Magnetic fields in the Venus ionosphere

Details Magnetic fields in the Venus ionosphere Magnetic fields in the Venus ionosphere

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kosis..26..770k&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 26, Sept.-Oct. 1988, p. 770-784. In Russian.

Physics

Planetary Ionospheres, Planetary Magnetic Fields, Plasma Dynamics, Venus Atmosphere, Convective Flow, Daytime, Lines Of Force, Magnetic Effects

Scientific paper

The formation and evolution of the large-scale magnetic field and magnetic ropes in the Venus ionosphere are analyzed in the framework of the plasma-convection hypothesis. It is suggested that the observed large-scale field or magnetic belt in the Venus dayside ionosphere is the result of the solar wind's magnetic field being 'pushed' into the ionosphere; the upper boundary of the magnetic belt passes near the upper boundary of the photochemical-equilibrium region.

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