Plasma Regimes Around Venus: VEX Insight on the Boundary Separating Solar and Planetary Plasmas.

Details Plasma Regimes Around Venus: VEX Insight on the Boundary Separating Solar and Planetary Plasmas. Plasma Regimes Around Venus: VEX Insight on the Boundary Separating Solar and Planetary Plasmas.

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufm.p42a..04s&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #P42A-04

Physics

2431 Ionosphere/Magnetosphere Interactions (2736), 2756 Planetary Magnetospheres (5443, 5737, 6033), 5443 Magnetospheres (2756), 6295 Venus

Scientific paper

We present data obtained during the Venus first orbits by the ASPERA-4 experiment onboard the VEX spacecraft. The main plasma regimes around the planet are discussed from ions, electrons and magnetic field measurements. The inner region Venusward of the magnetosheath is characterized by a sharp decrease of solar wind ions and the appearance of high fluxes of heavy planetary ions. Closer to the planet, CO2 photoelectrons sign the entry inside ionosphere proper. On the base of these VEX data we discuss the formation of the boundary separating solar and planetary plasmas.

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