Jacchia-Bowman Atmospheric Density Model

Computation of the total mass-desnity of atmosphere using Jacchia-Bowman model

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Updated Wed, 14 Dec 2022 13:34:46 +0000

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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:

Cite As

Meysam Mahooti (2023). Jacchia-Bowman Atmospheric Density Model (https://www.mathworks.com/matlabcentral/fileexchange/56163-jacchia-bowman-atmospheric-density-model), MATLAB Central File Exchange. Retrieved .

MATLAB Release Compatibility
Created with R2021b
Compatible with any release
Platform Compatibility
Windows macOS Linux

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Version Published Release Notes
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