MHD Modeling of the Interaction of the Solar Wind With Venus

Details MHD Modeling of the Interaction of the Solar Wind With Venus MHD Modeling of the Interaction of the Solar Wind With Venus

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996sri..reptt....s&link_type=abstract

Technical Report, Southwest Research Inst. San Antonio, TX United States

Computer Science

Numerical Analysis

Interplanetary Magnetic Fields, Venus (Planet), Magnetohydrodynamics, Solar Wind, Numerical Analysis, Solar Planetary Interactions, Bow Waves, Flow Velocity, Shock Waves, Three Dimensional Models, Magnetic Effects, Planetary Magnetotails, Two Dimensional Models

Scientific paper

The primary objective of this research program is to improve our understanding of the physical processes occurring in the interaction of the solar wind with Venus. This will be accomplished through the use of numerical solutions of the two- and three-dimensional magnetohydrodynamic (MHD) equations and through comparisons of the computed results with available observations. A large portion of this effort involves the study of processes due to the presence of the magnetic field and the effects of mass loading. Published papers are included in the appendix.

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