Magnetic field in the wake of Venus and the formation of ionospheric holes

Details Magnetic field in the wake of Venus and the formation of ionospheric holes Magnetic field in the wake of Venus and the formation of ionospheric holes

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jgr....90.1385m&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 90, Feb. 1, 1985, p. 1385-1398.

Physics

34

Planetary Ionospheres, Planetary Magnetic Fields, Solar Planetary Interactions, Venus Atmosphere, Interplanetary Magnetic Fields, Ionopause, Magnetic Field Configurations, Solar Wind, Venus, Magnetic Fields, Wakes, Ionosphere, Structure, Formation, Pvo, Magnetosheath, Nightside, Solar Wind, Interplanetary Magnetic Field, Imf, Observations, Pioneer Venus, Orbiters, Latitude, Altitude, Plasma, Flow, Distribution, Deformation, Models

Scientific paper

Magnetic field structures are analyzed for both the ionospheric hole region and the magnetosheath/ionosphere interaction region of the nightside of Venus, in search of possible coupling between these two regimes. A magnetic coordinate system based on the directions of the solar wind and the interplanetary magnetic field is found to order the data reasonably well, allowing consistent superposition of observational data from individual passes of the Pioneer Venus orbiter. The results indicate that the magnetosheath plasma flow in the wake region plays an important role in forming the ionospheric holes through deformation of the nightside ionopause. The results are combined in a model of the three-dimensional magnetic field structure around the ionosphere of Venus.

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