Development of a computational model for predicting solar wind flows past nonmagnetic terrestrial planets

Details Development of a computational model for predicting solar wind flows past nonmagnetic terrestrial planets Development of a computational model for predicting solar wind flows past nonmagnetic terrestrial planets

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983neri.rept.....s&link_type=abstract

Final Report, Jul. 1978 - Aug. 1983 Nielsen Engineering and Research, Inc., Mountain View, CA.

Statistics

Computation

Magnetic Fields, Solar Wind, Terrestrial Planets, Magnetohydrodynamics, Planetary Atmospheres, Planetary Ionospheres, Wind Measurement

Scientific paper

A computational model for the determination of the detailed plasma and magnetic field properties of the global interaction of the solar wind with nonmagnetic terrestrial planetary obstacles is described. The theoretical method is based on an established single fluid, steady, dissipationless, magnetohydrodynamic continuum model, and is appropriate for the calculation of supersonic, super-Alfvenic solar wind flow past terrestrial ionospheres.

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