Physics
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990icar...85..129s&link_type=abstract
Icarus (ISSN 0019-1035), vol. 85, May 1990, p. 129-144. Research supported by the National Natural Science Foundation of China.
Physics
1
Atmospheric Heating, Atmospheric Tides, Venus Atmosphere, Atmospheric Temperature, Diurnal Variations, Linear Equations, Solar Heating, Space Exploration, Vertical Distribution, Venus, Numerical Methods, Tidal Effects, Thermal Properties, Atmsophere, Heating, Parameters, Spacecraft Observations, Pioneer Venus Missions, Models, Torque, Calculations, Solar Effects, Flux, Oscillations, Wind, Temperature, Amplitude, Diurnal Variations, Pressure, Surface, Density, Latitude, Parameters
Scientific paper
The problems which emerge in choosing the basic equations and selecting the atmospheric heating function of the atmosphere during studies of Venus' atmospheric tides are presently approached via the numerical solution of the linear form of the basic equations. An analysis of the results thus obtained indicates that observations of the thermal parameters near the ground are important to the determination of the ground-heating mode of this planet's atmosphere. Pioneer Venus probe data are presently used to construct three heating models; the torque of the atmospheric tides is estimated to be 1.4 x 10 to the 16th J.
Shen Mingmin
Zhang Cheng-Zhi
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