GitHub - USNavalResearchLaboratory/TrackerComponentLibrary: This is a collection of Matlab functions that are useful in the development of target tracking algorithms. (original) (raw)

Tracker Component Library Release 6.1, September 2024 https://github.com/USNavalResearchLaboratory/TrackerComponentLibrary

A paper describing a number of features of the library is
D. F. Crouse, "The Tracker Component Library: Free Routines for Rapid Prototyping," IEEE Aerospace and Electronic Systems Magazine, vol. 32, no. 5, pp. 18-27, May. 2017.

Those looking for magnetic field synthesis code might want to look at ./Sample Code/Magnetic Models/ .

These are the release notes for the version 6.1 of the Tracker Component Library. The Tracker Component Library is a collection of Matlab routines for simulating and tracking targets in various scenarios. Due to the complexity of the target tracking problem, a great many routines can find use in other areas including combinatorics, astronomy, and statistics.

Making this code available and open source is in the spirit of the Federal Source Code Policy, which is OMB M-16-21, which is given inhttps://www.whitehouse.gov/wp-content/uploads/legacy_drupal_files/omb/memoranda/2016/m_16_21.pdf https://code.gov/

Those looking to get a quick idea of a very simple end-to-end tracking algorithm (track initiation, data association, maintenance, and termination) might want to look at ./Sample Code/Basic Tracking Examples/demo2DIntegratedDataAssociation.m to see an example of a complete GNN-JIPDAF tracker run on a simple 2D tracking scenario, which can be easily transformed into a normal JIPDAF by changing a single parameter. The tracker is made from the modular components of the library. A lot of other sample code is also provided to demonstrate the use of other parts of the library.

To use the full library, add the library and all of its subfolders to your active path in Matlab. Some functions are available as C/C++ files for use in Matlab either because they use third-party libraries (and must be compiled to be used) or because the native Matlab implementations provided are too slow in certain circumstances. These files can be compiled by running the CompileCLibraries function. Precompiled code is not distributed with the library. Note that a C/C++ compiler supported by Matlab must be installed. See below for comments regarding compilation.

Note that NASA's ephemerides are nolonger distributed with the library on GitHub due to the file size. Additionally, the GSHHG data for plotting maps and determining if a point is on land is not distributed with the library. See below for where to download these free datasets.

SOME OF THE CHANGES SINCE VERSION 6.0:

Bug fixes, notably the CDF in the chi squared distribution now works over a much wider range of values of the noncentrality parameter. Previously, values as low as 500 were problematic.
All of the detection statistics classes and related functions have been redone to handle a more common normalization and have better comments. One can now choose the normalization to use. Also, SwerlingISqLawD now has new methods for the first and second derivative of the PDF with respect to the average SNR.
extractSubPlots To let one to pull sub plots out of figures in Matlab that have already been plotted with suplots.
Added functions for displaying maps and for determining whether a point is on land or not. For example, run the sample code in the comments to pointIsOnLand. Note that these functions rely on the data from the GSHHG, which is not provided, but which can be downloaded fromhttps://www.ngdc.noaa.gov/mgg/shorelines/ . The binary archive gshhg-bin.zip should be placed in Misc/Maps/data.
Added an example to the comments of expRateLikeGammaConjUpdate on how to use the function.
The inputs and outputs of pseudoInverseDerivative have been reformulated to be more useful.
Added the Erlang distribution in ErlangD and a distribution for a weighted sum of noncentral chi squared random variables plus an optional normal in ChiSquaredSumD.
New Lorentz transformation functions along with gradients and Hessians.
New functions related to simple refraction models. Specifically, atmosExpDecayConst4Refrac and approxRefractivity.
Combinatorial functions for involutions: genAllInvolutions, numPureInvolutions, numFixedPointInvolutions, isPureInvolution, and genAllPureInvolutions.
The C implementation of clipPolygonSH2D was buggy and was removed.
In all, 55 new functions (not all in unique files) added and one removed.

COMPILED CODE:

The compilation of the library has been tested under Matlab2024a under Windows 10 using minGW64 and Microsoft Visual C++ 2022. The code will probably compile under Mac OS X and Linux. Precompiled code is not distributed with the library.

EXTERNAL SOLVERS:

Almost all of the function in the library work without any external resources. However, the folder ./Mathematical_Functions/Polynomials/Generic_Multivariate_Polynomials/ contains the function solvePolySysWithExtProg. This is an interface to external solvers for simultaneous multivariate polynomial systems. The solvers are external programs and are not included. Though the functions polyRootsMultiDim and solveQuadBivarEq can solver certain types of simultaneous multivariate polynomials, they are limited. For more general systems, an external solver is the best choice. The functions polyMeasConvert, polyMeasConvertAsync, and DopplerOnlyInit6D are located in subfolders entitled 'Uses_External_Solver" and use the function solvePolySysWithExtProg. Supported external solvers for the function solvePolySysWithExtProg are PHCpack, Bertini, and the certified solver in Macaulay2. Note that Macaulay2 tends to fail more often than the other solvers.

The solvers can be downloaded from: PHCpack for Mac OS X, Windows and Linux:http://homepages.math.uic.edu/~jan/download.htmlBertini (version 1.5) for Mac OS X and Linux and Windows, only with Cygwin:https://bertini.nd.edu/download.htmlMacaulay2 for Mac OS X, Linux, and Windows:https://www.macaulay2.com/

For the external solvers to work, they need to be added to the search path used in Matlab so that the phs/bertini/m2 commands can be called using the system command in Matlab.

DATA SOURCES:

If the library was downloaded without associated data files for solar system ephemerides as well as magnetic, gravitational and terrain models, then the relevant data files will have to be downloaded The original sources of the data are:

Earth2014 terrain model:https://geodesy.curtin.edu.au/research/harmonic-topography/The files Earth2014.BED2014.degree2160.bshc, Earth2014.ICE2014.degree2160.bshc, Earth2014.RET2014.degree2160.bshc, Earth2014.SUR2014.degree2160.bshc, Earth2014.TBI2014.degree2160.bshc should be placed into ./Terrain/data . Though data files to degree and order 10,800 are also available, they are not currently supported as the function spherHarmonicEval does not use extended precision arithmetic, which is required to avoid overflows when using the model.
EGM2008 terrain model (The DTM2006.0 model):http://earth-info.nga.mil/GandG/wgs84/gravitymod/egm2008/first_release.htmlThe file Coeff_Height_and_Depth_to2190_DTM2006.0 should be placed into ./Terrain/data . The first time using the getEGM2008TerrainCoeffs function will be significantly slower than subsequent calls, assuming the full model is loaded the first time.
The EMM2017 magnetic field coefficients:https://www.ngdc.noaa.gov/geomag/EMM/The coefficients are included with the software that is provided. The files having names like EMM2015.COF and EMM2000.COF should all be zipped into an archive with the name EMM_Coefficients.zip and placed in ./Magnetism/data . The files with names like EMM2015SV.COF andEMM2000SV.COF should all be zipped into an archive with the name EMM_Secular_Variations.zip and placed into ./Magnetism/data . If all of the data for a single year is loaded, then a .mat file containing the data is placed in the data folder to speed up subsequent calls to the function.
The IGRF13 magnetic field coefficients:http://www.ngdc.noaa.gov/IAGA/vmod/igrf.htmlThe file http://www.ngdc.noaa.gov/IAGA/vmod/igrf13coeffs.txt can be downloaded and placed into the folder ./Magnetism/data .
The WMM2020 magnetic field coefficients:https://www.ngdc.noaa.gov/geomag/WMM/The coefficient file WMM2020COF.zip shown be downloaded, unzipped and the file WMM.COF placed into ./Magnetism/data .
EGM2008 gravitational coefficientshttp://earth-info.nga.mil/GandG/wgs84/gravitymod/egm2008/egm08_wgs84.htmlDownload the file EGM2008_to2190_TideFree.gz, which is under "EGM2008 Tide Free Spherical Harmonic Coefficients". Decompress the file and place it in ./Gravity/data .
EGM96 gravitational coefficientshttp://earth-info.nga.mil/GandG/wgs84/gravitymod/egm96/egm96.htmlThe file egm96.z should be downloaded and decompressed, resulting in a file names egm96 without an extension, which should be placed in ./Gravity/data .
EGM2008 parameters needed to convert height anomalies to geoid undulations:http://earth-info.nga.mil/GandG/wgs84/gravitymod/egm2008/egm08_wgs84.htmlThe "Correction Model" file Zeta-to-N_to2160_egm2008.gz should be downloaded, ungzipped and placed in ./Gravity/data .
EGM96 parameters needed to convert height anomalies to geoid undulations:http://earth-info.nga.mil/GandG/wgs84/gravitymod/egm96/egm96.htmlThe file corrcoef.z should be decompressed and placed in ./Gravity/data .
NASA JPL's DE440t planetary/solar/lunar ephemerideshttps://ssd.jpl.nasa.gov/ftp/eph/planets/Linux/de440t/The file linux_p1550p2650.440t should be downloaded and placed in ./Astronomical Code/data for use by the readJPLEphem function. The readJPLEphem function can read other NASA ephemerides, but the DE440t set are the default.
NASA JPL's GL0900C gravitational model of the Moonhttp://pds-geosciences.wustl.edu/missions/grail/default.htmDownload the file jggrx_0900c_sha.tab and place it in ./Gravity/data .
The FES2004 tide model of the effects of ocean Earth tides.http://maia.usno.navy.mil/conv2010/convupdt/convupdt_c6.htmlThe file fes2004_Cnm-Snm.dat should be downloaded and placed in ./Gravity/Tides/data .
The Hipparcos 2 Star Cataloghttp://cdsarc.u-strasbg.fr/viz-bin/Cat?I/311Place the file hip2.dat in ./Astronomical Code/data .
A 5400X2700 image of the Earth. The August, Blue Marble Next Generation with Topography and Bathymetry from NASA:https://visibleearth.nasa.gov/images/73776/august-blue-marble-next-generation-w-topography-and-bathymetryName the file NASABlueMarble.jpg and place the file in Misc/data . This is used as the default map to show on the Earth given by the plotMapOnEllipsoid function.
The Global Self-consistent, Hierarchical, High-resolution Geography Databasehttps://www.ngdc.noaa.gov/mgg/shorelines/Download the zipped binary formatted archive. The file is gshhg-bin-2.3.7.zip. It should be renamed to gshhg-bin.zip and be placed in Misc/Maps/data. Note that the claims a weak copyleft license.

September 2024 David F. Crouse, Naval Research Laboratory, Washington D.C.
(UNCLASSIFIED) DISTRIBUTION STATEMENT A. Approved for public release. Distribution is unlimited.

LICENSE:

The source code is in the public domain and not licensed or under copyright. The information and software may be used freely by the public. As required by 17 U.S.C. 403, third parties producing copyrighted works consisting predominantly of the material produced by U.S. government agencies must provide notice with such work(s) identifying the U.S. Government material incorporated and stating that such material is not subject to copyright protection.

Derived works shall not identify themselves in a manner that implies an endorsement by or an affiliation with the Naval Research Laboratory.

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