The structure of the Venus ionosphere

Details The structure of the Venus ionosphere The structure of the Venus ionosphere

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ssrv...55...81b&link_type=abstract

Space Science Reviews (ISSN 0038-6308), vol. 55, Jan.-Feb. 1991, p. 81-163.

Computer Science

74

Atmospheric Circulation, Ionopause, Ionospheric Ion Density, Planetary Ionospheres, Solar Planetary Interactions, Venus Atmosphere, Diurnal Variations, Pioneer Venus Spacecraft, Planetary Magnetic Fields, Radio Occultation, Solar Wind, Spatial Distribution, Venus, Ionosphere, Structure, Spacecraft Observations, Pvo Mission, Plasma, Radio Methods, Occultations, Thermal Properties, Composition, Ions, Symmetry, Nightside, Waves, Latitude, Seasonal Variation, Mars, Electrons, Solar Cycles, Ionopause, Stability,

Scientific paper

The morphology and temporal variability of the Venus ionosphere are characterized, reviewing the results of recent theoretical investigations, observations, and in situ measurements, especially by the Pioneer Venus Orbiter (PVO). Consideration is given to the Pioneer mission and orbit evolution, early radio occultation profiles of ionospheric N(e), the mean structure and thermal balance of the ionosphere, the ion composition and its dawn-dusk asymmetry, the small-scale spatial structure on the nightside, latitudinal and seasonal variations, solar-cycle effects, suprathermal electrons and superthermal ions, and the global configuration and stability of the ionopause. Data from a single PVO passage through the ionotail are discussed in detail, examining the implications for ion escape and the solar-cycle and short-term variability. The differences among the terrestrial, Martian, and Venusian ionospheres are outlined; the PVO data base is described; and the sources of measurement error are indicated.

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