Physics – Geophysics
Scientific paper
Nov 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jats...37.2545f&link_type=abstract
Journal of the Atmospheric Sciences, vol. 37, Nov. 1980, p. 2545-2567. Research supported by the Science Research Council of En
Physics
Geophysics
221
Atmospheric Models, Geophysics, Solar Terrestrial Interactions, Thermosphere, Diurnal Variations, Far Ultraviolet Radiation, Meridional Flow, Three Dimensional Flow
Scientific paper
A global, three-dimensional, time-dependent numerical model of the thermosphere was constructed to simulate the dynamical behavior of the earth's thermosphere under various geophysical conditions. The model can simulate thermospheric dynamics by considering only the three processes which deposit energy, or energy and momentum in the thermosphere. The simulations can be made under various solar and geomagnetic conditions using one major and ubiquitous source due to solar u.v. and e.u.v. radiation, and an additional geomagnetic source of energy and momentum due to a polar electric field.
Fuller-Rowell Tim J.
Rees David
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