver, you will need star catalogues. They can get large.
-The \texttt{stvid} application includes a basic star catalogue.
+To use a \gls{plate-solver}, you will need \glspl{star-catalogue}. They can get large.
+The \texttt{stvid} application includes a basic \gls{star-catalogue}.
 XXX The \texttt{4200} index series is also recommended.
 
 
 \section{World Coordinate System}
 \label{sec:wcs}
-\index{WCS}
-
 \gls{WCS} info. XXX
 
 
 \section{SIP}
 \label{sec:sip}
-\index{SIP}
-
 \gls{SIP} info. XXX
 
 
 \section{Plate Solving with \texttt{stvid}}
 \label{sec:plate-solving-stvid}
-\index{plate solver}\index{stvid}\index{process}
+\index{process}
 
 Use the \texttt{process.py} scripts described in section \ref{sec:plate-solver},
 page \pageref{sec:plate-solver}, to solve plates
-with \texttt{stvid}.
+with \texttt{\gls{stvid}}.
 

src/Support.tex

@@ -11,10 +11,8 @@
 
 \section{Support}
 \label{sec:support}
-\index{community}
-\index{support}
-\index{forum}
-\index{Matrix}
+\index{community}\index{support}\index{forum}\index{help}
+
 \setlength{\parindent}{0pt}
 How to get help.
 

src/Upload.tex

@@ -9,10 +9,336 @@
 % International Public License (CC BY-SA 4.0) by Jeff Moe.
 %
 
-\section{Upload Data}
+\section{Push Data Upstream}
 \label{sec:upload}
 \index{upload}
-
-Push.
 The \gls{SatNOGS} network isn't ready for optical data yet.
+So there is nothing that can be uploaded. This is under
+development.
+
+\section{File Extensions}
+\label{sec:upload-extensions}
+\index{formats}
+\index{.cal}\index{.cat}\index{.csv}\index{.dat}\index{.fits}\index{.png}
+The following file extensions are in use:
+
+\begin{mdframed}[backgroundcolor=blue!10,linecolor=blue!30]
+\begin{description}
+        \item [.cal] --- Cal % XXX \index{.cal}
+        \item [.cat] --- Cat % XXX \index{.cat}
+        \item [.csv] --- \gls{CSV}
+        \item [.dat] --- Data.     \index{.dat}
+        \item [.fits] --- \gls{FITS}.
+        \item [.png] --- \gls{PNG}.
+\end{description}
+\end{mdframed}
+
+
+\section{Data Files}
+\label{sec:upload-data}
+\index{data}\index{process}\index{acquire}
+After the \texttt{stvid} acquisition and processing steps have been
+run, files such as below will be generated:
+
+\begin{minted}{sh}
+2022-08-23T04:16:26.633.fits
+2022-08-23T04:16:26.633.fits.cal
+2022-08-23T04:16:26.633.fits.cat
+2022-08-23T04:16:26.633.fits.png
+2022-08-23T04:16:26.633_48473_catalog.dat
+2022-08-23T04:16:26.633_48473_catalog.png
+2022-08-23T04:16:26.633_52718_catalog.dat
+2022-08-23T04:16:26.633_52718_catalog.png
+2022-08-23T04:16:26.633_90000_unid.dat
+2022-08-23T04:16:26.633_90000_unid.png
+2022-08-23T04:16:26.633_hough.csv
+2022-08-23T04:16:26.633_predict.csv
+2022-08-23T04:16:26.633_threshold.csv
+\end{minted}
+\index{.cal}\index{.cat}\index{.csv}\index{.dat}\index{.fits}\index{.png}
+
+
+\subsection{\texttt{.fits} FITS Files}
+\gls{FITS} files are the main files created during acquisition and
+are the main files used in processing. It has the data of
+the actual image taken with the camera. \gls{FITS} files will be significantly
+larger than the other files, at around 8 to 35 megabytes each, depending
+on sample rate, frame size, and \gls{binning}.
+\index{acquire}\index{process}
+\index{frame size}\index{sample rate}
+
+The \texttt{\gls{stvid}} program creates it's customized \gls{FITS} format
+file, which is a stack up of multiple images.
+I'll leave explanation of the \texttt{\gls{stvid}} \gls{FITS} file structure
+to the program's author, Cees Bassa:
+
+\begin{quote}
+With \gls{stvid}, I typically store 10 seconds worth of video frames, 100 frames at 10 \gls{Hz} frame rate or 250 frames at 25 \gls{Hz} frame rate into a so-called ``four frame''. Here, for each pixel of the initial 100 or 250 frames, the mean, standard deviation, maximum and argmax are stored, each as its own frame. Objects that move will stand out because they will have a high (max - mean) / standard deviation, which allows me to detect trails. Once a trail is detected, the argmax frame tells me the frame number and hence the motion of the trail, and using the timestamps of the individual 100 or 250 frames, I can reconstruct the pixel position as a function of time during the 10 second exposure, using only 4 frames instead of the 100 or 250 individual video frames.
+\end{quote}
+\index{Bassa, Cees}\index{four frame}
+\index{.fits}
+
+
+\subsection{\texttt{.cal} CAL Files}
+\index{.cal}
+Example \texttt{.cal} filename:\\
+\texttt{2022-08-23T04:16:26.633.fits.cal}\\
+
+Sample data from \texttt{.cal} file, just the top select lines of a 577 line file:
+
+\begin{minted}{sh}
+1172.876   11.776  7.1775 221.117561  45.185979  6.761
+ 786.524    1.817  6.0213 222.623526  37.272049  5.590
+ 838.954   21.772  8.0430 222.941344  38.403949  7.653
+ 872.352   25.919  8.3855 222.909215  39.103246  7.884
+ 692.542   37.123  8.2615 223.889916  35.455924  8.718
+ 738.829   47.126  8.2037 223.973142  36.430116  7.777
+ 691.964   52.656  7.7910 224.278547  35.490201  7.411
+ 951.962   53.159  8.0072 223.315748  40.816697  7.844
+1209.704   60.030  6.0799 222.327791  46.116208  5.811
+ 893.057   66.086  7.1867 223.943996  39.648460  8.039
+...
+\end{minted}
+
+
+\subsection{\texttt{.cat} CAT Files}
+\index{.cat}
+\texttt{\gls{stvid}} generates \texttt{.cat} files, generated from \gls{FITS} files, such as:\\
+\texttt{2022-08-23T04:16:26.633.fits.cat} \\
+
+Sample data from \texttt{.cat} file, just the top select lines of a 1,033 line file:
+
+\begin{minted}{sh}
+#   1 X_IMAGE                Object position along x                                    [pixel]
+#   2 Y_IMAGE                Object position along y                                    [pixel]
+#   3 MAG_BEST               Best of MAG_AUTO and MAG_ISOCOR                            [mag]
+#   4 FLUX_BEST              Best of FLUX_AUTO and FLUX_ISOCOR                          [count]
+#   5 FLUX_MAX               Peak flux above background                                 [count]
+#   6 BACKGROUND             Background at centroid position                            [count]
+  1172.8755     11.7756   7.1775     33.80787     11.09625     16.06616
+    28.8250     11.4696   6.7443     50.38253     5.008112     15.81194
+  1347.4933     10.4887   8.3649     11.32553     2.619246     16.04644
+   269.9134      9.8019   8.4220     10.74506      1.56768     15.97937
+   468.9823      7.9780   8.8072     7.535751     5.987358     16.02673
+  1475.9681      6.6672   8.6115     9.024131     2.281431     16.03049
+   847.0105      5.9795   8.1992     13.19223     14.31796     16.08833
+   181.5139      5.5141   7.9473     16.63711     2.278276     15.95168
+   460.1482      5.1577   8.5318     9.711239     2.795708     16.02688
+  1559.9583      2.9245   7.5915     23.08835     6.981803      15.9909
+   786.5237      1.8174   6.0213     98.05751     27.88283     16.09418
+...
+\end{minted}
+
+
+\subsection{\texttt{.fits.png} FITS PNG Files}
+
+\index{.fits.png}
+The \texttt{\gls{stvid}} application can generate multiple \gls{PNG} files,
+depending how many satellites it finds. In every case it creates at
+least one \gls{PNG} file, with a name like:
+
+\texttt{2022-08-23T04:16:26.633.fits.png}
+
+In this image, as can be see in figure \ref{fig:stvid-png}, page \pageref{fig:stvid-png},
+no detected satellites are indicated.
+The blue lines are from the ``Catalog'', which in this case means \glspl{TLE}.
+The blue lines are drawn whether no, a few, or many satellites are detected.
+They are generated by taking data from the \gls{plate-solver} about where the picture
+\gls{FoV} is, and overlaying satellite \glspl{orbit} that are calculated from
+\glspl{TLE}.
+\index{detect}
+
+The main blue line is slightly offset from where the satellite is calculated to
+appear.
+The blue line forms a small \texttt{L} shape.
+The smaller segment indicates the area where the satellite may pass.
+Next to the small segment line is the \gls{NORAD-ID} for the satellite.
+If it is unknown, it will be given the number \texttt{90000} or larger.
+
+\begin{figure}[h!]
+        \begin{center}
+                \includegraphics[keepaspectratio=true,height=0.85\textheight,width=0.85\textwidth,angle=0]{stvid/data/2022-08-23T04:16:26.633.fits.png}
+                \caption{\texttt{\gls{stvid}} PNG.}
+                \label{fig:stvid-png}
+        \end{center}
+\end{figure}
+\index{.fits.png}
+
+
+\subsection{\texttt{catalog.png} catalog PNG Files}
+
+\index{detect}\index{identify}
+When \texttt{\gls{stvid}} identifies a satellite, it creates a new \gls{PNG} file for each
+satellite detected in the image. A file name example follows, with satellite
+\gls{NORAD-ID} 48473 identified, also shown in figure
+\ref{fig:stvid-png-48473-catalog}, page \pageref{fig:stvid-png-48473-catalog}.
+
+\texttt{2022-08-23T04:16:26.633\_48473\_catalog.png}
+
+\begin{figure}[h!]
+        \begin{center}
+                \includegraphics[keepaspectratio=true,height=0.85\textheight,width=0.85\textwidth,angle=0]{stvid/data/2022-08-23T04:16:26.633_48473_catalog.png}
+                \caption{\texttt{\gls{stvid}} \gls{PNG} of the satellite trail of \gls{NORAD-ID} 48473 identified in red.}
+                \label{fig:stvid-png-48473-catalog}
+        \end{center}
+\end{figure}
+\index{identify}
+
+If multiple satellites are detected in the image, they will each get a \gls{PNG} file.
+For the example image, a satellite with \gls{NORAD-ID} 52718 was also identified.
+The file name is:
+
+\texttt{2022-08-23T04:16:26.633\_52718\_catalog.png}
+
+\begin{figure}[h!]
+        \begin{center}
+                \includegraphics[keepaspectratio=true,height=0.85\textheight,width=0.85\textwidth,angle=0]{stvid/data/2022-08-23T04:16:26.633_52718_catalog.png}
+                \caption{\texttt{\gls{stvid}} \gls{PNG} of the satellite trail of \gls{NORAD-ID} 52718 identified in red.}
+                \label{fig:stvid-png-52718-catalog}
+                \index{identify}
+        \end{center}
+\end{figure}
+
+
+\subsection{\texttt{unid.png} Unidentified PNG Files}
+
+\index{unidentified}
+As shown previously, \texttt{\gls{stvid}} will create a new \gls{PNG} with a
+red line when it identifies a satellite.
+When \texttt{\gls{stvid}} finds a trail it can't identify in the
+\gls{TLE} catalogs, it gives it a \gls{NORAD-ID} starting with \texttt{90000},
+incrementing by one.
+See figure \ref{fig:stvid-png-90000-unid}, page \pageref{fig:stvid-png-90000-unid},
+for an example of \texttt{\gls{stvid}} marking an unidentified trail red.
+In this case, the trail was created by an airplane, but \texttt{\gls{stvid}} would
+do the same with an unidentified satellite trail.
+\index{airplane}\index{unidentified}
+
+\begin{figure}[h!]
+        \begin{center}
+                \includegraphics[keepaspectratio=true,height=0.85\textheight,width=0.85\textwidth,angle=0]{stvid/data/2022-08-23T04:16:26.633_90000_unid.png}
+                \caption{\texttt{\gls{stvid}} \gls{PNG} of an unidentified trail in red.}
+                \label{fig:stvid-png-90000-unid}
+        \end{center}
+\end{figure}\index{unidentified}
+
+
+\subsection{\texttt{.dat} Data Files}
+\index{.dat}
+For each trail detected as shown in previous sections, such as for which
+a \gls{PNG} file was created,
+\texttt{\gls{stvid}} will output a \texttt{.dat} file. The \texttt{.dat} filenames
+corresponding to the figures at \ref{fig:stvid-png-48473-catalog}, \ref{fig:stvid-png-52718-catalog},
+and \ref{fig:stvid-png-90000-unid} are:
+
+\begin{minted}{sh}
+2022-08-23T04:16:26.633_48473_catalog.dat
+2022-08-23T04:16:26.633_52718_catalog.dat
+2022-08-23T04:16:26.633_90000_unid.dat
+\end{minted}
+
+Note, there is no \texttt{.dat} file created corresponding to the
+\texttt{2022-08-23T04:16:26.633.fits.png} file, since it doesn't show
+detected trails.
+
+The \texttt{.dat} file contents look like this, for \gls{NORAD-ID} 48473:
+
+\begin{minted}{sh}
+48473 21 040AX  9999 G 20220823041631625 17 25 1533406+483563 37 S
+\end{minted} 
+
+XXX This is the IOD ? XXX
+The first field is the \gls{NORAD-ID}. The fourth field looks like COSPAR. XXX
+Large number starting with 2022 is date and time stamp.
+\index{IOD}\index{COSPAR}
+
+The \texttt{.dat} file contents look like this, for \gls{NORAD-ID} 52718:
+\index{.dat}
+
+\begin{minted}{sh}
+52718 22 056C   9999 G 20220823041631625 17 25 1527277+381243 37 S
+\end{minted} 
+
+The \texttt{.dat} file contents look like this, for the unidentified trail
+(the airplane):
+\index{airplane}\index{unidentified}
+
+\begin{minted}{sh}
+90000 22 500A   9999 G 20220823041631625 17 25 1457613+535844 37 S
+\end{minted} 
+
+
+\subsection{\texttt{stvid} \texttt{.csv} Files}
+\index{.csv}\index{hough}\index{predict}\index{threshold}
+During processing, \texttt{\gls{stvid}} generates (at least!) three \gls{CSV} files.
+For the observation discussed above, staring with figure \ref{fig:stvid-png},
+the following \gls{CSV} files are generated:
+
+\begin{minted}{sh}
+2022-08-23T04:16:26.633_hough.csv
+2022-08-23T04:16:26.633_predict.csv
+2022-08-23T04:16:26.633_threshold.csv
+\end{minted} 
+
+
+\subsubsection{\texttt{stvid} \texttt{hough.csv} Files}
+\index{.csv}\index{hough}
+Full contents of the \texttt{2022-08-23T04:16:26.633\_hough.csv} file:
+
+\begin{minted}{sh}
+ax,ay,az,bx,by,bz,n
+1585.699766,186.468458,51.073014,0.879795,0.416052,0.229917,3424
+794.849123,355.614035,48.596491,0.780147,-0.382158,0.495304,285
+1297.660777,432.469965,52.989399,0.923059,0.193205,0.332617,283
+\end{minted} 
+
+
+\subsubsection{\texttt{stvid} \texttt{predict.csv} Files}
+\index{.csv}\index{predict}
+The \texttt{2022-08-23T04:16:26.633\_predict.csv} is 3,764 lines long.
+Below is an extract of the lines. I shortened the path, which
+included the full path to my home directory, for clarity:
+
+\begin{minted}{sh}
+satno,cospar,mjd,ra,dec,state,tlefile,age
+00134,61015U  ,59814.17808603,182.367480,+37.582914,sunlit,/data/tle/catalog.tle,0.441
+00134,61015U  ,59814.17809887,182.231429,+37.736730,sunlit,/data/tle/catalog.tle,0.441
+00134,61015U  ,59814.17811171,182.094454,+37.890457,sunlit,/data/tle/catalog.tle,0.441
+00134,61015U  ,59814.17812455,181.956550,+38.044091,sunlit,/data/tle/catalog.tle,0.441
+...
+00735,64002C  ,59814.17808603,227.004270,+34.763570,sunlit,/data/tle/catalog.tle,0.027
+00735,64002C  ,59814.17809887,227.192764,+34.379114,sunlit,/data/tle/catalog.tle,0.027
+00735,64002C  ,59814.17811171,227.378969,+33.994697,sunlit,/data/tle/catalog.tle,0.027
+...
+46083,20055BJ ,59814.17808603,204.492490,+40.972573,sunlit,/data/tle/catalog.tle,0.022
+46083,20055BJ ,59814.17809887,204.840813,+41.039396,sunlit,/data/tle/catalog.tle,0.022
+46083,20055BJ ,59814.17811171,205.193715,+41.105756,sunlit,/data/tle/catalog.tle,0.022
+...
+32706,08010A  ,59814.17808603,169.555855,+50.073199,sunlit,/data/tle/inttles.tle,0.624
+32706,08010A  ,59814.17809887,169.560127,+50.075268,sunlit,/data/tle/inttles.tle,0.624
+32706,08010A  ,59814.17811171,169.564400,+50.077336,sunlit,/data/tle/inttles.tle,0.624
+...
+\end{minted} 
+\index{.csv}\index{COSPAR}
+
+
+\subsubsection{\texttt{stvid} \texttt{threshold.csv} Files}
+\index{.csv}\index{threshold}
+\texttt{\gls{stvid}} creates a \texttt{threshold.csv} file with a filename like:
+
+\texttt{2022-08-23T04:16:26.633\_threshold.csv}
+
+The above file has 5,293 lines. Here are a few of them:
+
+\begin{minted}{sh}
+58.000000,0.000000,38.000000
+69.000000,1.000000,59.000000
+1832.000000,1.000000,52.000000
+418.000000,2.000000,11.000000
+1183.000000,2.000000,71.000000
+...
+1276.000000,1078.000000,1.000000
+11.000000,1079.000000,38.000000
+1500.000000,1079.000000,45.000000
+\end{minted}
 

src/figures/stvid/data/2022-08-23T04:16:26.633.fits.cal

@@ -0,0 +1,577 @@
+1172.876   11.776  7.1775 221.117561  45.185979  6.761
+ 786.524    1.817  6.0213 222.623526  37.272049  5.590
+ 838.954   21.772  8.0430 222.941344  38.403949  7.653
+ 872.352   25.919  8.3855 222.909215  39.103246  7.884
+ 692.542   37.123  8.2615 223.889916  35.455924  8.718
+ 738.829   47.126  8.2037 223.973142  36.430116  7.777
+ 691.964   52.656  7.7910 224.278547  35.490201  7.411
+ 951.962   53.159  8.0072 223.315748  40.816697  7.844
+1209.704   60.030  6.0799 222.327791  46.116208  5.811
+ 893.057   66.086  7.1867 223.943996  39.648460  8.039
+1644.801   60.641  8.0809 219.859908  54.774064  9.909
+1298.030   59.698  8.1633 221.848032  47.909366  7.946
+1231.085   66.293  8.0308 222.396519  46.574497  7.589
+ 662.623   64.225  8.8055 224.659389  34.918614  8.349
+1135.054   65.710  8.4105 222.856168  44.608568  9.757
+ 891.525 1009.674  6.8304 249.516782  39.577225  6.872
+ 893.222 1079.415  8.7107 251.380069  39.383044  8.346
+ 752.156 1079.244  7.1731 250.767598  36.509643  7.016
+1288.133 1075.341  6.0820 253.323153  47.416729  6.136
+1039.455 1040.776  8.7354 251.004342  42.508585  8.639
+ 716.277 1040.951  8.5025 249.656598  35.892589  8.456
+ 613.550 1033.001  7.0904 249.092899  33.821780  7.072
+1165.026 1029.680  8.6670 251.299431  45.103648  8.717
+1210.755 1027.226  7.5843 251.466081  46.044693  7.618
+ 855.304 1004.021  8.4547 249.225945  38.848159  8.631
+ 691.398  999.942  8.2416 248.534188  35.499970  8.085
+1314.932  997.784  7.7617 251.152001  48.264417  7.929
+1106.920  997.648  8.3066 250.107536  44.028904  8.371
+ 669.511  990.055  8.5380 248.218833  35.075365  8.327
+ 592.702  986.131  7.4661 247.877384  33.513673  7.124
+1025.337  985.868  8.3269 249.417879  42.392378  8.349
+1073.988  984.685  8.5050 249.595483  43.395314  8.429
+ 735.532  985.013  8.6605 248.308086  36.448484  8.550
+1390.995  983.505  7.5695 251.143955  49.862945  7.243
+1318.930  981.040  8.1057 250.663109  48.406609  8.679
+ 950.996  980.034  8.4477 248.958077  40.888100  8.058
+ 814.804  978.933  6.7769 248.424252  38.091062  6.636
+ 631.097  977.189  7.9174 247.776605  34.320316  8.081
+1080.695  975.894  7.4539 249.375707  43.564738  7.272
+ 602.818  974.585  7.1718 247.623842  33.750880  7.086
+ 674.362  971.449  6.2660 247.761598  35.225063  6.470
+ 586.102  972.495  8.4348 247.518779  33.410615  8.256
+1391.531  966.716  6.7516 250.615879  49.936443  6.530
+ 652.431  964.683  8.4363 247.523163  34.785894  8.182
+1216.935  963.543  8.2684 249.631548  46.393849  8.109
+ 671.703  958.869  7.5604 247.437885  35.201901  7.562
+1022.521  954.116  4.3042 248.525751  42.437027  4.193
+ 909.947  955.312  7.6845 248.138295  40.113248  7.974
+ 549.315  955.135  7.0626 246.990420  32.699461  6.990
+ 810.341  952.970  8.2536 247.732092  38.064532  8.123
+ 691.946  950.918  7.9018 247.300507  35.633811  8.106
+1337.684  945.822  4.4778 249.686859  48.928346  5.070
+1274.978  947.260  8.5118 249.419299  47.628315  8.417
+ 823.324  947.047  8.5981 247.623409  38.347310  8.208
+1224.335  942.785  5.9244 249.097154  46.610030  8.796
+1429.720  933.131  7.2529 249.757688  50.829831  7.147
+1006.625  933.053  7.9343 247.880228  42.162615  7.772
+ 937.017  931.758  8.0945 247.593948  40.736673  7.943
+1107.018  923.012  8.1554 247.983664  44.264198  7.830
+ 534.533  921.228  7.7138 246.127171  32.468304  7.735
+1341.771  918.813  8.1135 248.870818  49.086674  8.647
+1253.005  919.322  8.5887 248.479131  47.271604  9.001
+1071.793  916.797  7.6370 247.653746  43.545361  7.749
+1170.515  913.144  5.8147 247.946785  45.598273  5.686
+ 454.836  914.795  8.2797 245.771275  30.850165  9.707
+ 989.797  909.519  3.9964 247.160620  41.881677  5.047
+ 843.037  911.759  8.4800 246.755844  38.843167  8.140
+1044.786  909.053  8.1853 247.347133  43.015709  7.840
+ 526.441  905.893  6.6086 245.738337  32.341485  9.788
+ 772.007  904.532  5.6691 246.350709  37.394057  5.554
+ 540.722  905.390  7.7741 245.758052  32.626516  7.763
+ 706.049  903.679  8.5527 246.147421  36.027558  8.586
+ 592.448  902.341  7.6378 245.811207  33.697087  7.710
+ 796.738  901.959  8.4003 246.356113  37.910237  8.365
+1526.519  895.959  4.7044 249.047588  52.900048  5.498
+ 592.185  894.810  5.2941 245.621742  33.703485  5.576
+ 596.730  892.995  5.1006 245.589267  33.799051  5.390
+1061.394  896.207  8.6064 247.050071  43.390897  8.558
+ 936.189  894.927  7.0139 246.589516  40.809484  7.031
+1430.355  894.978  8.2965 248.537835  50.968903  8.001
+ 753.844  894.671  8.2015 246.043360  37.036632  8.431
+ 684.477  893.314  7.1986 245.823423  35.611768  7.293
+1389.241  891.727  7.1112 248.236228  50.142109  6.917
+ 822.939  888.183  7.8832 246.068366  38.478292  7.855
+1281.170  885.345  7.3050 247.562323  47.952380  7.043
+1491.252  884.587  7.1127 248.496612  52.237960  6.927
+ 830.196  884.367  8.0983 245.989801  38.641750  8.010
+1329.315  877.572  6.6297 247.525147  48.961097  6.431
+1134.456  875.638  7.7996 246.714273  44.954389  7.418
+ 558.625  875.727  8.3836 245.070962  33.053280  8.558
+ 992.115  874.477  8.4329 246.200422  42.017097  8.450
+1435.296  872.043  8.6236 247.818980  51.137996  8.539
+ 634.920  871.369  8.0418 245.145714  34.627796  9.095
+1016.837  876.676  8.0019 246.346653  42.520018  7.801
+1249.112  867.474  7.5915 246.891112  47.341705  7.444
+ 760.108  866.092  8.7034 245.377996  37.232054  9.670
+ 995.782  864.856  8.2152 245.949347  42.111302  8.019
+ 537.176  863.929  7.9528 244.734918  32.627060  8.113
+ 901.059  862.453  8.5954 245.593596  40.163440  8.712
+ 616.217  862.080  8.3532 244.869160  34.262874  8.089
+1153.011  860.260  7.9810 246.329876  45.378596  7.854
+1041.835  861.212  8.3949 245.994095  43.074161  8.159
+1119.775  859.659  7.3502 246.200282  44.689935  7.227
+ 747.102  858.033  6.5024 245.075866  36.975584  6.784
+1415.017  858.274  8.5458 247.279253  50.766399  8.172
+ 496.439  855.487  7.0771 244.441546  31.804391  6.918
+1277.649  855.457  6.6877 246.633409  47.957606  6.628
+1445.552  851.232  6.4715 247.181018  51.407735  6.424
+1461.995  848.971  8.0188 247.179163  51.751052  7.772
+1179.033  848.094  7.7942 246.066920  45.944455  8.003
+ 625.703  847.564  7.7702 244.524487  34.482759  7.565
+ 961.026  846.950  8.1079 245.347832  41.435092  8.014
+1088.913  845.555  7.8927 245.691342  44.083615  7.725
+ 939.244  845.538  7.7492 245.263801  40.991091  8.325
+1453.678  844.716  7.5129 247.005156  51.592089  7.427
+ 904.023  842.665  8.4275 245.070605  40.259429  8.161
+ 877.379  841.673  5.6439 244.979751  39.708595  5.528
+ 783.788  842.100  7.3577 244.752378  37.765715  7.346
+ 615.511  841.955  8.5761 244.364081  34.281242  8.252
+ 683.970  839.874  7.7135 244.463523  35.699581  7.480
+1388.895  835.500  8.4745 246.436952  50.290072  8.493
+1074.929  833.478  8.3426 245.299712  43.819768  7.987
+ 807.513  832.970  8.6113 244.567474  38.275306  8.324
+1279.185  831.197  8.6139 245.892345  48.052692  8.638
+1258.837  829.976  8.0205 245.786395  47.630551  8.651
+1429.283  828.756  7.5079 246.383304  51.138479  7.271
+1395.914  828.881  7.9934 246.249254  50.452063  7.907
+ 969.906  826.636  8.4319 244.810187  41.659374  8.073
+ 721.979  825.726  8.4138 244.186654  36.510952  8.166
+ 568.189  825.170  8.6031 243.849121  33.330063  9.116
+1456.637  821.532  7.5580 246.251096  51.716610  7.368
+1382.870  822.213  8.2002 245.990346  50.202803  8.279
+ 690.165  820.707  7.9290 243.985714  35.870715  8.173
+1158.168  819.539  7.7364 245.145730  45.579193  7.614
+ 679.355  819.055  8.3201 243.926106  35.640970  8.252
+ 634.443  818.393  7.3967 243.812378  34.713171  7.363
+ 723.337  816.980  7.1779 243.961336  36.554482  7.136
+ 592.824  815.957  5.3757 243.670225  33.858616  5.620
+ 823.919  816.669  7.8162 244.177236  38.645022  7.900
+1483.727  814.010  7.1635 246.110001  52.289411  6.830
+1388.661  815.102  7.6256 245.779531  50.344216  7.477
+1524.866  813.842  8.6012 246.272811  53.126570  8.477
+1192.517  808.990  4.0162 244.935156  46.313369  3.854
+ 957.771  812.806  7.9418 244.392346  41.429561  8.173
+ 890.586  811.447  6.8347 244.193601  40.038366  6.916
+ 527.009  811.508  8.2604 243.435059  32.503521  8.399
+1408.292  811.033  8.3401 245.714867  50.756978  8.678
+ 531.029  802.183  7.7226 243.212501  32.599210  7.606
+1324.034  799.710  8.6170 245.069008  49.051972  8.217
+ 656.518  798.554  7.6131 243.355448  35.198926  7.650
+ 561.788  798.937  8.1854 243.190160  33.236786  8.570
+1625.124  796.573  5.9103 246.005420  55.159689  8.871
+ 533.315  796.307  7.6460 243.072927  32.655355  7.458
+1442.139  793.869  8.1378 245.285393  51.488556  8.071
+1322.734  791.262  6.0122 244.796724  49.038161  6.072
+ 565.920  787.652  6.4251 242.915001  33.342760  6.443
+ 451.090  786.687  7.1724 242.725099  30.985399  7.501
+ 793.815  786.191  7.3406 243.303848  38.072416  7.121
+1468.120  785.468  6.9196 245.102406  52.039034  6.635
+ 616.955  785.958  8.0599 242.960495  34.396652  7.935
+ 500.856  784.543  7.9769 242.731303  32.003080  7.636
+ 903.207  783.725  8.5669 243.464347  40.348811  8.094
+ 877.725  781.879  7.2253 243.365176  39.824427  7.268
+ 714.013  778.527  5.6515 242.950216  36.425089  5.772
+ 694.301  774.055  7.9722 242.801764  36.021145  7.801
+ 840.081  772.206  6.5044 243.027270  39.055521  6.531
+1224.035  768.376  7.7932 243.799590  47.040088  7.976
+1215.915  765.682  8.5323 243.696515  46.877603  8.623
+ 421.012  766.048  8.2476 242.161672  30.382399  8.067
+1059.796  760.983  8.5551 243.179814  43.649583  8.190
+1028.564  760.179  8.4694 243.089562  42.988660  8.805
+ 353.353  759.286  7.7792 241.903089  29.027824  9.476
+ 998.461  757.660  5.9661 242.948331  42.374570  6.043
+ 922.921  771.619  7.9360 243.179989  40.781706  7.911
+1203.627  757.818  8.7465 243.431745  46.639703  8.426
+ 973.019  757.983  8.3721 242.906921  41.843042  8.844
+1249.565  755.717  8.4190 243.481280  47.595719  8.320
+ 582.836  754.199  8.7249 242.112209  33.733083  8.446
+1167.084  752.583  7.7616 243.179214  45.894369  7.674
+ 715.476  751.051  4.8317 242.242874  36.490923  4.845
+ 670.214  752.205  7.8809 242.199965  35.549897  7.601
+ 910.885  750.165  7.9068 242.565554  40.555718  7.780
+1030.488  747.988  7.6151 242.747015  43.055005  7.472
+ 889.814  746.710  8.0768 242.498928  40.126427  9.167
+1182.852  747.177  8.1071 243.063123  46.226031  7.869
+1017.319  746.495  7.5962 242.706266  42.810762  9.212
+1522.453  745.764  7.2666 243.947009  53.236671  6.988
+ 516.986  744.994  8.4824 241.786074  32.379583  9.473
+1090.089  743.868  8.1709 242.741706  44.309501  8.252
+ 396.577  744.167  7.9161 241.608310  29.904627  7.771
+1066.414  740.467  6.8169 242.601311  43.817649  6.704
+ 935.727  739.672  6.8783 242.396053  41.067588  9.933
+1338.772  737.395  8.6736 243.136440  49.471795  8.553
+1272.962  746.993  8.1705 243.271700  48.093626  8.742
+1256.159  735.796  8.2132 242.876034  47.769002  8.120
+1245.624  733.641  7.6185 242.798801  47.560020  8.035
+ 445.207  733.786  8.3129 241.418461  30.917022  8.539
+ 509.538  731.072  6.7079 241.438012  32.247783  6.879
+ 477.368  730.265  8.0287 241.376424  31.583428  7.739
+ 912.691  729.427  7.6454 242.004227  40.627533  7.660
+1361.627  728.816  8.7584 242.927206  49.963004  8.518
+1257.243  727.517  7.7889 242.632193  47.807006  7.670
+ 841.980  727.956  8.7939 241.843211  39.155908  8.459
+1318.008  726.324  8.2853 242.738144  49.063651  8.129
+1118.724  722.712  4.3521 242.192403  44.934918  4.216
+ 642.660  725.076  8.3926 241.468557  35.006039  8.115
+1295.966  722.574  7.5827 242.566994  48.611384  7.502
+1138.979  722.498  8.2367 242.228186  45.353288  8.237
+ 553.050  721.932  8.0479 241.267822  33.152378  7.967
+ 716.208  720.639  7.3711 241.453304  36.528225  7.491
+ 605.234  720.443  7.6108 241.296915  34.236747  7.756
+ 520.995  715.971  7.8228 241.081838  32.497244  8.057
+1139.765  714.656  7.2226 241.997467  45.380293  7.125
+1465.974  713.497  8.8022 242.689212  52.137071  8.590
+ 601.911  710.867  7.0091 241.056183  34.178795  6.778
+1509.888  708.648  7.8949 242.634432  53.042633  7.995
+1370.660  708.492  7.0607 242.288943  50.180863  6.965
+1397.178  706.216  8.6001 242.279445  50.733354  8.197
+ 840.763  705.332  6.8396 241.236636  39.156511  6.735
+ 593.606  706.161  8.7971 240.928449  34.012974  8.296
+ 667.755  702.516  8.2769 240.927310  35.549078  8.131
+ 977.977  702.254  8.5799 241.346180  42.026652  8.436
+1502.492  700.539  7.8351 242.339515  52.904973  7.935
+1240.868  699.941  6.8638 241.748195  47.505042  6.638
+ 626.001  699.963  8.6893 240.807292  34.688024  8.359
+1059.034  697.974  7.6431 241.364067  43.719053  7.659
+ 719.207  696.378  5.9561 240.830685  36.631789  5.870
+1316.903  696.200  7.9004 241.784024  49.083094  7.636
+1143.989  696.777  8.4118 241.478458  45.495324  8.292
+ 641.605  696.765  8.5660 240.750265  35.019160  8.536
+ 391.432  691.963  5.2159 240.360689  29.851059  4.963
+ 489.988  690.911  7.9580 240.440327  31.876226  7.733
+1242.592  684.793  8.7227 241.287562  47.557102  8.550
+ 558.130  681.053  5.5878 240.261085  33.303508  5.471
+ 474.435  681.063  6.7233 240.177160  31.568241  6.738
+ 497.304  680.266  7.1592 240.181753  32.039537  7.195
+1519.732  677.055  8.3917 241.573933  53.294304  8.456
+ 880.823  676.539  6.9345 240.508708  40.022847  6.989
+1168.512  669.620  4.8887 240.699569  46.036700  4.694
+1383.662  668.766  7.8673 241.055872  50.499167  8.888
+1226.540  665.668  5.4229 240.663224  47.240360  6.624
+ 839.994  668.075  6.9715 240.228947  39.177514  6.767
+ 370.221  668.164  7.3561 239.774652  29.431582  7.235
+1045.705  667.005  8.6973 240.453077  43.473225  8.637
+ 965.486  666.972  8.4232 240.348186  41.796189  8.454
+1491.480  666.001  8.4885 241.141174  52.727747  8.374
+1279.665  663.861  8.4961 240.689693  48.351019  8.335
+ 398.183  663.457  7.4752 239.686388  30.004642  7.531
+1573.761  661.007  8.2742 241.134254  54.422412  8.157
+1221.187  656.752  7.1268 240.424618  47.184820  9.430
+1524.189  656.068  8.4663 240.869884  53.409278  8.631
+ 718.043  654.434  5.5297 239.740467  36.643776  5.772
+1514.682  655.112  8.2993 240.816113  53.216948  8.057
+ 732.525  654.169  8.0365 239.749619  36.941992  7.885
+1083.539  651.543  6.9681 240.049311  44.279504  6.902
+ 688.423  651.063  7.4154 239.628188  36.022147  7.606
+1289.989  650.737  8.5778 240.298933  48.578239  8.478
+1499.540  647.596  5.9919 240.523163  52.915919  6.083
+ 774.700  647.029  7.4721 239.601199  37.827483  7.373
+1460.528  644.105  8.7799 240.345854  52.119361  8.207
+1314.899  642.169  8.7480 240.064884  49.109229  8.430
+1352.205  638.871  7.7217 240.007392  49.900149  8.002
+1031.955  638.155  7.7364 239.606983  43.213711  7.425
+ 456.414  635.878  7.8104 239.064014  31.222072  8.104
+ 863.458  635.582  6.3955 239.374269  39.695083  6.420
+1145.012  633.974  8.8102 239.602194  45.574580  8.818
+1549.978  633.024  7.8988 240.103369  53.966638  7.733
+ 957.558  632.929  8.4985 239.397319  41.663092  8.818
+1576.931  631.361  8.1170 240.088556  54.522562  7.894
+1351.742  631.429  6.3211 239.768319  49.881046  6.067
+1218.824  630.872  8.8251 239.598110  47.117462  8.310
+1388.199  630.221  8.1555 239.781302  50.639262  7.978
+1510.101  628.999  8.1651 239.904975  53.152942  8.008
+ 374.418  629.148  8.0905 238.857550  29.537090  7.683
+1075.989  628.268  8.5690 239.362288  44.135708  8.444
+ 779.564  622.284  5.6371 238.948280  37.946957  5.466
+ 850.654  623.177  8.1418 239.029539  39.429400  7.891
+ 607.550  618.640  7.3455 238.736820  34.362530  7.138
+1574.804  616.806  8.6761 239.565000  54.487098  8.635
+1587.443  612.873  5.1949 239.447673  54.749766  4.987
+1000.106  613.648  5.9696 238.877462  42.566193  5.729
+ 867.027  613.711  8.4550 238.778843  39.782745  8.173
+ 510.057  613.483  8.3402 238.551370  32.342676  8.338
+ 370.529  609.009  8.5414 238.374056  29.468751  8.323
+1027.400  605.283  5.2286 238.657710  43.138565  5.556
+ 456.506  604.865  8.4457 238.312754  31.237409  8.253
+1596.881  600.339  7.9576 239.010222  54.952536  7.795
+1349.651  599.824  8.8943 238.749578  49.860523  8.418
+ 343.374  599.106  8.0692 238.128590  28.913298  7.939
+1551.954  597.051  8.7791 238.846455  54.031882  8.321
+ 912.170  597.201  8.4679 238.355058  40.731902  8.483
+ 938.933  593.399  8.1590 238.268384  41.295216  7.982
+ 390.451  593.351  7.4816 238.009437  29.881671  7.535
+ 994.265  588.989  4.8049 238.168928  42.451518  4.664
+1166.002  588.917  7.1562 238.285368  46.040055  7.352
+1003.904  582.174  7.7890 238.004061  42.663537  9.765
+ 668.760  580.898  4.8752 237.808049  35.657384  4.908
+1543.472  580.882  8.5643 238.268656  53.871046  8.351
+ 864.327  580.898  8.0538 237.887093  39.735943  8.099
+ 759.953  576.104  7.6542 237.715380  37.553495  7.634
+ 999.425  573.528  7.7333 237.738615  42.565410  7.437
+1283.269  568.111  6.2756 237.694261  48.483015  7.903
+1496.318  567.882  7.0657 237.791991  52.906983  6.894
+1441.047  563.513  8.4298 237.620094  51.771414  8.444
+1092.889  562.796  8.1584 237.458189  44.522103  7.757
+ 860.863  560.595  8.8854 237.332124  39.674230  8.438
+ 479.788  550.845  6.4566 237.007473  31.735614  6.576
+ 541.466  547.686  7.1955 236.937681  33.011995  7.174
+1401.545  546.914  8.6110 237.055806  50.954554  8.469
+1355.860  546.222  8.1795 237.024256  50.004577  8.024
+1150.625  544.832  6.9559 236.943195  45.732879  6.894
+1254.016  543.951  9.0320 236.932223  47.893023  8.645
+ 741.675  543.497  8.1295 236.852551  37.179617  8.042
+1096.259  541.693  7.3753 236.845225  44.598788  7.442
+ 423.217  542.081  8.1959 236.790625  30.565640  7.775
+ 958.788  539.193  8.6611 236.758911  41.719716  8.202
+1210.685  537.358  7.5633 236.724223  46.986257  7.278
+1451.153  537.177  8.6695 236.738501  51.979637  8.455
+1177.779  537.139  7.8837 236.715407  46.296790  8.011
+ 821.705  534.039  8.5613 236.613430  38.850303  8.354
+ 706.664  533.739  7.4648 236.602089  36.446003  7.602
+1459.068  533.274  8.4929 236.602175  52.147803  8.147
+1116.744  532.240  8.3680 236.568609  45.021844  7.910
+ 994.542  532.025  7.6838 236.556830  42.468405  7.495
+ 884.963  525.968  8.1189 236.390627  40.177549  7.850
+1484.984  525.113  8.2243 236.326216  52.677119  8.027
+ 934.327  522.065  8.1615 236.286474  41.211545  8.109
+1499.840  518.180  7.5471 236.090173  52.983570  7.439
+1496.043  516.305  7.8852 236.023999  52.905433  7.849
+ 758.752  515.574  8.6279 236.119820  37.534924  8.519
+1130.837  513.847  8.6444 236.022827  45.316068  8.403
+ 856.280  511.746  7.5129 236.007642  39.573858  7.740
+ 517.474  509.567  5.7668 235.997086  32.515808  5.694
+1157.993  510.037  8.5333 235.904373  45.885597  8.592
+1248.152  509.140  8.6118 235.849845  47.768402  8.421
+1206.796  509.607  8.6788 235.877547  46.903874  8.379
+1469.699  506.940  5.7435 235.711501  52.360902  5.473
+1115.742  502.984  8.4852 235.700577  45.000748  8.384
+ 628.458  502.977  8.0301 235.813318  34.812010  8.217
+1152.048  501.814  7.3989 235.658007  45.762058  7.050
+ 463.003  501.613  7.5845 235.809830  31.384583  7.309
+ 478.633  495.863  6.8605 235.669181  31.708754  6.871
+ 974.881  494.179  8.2378 235.492993  42.051327  8.339
+ 955.000  489.685  8.5784 235.369724  41.634073  8.310
+ 735.575  489.960  8.1402 235.452624  37.048405  7.720
+ 807.930  487.359  6.6314 235.359288  38.557393  7.887
+1262.099  484.641  8.3131 235.081461  48.054907  7.822
+1107.905  481.625  7.6234 235.073719  44.831009  7.595
+1060.767  481.441  7.3896 235.089267  43.846377  7.199
+ 815.735  481.070  7.6638 235.188798  38.718583  7.945
+ 758.250  477.197  6.9724 235.108297  37.517094  7.085
+ 734.270  477.466  7.5203 235.125916  37.016988  7.166
+1431.848  476.822  8.5104 234.720544  51.570246  8.481
+1082.988  476.689  8.6067 234.938433  44.311194  8.308
+ 394.741  475.209  7.7370 235.188783  29.972246  7.656
+1376.559  473.153  6.0898 234.642492  50.423271  5.932
+1208.377  472.611  6.7462 234.745353  46.926563  6.956
+1005.398  473.016  7.3058 234.883565  42.696946  7.899
+ 602.050  473.384  7.9511 235.072812  34.260305  7.938
+1121.893  472.670  8.2232 234.799197  45.117401  8.147
+1574.958  470.642  6.0266 234.383368  54.508730  5.969
+1282.147  470.871  7.9645 234.638402  48.462782  8.342
+ 716.015  466.351  4.8182 234.842726  36.636839  5.913
+1360.022  467.902  8.0682 234.480710  50.082206  7.785
+1202.142  466.748  6.0191 234.567583  46.797696  5.784
+1049.449  464.078  7.0841 234.594777  43.604260  6.818
+1581.189  459.723  6.0625 233.987670  54.630545  5.769
+1010.043  460.468  8.5196 234.531002  42.782465  8.594
+ 406.807  461.603  8.6892 234.860171  30.207289  8.863
+ 622.146  459.139  6.2683 234.703549  34.675040  6.245
+ 478.014  460.475  8.3853 234.806647  31.687928  8.425
+ 894.163  455.664  5.3611 234.456661  40.353433  5.353
+1456.721  456.506  7.0420 234.017407  52.069813  6.733
+ 783.028  456.004  7.8894 234.538252  38.028046  7.622
+ 697.631  454.941  7.1815 234.559503  36.247139  9.865
+ 471.624  455.158  7.5728 234.677103  31.551852  7.245
+1546.859  453.731  6.1130 233.817489  53.922148  6.098
+1114.432  449.016  8.6624 234.105599  44.950572  8.341
+1356.653  446.632  6.9457 233.799450  49.994638  7.073
+1342.355  446.486  7.3914 233.811769  49.698370  7.542
+ 401.832  445.122  8.0978 234.473845  30.102951  8.539
+1506.483  440.071  8.6798 233.401488  53.081100  8.453
+ 752.358  439.211  7.8399 234.109086  37.376597  8.495
+ 868.885  438.133  6.5189 234.009322  39.802568  6.903
+1029.428  435.612  6.8342 233.791705  43.167539  6.852
+ 800.112  434.579  6.4040 233.954973  38.373923  6.441
+ 396.325  434.631  6.6334 234.222614  29.991188  6.503
+ 672.369  434.681  7.8059 234.052753  35.705394  7.570
+1112.914  433.448  7.9654 233.644164  44.914217  8.579
+1072.608  433.632  7.2437 233.697289  44.067636  7.252
+ 830.676  430.210  4.9818 233.812163  39.010066  5.322
+ 682.771  431.588  8.6649 233.965269  35.923623  8.296
+1574.967  430.327  8.2750 232.954282  54.471415  8.601
+ 965.069  416.689  8.4229 233.316237  41.809679  8.245
+ 684.004  408.698  8.3886 233.372572  35.928958  8.597
+1230.180  408.583  8.8485 232.760013  47.333853  8.333
+ 922.051  401.567  5.1729 232.945743  40.899337  4.992
+ 919.272  393.821  4.9782 232.732327  40.833048  5.219
+1185.012  399.194  7.8392 232.540005  46.386087  7.766
+ 863.960  398.978  7.8711 232.934865  39.678877  7.785
+ 463.647  395.417  4.3256 233.232425  31.359130  4.143
+1018.679  398.112  8.5360 232.731917  42.911111  8.108
+1248.992  396.207  7.1772 232.347084  47.713440  6.855
+ 411.658  393.930  8.3178 233.235475  30.281222  8.222
+1554.749  391.750  6.8027 231.634131  54.020297  6.443
+1374.963  389.485  8.2368 231.918943  50.314911  8.036
+1224.733  389.497  6.4835 232.184971  47.201516  6.151
+ 717.422  389.366  6.6654 232.842935  36.616594  6.445
+1389.816  386.914  7.9480 231.812231  50.619560  7.819
+1459.304  385.332  7.1939 231.617187  52.052567  7.282
+ 898.078  385.445  8.3672 232.529734  40.385376  7.960
+ 875.638  384.300  8.1580 232.523092  39.909048  7.694
+ 726.704  381.180  6.6359 232.615869  36.804553  6.649
+ 614.502  379.381  7.0811 232.691961  34.465659  6.811
+1565.124  378.480  6.9523 231.146944  54.212801  6.891
+ 954.864  378.373  7.9949 232.264969  41.560087  8.034
+1402.019  377.005  8.7297 231.448673  50.912778  9.964
+1389.306  373.733  7.6442 231.384483  50.594148  7.867
+ 555.508  372.988  8.5410 232.592021  33.236869  8.380
+ 648.900  370.697  7.8957 232.435823  35.175237  8.015
+1018.495  369.500  7.5756 231.908002  42.889784  9.738
+ 461.200  369.026  6.7721 232.594868  31.285934  6.477
+1149.164  368.635  7.4177 231.681740  45.603916  7.214
+ 819.597  367.077  6.9371 232.130354  38.723732  6.720
+ 526.001  367.487  8.5878 232.490131  32.618757  8.435
+1072.919  361.833  7.8139 231.610903  44.003482  7.831
+1219.725  359.751  7.1897 231.283332  47.060826  6.866
+1166.120  359.558  7.6011 231.372652  45.947703  7.342
+1087.231  358.671  7.3277 231.496184  44.302238  7.316
+1465.935  358.511  8.6662 230.710636  52.153119  8.659
+1552.967  352.591  8.0541 230.265485  53.928525  7.661
+1476.044  349.008  8.1445 230.362137  52.344454  7.696
+1134.643  345.594  6.2118 231.021322  45.271035  6.191
+1458.154  337.529  5.9987 230.021461  51.958516  5.656
+1473.705  337.375  8.6425 229.954323  52.287535  8.831
+ 610.210  334.625  5.5014 231.572433  34.335996  5.615
+1249.149  334.188  8.5081 230.437100  47.634325  8.544
+ 756.829  325.469  4.3529 231.122618  37.377170  4.334
+ 520.701  326.891  7.2215 231.498738  32.474035  7.132
+1187.796  327.597  8.7934 230.372692  46.356610  8.337
+ 795.806  326.072  7.6925 231.077074  38.187698  7.688
+1374.489  325.487  8.0059 229.850748  50.214642  7.618
+1215.962  322.664  8.4409 230.155973  46.925698  8.209
+1442.990  321.526  8.6361 229.532811  51.617097  8.311
+1155.290  320.065  6.9188 230.220493  45.664871  6.785
+ 863.490  314.681  5.4811 230.655718  39.581462  5.733
+1096.660  314.037  6.4716 230.173666  44.434374  6.183
+1411.955  301.477  6.6330 228.990660  50.934668  8.944
+1256.913  301.595  8.0234 229.409945  47.739405  7.767
+ 663.485  302.022  8.3988 230.682084  35.394787  8.657
+1155.060  297.887  6.6444 229.562331  45.619827  6.828
+1125.948  298.954  8.2824 229.665156  45.017260  7.934
+ 607.381  297.112  7.6298 230.634689  34.229423  7.411
+ 490.329  298.114  8.4101 230.838435  31.811832  8.076
+ 932.398  295.885  7.1983 230.009625  40.984170  6.949
+ 968.850  290.335  8.2685 229.775751  41.733208  7.983
+ 500.074  289.504  8.3445 230.612626  32.003674  8.308
+ 545.245  285.789  5.6369 230.452396  32.933695  5.362
+1511.420  285.550  7.4926 228.109077  52.930089  7.751
+1380.895  284.477  8.2948 228.505368  50.259982  8.241
+1106.942  278.736  8.0676 229.081631  44.580559  8.449
+ 469.622  276.637  5.6139 230.349811  31.367373  9.308
+1009.915  277.562  7.5918 229.328585  42.565875  7.518
+ 779.801  277.590  8.5117 229.828702  37.784491  8.324
+1358.079  274.222  7.4924 228.251463  49.775235  7.379
+1270.654  273.070  7.8980 228.495551  47.969031  7.492
+ 475.817  271.239  7.1977 230.208661  31.480109  6.954
+1248.100  270.292  8.4812 228.475959  47.501973  8.281
+1301.144  266.125  7.3405 228.182239  48.580775  7.283
+1365.599  263.816  7.2409 227.895760  49.903035  7.887
+1488.369  263.754  8.4044 227.461785  52.410832  8.480
+ 526.685  261.083  6.6922 229.875199  32.514899  6.341
+ 830.024  254.559  8.3771 229.114559  38.790253  8.475
+1035.451  250.572  7.0078 228.496749  43.048080  6.685
+ 655.612  251.805  8.8122 229.405166  35.159591  8.642
+1518.171  250.850  8.2627 226.894100  52.993571  7.872
+1422.883  250.383  7.8747 227.269686  51.032413  8.314
+ 993.443  248.206  6.0541 228.542958  42.171407  6.333
+ 579.912  248.596  6.9719 229.471132  33.594331  6.755
+1506.165  247.644  7.6732 226.835525  52.743074  7.471
+ 747.836  246.771  7.4839 229.089040  37.069536  7.171
+ 485.835  244.766  8.2296 229.547304  31.647061  7.821
+1375.712  239.390  6.5694 227.081410  50.054959  6.444
+ 446.444  239.657  7.2443 229.498682  30.832930  6.970
+ 807.954  238.475  7.4575 228.735698  38.301109  7.175
+1767.008  233.994  8.7587 225.229703  57.753547  8.640
+ 807.315  225.696  6.4017 228.398259  38.264702  6.325
+ 567.998  223.605  3.6278 228.909787  33.320922  7.894
+ 826.865  224.358  7.9446 228.310461  38.665361  8.188
+ 842.971  217.766  7.9423 228.096023  38.987575  7.816
+ 828.053  212.494  8.2919 227.999983  38.670123  8.562
+1287.072  205.596  5.8959 226.357643  48.150971  5.575
+ 698.354  205.971  8.1842 228.143592  35.971610  7.897
+1456.980  204.863  7.3701 225.630434  51.619606  7.372
+ 495.496  203.144  5.9796 228.525181  31.787844  6.162
+ 736.521  203.485  7.6151 227.990011  36.754719  7.366
+ 844.578  194.724  8.6523 227.475625  38.975831  8.402
+1265.058  189.306  5.0502 225.947850  47.654426  6.095
+1009.721  192.091  8.3766 226.925295  42.388130  8.127
+1843.464  188.392  5.7643 223.155533  59.051060  9.677
+1408.762  183.300  8.3257 225.147213  50.578012  7.858
+1341.365  180.634  7.5003 225.359597  49.194777  7.377
+ 901.481  175.044  8.7452 226.788646  40.108045  8.164
+ 560.928  173.806  7.1825 227.662063  33.078883  7.031
+1354.592  170.218  8.8078 224.973479  49.433547  8.396
+1564.774  165.949  8.0982 223.913238  53.591237  9.684
+1122.157  165.259  6.8238 225.777305  44.644486  6.646
+1388.765  162.497  7.8620 224.576646  50.104272  7.969
+1250.521  161.691  6.6810 225.161324  47.277440  6.335
+ 951.775  160.925  7.7748 226.251055  41.109442  7.656
+ 571.640  157.617  7.5041 227.238782  33.265363  7.281
+ 593.500  153.130  6.9479 227.076767  33.706513  6.800
+ 727.338  150.211  6.6861 226.646440  36.456065  6.411
+1070.960  148.030  8.6585 225.474898  43.541835  8.204
+1368.029  144.226  5.9740 224.096002  49.628447  5.689
+ 832.080  144.456  7.9544 226.181329  38.605230  7.547
+ 607.346  142.643  8.2280 226.776230  33.965033  7.933
+1308.152  141.274  7.9302 224.284427  48.395271  7.759
+ 999.494  140.933  8.0761 225.526826  42.052346  8.026
+1122.780  138.984  7.2189 225.014957  44.586338  7.022
+ 646.515  137.019  8.2352 226.533606  34.753500  8.010
+ 920.336  129.095  3.6488 225.486509  40.390568  3.577
+ 850.724  121.034  8.4415 225.506471  38.927058  8.207
+ 906.898  118.798  7.3990 225.252878  40.084321  7.202
+1119.930  118.190  7.6733 224.429005  44.466318  7.407
+ 671.121  109.574  5.6714 225.792355  35.225802  9.781
+ 639.881  110.928  6.8562 225.902058  34.565759  6.692
+1225.123  107.394  7.6405 223.640190  46.593741  7.457
+1327.672  105.121  8.2153 223.087116  48.670722  7.715
+ 592.074  103.509  8.3242 225.852926  33.571166  8.123
+ 887.849  101.401  7.0359 224.854059  39.644892  6.730
+ 869.560  100.735  5.9185 224.903946  39.265335  5.674
+1066.975   96.691  8.3569 224.033387  43.317805  7.989
+1163.906   96.293  8.3078 223.602170  45.298816  7.965
+1182.714   94.095  8.3854 223.455446  45.682663  8.123
+ 579.026   92.551  7.4135 225.621927  33.274357  7.264
+1387.593   91.227  8.3931 222.325412  49.837749  8.229
+ 915.004   87.158  8.0047 224.369191  40.164288  8.884
+1223.133   85.626  7.0972 223.013508  46.476623  6.896
+ 835.002   87.030  8.4153 224.667684  38.519282  8.406
+1333.632   84.663  5.9300 222.422359  48.720999  6.674
+1477.820   81.433  8.5560 221.612055  51.564864  9.729
+ 963.399   80.309  7.6162 223.999374  41.136610  7.214
+ 773.604   80.790  8.7149 224.739888  37.248412  9.388
+ 670.058   75.977  8.2642 224.931335  35.100859  7.861
+1031.985 1072.640  5.5063 251.832276  42.238914  6.096
+1150.005   68.707  8.4126 222.864716  44.928498  8.399
+ 866.961 1059.411  3.5912 250.724021  38.922257  3.577
+ 203.901 1062.275  8.1353 248.338291  25.689697  8.390
+1009.692 1069.823  8.3230 251.647876  41.792286  8.005
+1727.415 1069.376  7.4820 256.028014  55.975891  9.435
+1083.571 1066.671  8.3468 251.934384  43.310497  8.705
+ 952.322 1065.920  8.4607 251.274115  40.638184  8.175
+ 656.987 1061.387  8.1242 249.949238  34.625384  7.941
+ 734.492 1062.727  7.4439 250.269095  36.201198  7.319
+ 699.979 1050.934  7.6200 249.834957  35.532235  8.336
+1213.018 1055.635  4.9818 252.309477  45.983892  8.848
+1246.101 1055.651  6.9898 252.497504  46.649075  7.045
+1328.090 1046.764  7.9979 252.713179  48.343769  7.892
+ 699.782 1054.585  8.1298 249.938194  35.515504  7.635
+1039.180 1054.804  8.5467 251.382868  42.447196  8.198
+ 788.523 1046.277  7.9359 250.064309  37.355649  7.891
+1117.842 1037.203  8.2075 251.285478  44.113335  8.061
+1075.164 1045.482  6.1448 251.299144  43.217173  6.226
+ 827.960 1035.506  8.6012 249.940911  38.196607  8.357
+1298.822 1034.748  8.6515 252.179581  47.798368  8.428
+ 974.497 1034.928  8.4335 250.540550  41.195277  8.139
+1320.102 1033.666  7.8227 252.272533  48.235477  7.508
+1085.543 1032.092  8.5486 250.984538  43.475320  9.039
+1190.165 1026.825  8.7460 251.346888  45.623086  8.686
+ 720.476 1019.724  6.9924 249.132003  36.039935  7.265
+ 834.222 1028.520  7.6541 249.787309  38.344987  7.429
+1355.842 1009.142  8.6162 251.720718  49.057486  8.640
+ 791.052 1018.515  7.7982 249.361029  37.490351  7.801
+1283.029 1018.309  8.0237 251.599232  47.543303  8.048
+1032.955 1014.037  7.4827 250.236493  42.461749  7.695
+1017.689 1014.321  8.1387 250.175483  42.145343  8.056

src/figures/stvid/data/2022-08-23T04:16:26.633_48473_catalog.dat

@@ -0,0 +1 @@
+48473 21 040AX  9999 G 20220823041631625 17 25 1533406+483563 37 S

src/figures/stvid/data/2022-08-23T04:16:26.633_52718_catalog.dat

@@ -0,0 +1 @@
+52718 22 056C   9999 G 20220823041631625 17 25 1527277+381243 37 S

src/figures/stvid/data/2022-08-23T04:16:26.633_90000_unid.dat

@@ -0,0 +1 @@
+90000 22 500A   9999 G 20220823041631625 17 25 1457613+535844 37 S

src/figures/stvid/data/2022-08-23T04:16:26.633_hough.csv

@@ -0,0 +1,4 @@
+ax,ay,az,bx,by,bz,n
+1585.699766,186.468458,51.073014,0.879795,0.416052,0.229917,3424
+794.849123,355.614035,48.596491,0.780147,-0.382158,0.495304,285
+1297.660777,432.469965,52.989399,0.923059,0.193205,0.332617,283