Physics
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rpsct...1...77b&link_type=abstract
In its JPRS Report: Science and Technology. USSR: Space p 77 (SEE N87-29547 24-12) Transl. into ENGLISH from Kosmicheskiye Issle
Physics
Charge Exchange, Coronas, Magnetic Fields, Planetary Atmospheres, Plasma-Particle Interactions, Solar Wind, Venus (Planet), Bow Waves, Heavy Ions, Photoionization
Scientific paper
The flow of the solar wind around Venus was modelled numerically, taking into account the loading of the flow by heavy ions forming during photoionization of the neutral oxygen corona of that planet. It is shown that this effect can explain a number of aspects of interaction between the solar wind and the planet which until now have not been clear, such as the position of the bow shock, characteristics of the solar wind flow and the magnetic field behind the front.
Breus Tamara K.
Krymskiy A. M.
Mitnitskiy Ya. V.
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