An Improvement Of TD-88 Model For The Terrestrial Atmosphere

Details An Improvement Of TD-88 Model For The Terrestrial Atmosphere An Improvement Of TD-88 Model For The Terrestrial Atmosphere

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..10e..40s&link_type=abstract

Progress in Planetary Exploration Missions, 26th meeting of the IAU, Joint Discussion 10, 21-22 August 2006, Prague, Czech Repub

Astronomy and Astrophysics

Astronomy

Scientific paper

In this paper one examines air densities derived from our realization of aeronomic atmosphere models based on accelerometer measurements from satellites in a low Earth's orbit (LEO). Using the adapted MSISe-00 and TD-88 algorithms the comparison parameters are derived. The first results indicate that TD-88 model (L. Sehnal, 1988, Bull. Astron. Inst. Czechosl. 39, 120-127) developed for the Earth's atmosphere can be improved. By applying the least squares the TD-88 model parameters are modified for the purposes of improving the agreement between the experimental (obtained from MSISe-00 model) and theoretical (TD-88 model) values and of enlarging the calculation speed. On the basis of Sehnal's analytic model concerning the Martian atmosphere a preparation for formation of a TD model for the Martian atmosphere is simultaneously done in this paper.

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