Computer Science
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982icar...51..440h&link_type=abstract
(International Conference on the Venus Environment, Palo Alto, CA, Nov. 1-6, 1981.) Icarus, vol. 51, Aug. 1982, p. 440-447.
Computer Science
14
Atmospheric Composition, Exosphere, Hydrogen Atoms, Thermosphere, Venus Atmosphere, Wind Effects, Atmospheric Models, Lyman Alpha Radiation, Monte Carlo Method, Pioneer Venus 1 Spacecraft, Radial Distribution
Scientific paper
Monte Carlo models of the distribution of atomic hydrogen in the exosphere of Venus were computed which simulate the effects of thermospheric winds and the production of a 'hot' hydrogen component by charge exchange of H(+) and H and Q in the exosphere, as well as classic exospheric processes. A thermosphere wind system that is approximated by a retrograde rotating component with equatorial speed of 100 m/sec superimposed on a diurnal solar tide with cross-terminator day-to-night winds of 200 m/sec is shown to be compatible with the thermospheric hydrogen distribution deduced from Pioneer Venus orbiter measurements.
Hodges Richard Jr. R.
Tinsley Brian A.
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