Physics
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992lpico.789r..22c&link_type=abstract
In Lunar and Planetary Inst., Papers Presented to the International Colloquium on Venus p 22-23 (SEE N93-14288 04-91)
Physics
Planetary Ionospheres, Solar Wind, Thermosphere, Venus Atmosphere, Atmospheric Chemistry, Atmospheric Physics, Pioneer Venus Spacecraft
Scientific paper
Our knowledge of the upper atmosphere and ionosphere of Venus and its interaction with the solar wind has advanced dramatically over the last decade, largely due to the data obtained during the Pioneer Venus mission and to the theoretical work that was motivated by this data. Most of this information was obtained during the period 1978 through 1981, when the periapsis of the Pioneer Venus Orbiter (PVO) was still in the measurable atmosphere. However, solar gravitational perturbations will again lower the PVO periapsis into the upper atmosphere in September 1992, prior to the destruction of the spacecraft toward the end of this year. The physics and chemistry of the thermosphere and ionosphere of Venus are reviewed.
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