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Jacchia-Bowman Atmospheric Density Model

version 2.0.0.0 (17.8 MB) by Meysam Mahooti
Computation of the total mass-desnity of atmosphere using Jacchia-Bowman model

12 Downloads

Updated 03 Feb 2018

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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 (DE430) to improve accuracy of the model.
References:
http://sol.spacenvironment.net/jb2008/
http://ssd.jpl.nasa.gov/?ephemerides
http://www.iausofa.org/
http://celestrak.com/SpaceData/

Comments and Ratings (7)

marzieh

zz xx

terry moore

Demi Moore

Updates

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.

1.1.0.0

Jacchia-Bowman 2008 model is added.

MATLAB Release Compatibility
Created with R2017b
Compatible with any release
Platform Compatibility
Windows macOS Linux