Jacchia-Bowman Atmospheric Density Model

Versión 2.1.2 (94,7 MB) por Meysam Mahooti
Computation of the total mass-desnity of atmosphere using Jacchia-Bowman model
5.0
(11)
1,4K Descargas
Actualizado 14 dic 2022

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Dynamic modeling of a LEO satellite's motion requires precise computation of atmospheric density for drag effect modeling. Here, Jacchia-Bowman 2006 and 2008 atmospheric models are used to calculate the total mass-desnity of atmosphere. Position of the Sun is computed by JPL Ephemerides (DE440) to improve accuracy of the model.
References:
http://sol.spacenvironment.net/jb2008/indices.html
https://ssd.jpl.nasa.gov/planets/eph_export.html
http://www.iausofa.org/
http://celestrak.org/SpaceData/EOP-All.txt

Citar como

Meysam Mahooti (2024). Jacchia-Bowman Atmospheric Density Model (https://www.mathworks.com/matlabcentral/fileexchange/56163-jacchia-bowman-atmospheric-density-model), MATLAB Central File Exchange. Recuperado .

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Se creó con R2021b
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Jacchia-Bowman Atmospheric Density Model

Versión Publicado Notas de la versión
2.1.2

It was revised on 2022-12-14.
2.1.1

test_JB2006.m is modified.
2.1.0

JB2006.m and JB2008.m are modified.
2.0.0.0

IERS.m, test_JB2006.m, and test_JB2008.m are modified to decrease CPU time.
1.1.0.0

The image is added.
Jacchia-Bowman 2008 model is added.
1.0.0.0