Statistics – Computation
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985rmai.reptq....s&link_type=abstract
Quarterly Progress Report Resource Management Associates, Inc., Lafayette, CA.
Statistics
Computation
Computation, Gas Dynamics, Magnetohydrodynamics, Solar Wind, Terrestrial Planets, Three Dimensional Models, Algorithms, Computer Programs, Flow Distribution, Mathematical Models, Solar Terrestrial Interactions
Scientific paper
The development of a global, 3-D magnetohydrodynamic computational model is described. This model is used to quantitatively describe the detailed continuum field and plasma interaction process of the solar wind with cometary and planetary magneto/ionopause shapes. The present solar wind/terrestrial planet interaction (Level 1) model (which is based on an axisymmetric gas dynamic plus frozen field approximation to the full MHD equations) is extended to a full 3-D gas dynamic (Level 2) approximation. A mass loading capability in the Level 1 interaction model is implemented.
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