Jacchia-Bowman Atmospheric Density Model

Versión 2.2.0 (94,8 MB) por Meysam Mahooti
Computation of the total mass density of the atmosphere using the Jacchia-Bowman model
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Actualizado 10 dic 2024

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Dynamic modeling of a LEO satellite's motion requires precise computation of atmospheric density for drag effect modeling.​ Here, the Jacchia-Bowman 2006 and 2008 atmospheric models are used to calculate the total mass density of the atmosphere. The position of the Sun is computed using the JPL Ephemerides (DE440) to improve the accuracy of the model.
References:
https://sol.spacenvironment.net/JB2008/indices/SOLFSMY.TXT
https://sol.spacenvironment.net/JB2008/indices/SOLRESAP.TXT
https://sol.spacenvironment.net/JB2008/indices/DTCFILE.TXT
https://ssd.jpl.nasa.gov/planets/eph_export.html
http://celestrak.org/SpaceData/EOP-All.txt
http://www.iausofa.org/

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Meysam Mahooti (2025). Jacchia-Bowman Atmospheric Density Model (https://es.mathworks.com/matlabcentral/fileexchange/56163-jacchia-bowman-atmospheric-density-model), MATLAB Central File Exchange. Recuperado .

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Se creó con R2024a
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Jacchia-Bowman Atmospheric Density Model_2.2.0

Versión Publicado Notas de la versión
2.2.0

test_JB2006.m, test_JB2008, and JPL_Eph_DE440.m were modified.
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