Comparison of thermospheric density models at 285 km

Details Comparison of thermospheric density models at 285 km Comparison of thermospheric density models at 285 km

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988p%26ss...36.1121s&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 36, Nov. 1988, p. 1121-1123.

Computer Science

3

Atmospheric Models, Harmonic Functions, Legendre Functions, Spherical Harmonics, Thermosphere, Annual Variations, Atmospheric Density, Diurnal Variations, Exponential Functions, Solar Flux, Upper Atmosphere

Scientific paper

A thermospheric density model is proposed which provides a reliable description of the thermospheric total density distribution and variations. It is noted that the defining coefficients should be improved near the model height limits of 200 and 500 km. The model is found to compare favorably with the empirical model of Moore and Boulton (1986) for a height of 285 km.

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