Physics
Scientific paper
Mar 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979p%26ss...27..255w&link_type=abstract
Planetary and Space Science, vol. 27, Mar. 1979, p. 255-264.
Physics
11
Interplanetary Medium, Magnetohydrodynamic Flow, Solar Wind, Two Dimensional Flow, Conservation Equations, Magnetic Disturbances, Magnetic Field Configurations, Solar Flares, Time Dependence, Two Dimensional Models
Scientific paper
A two-dimensional, time-dependent nonlinear MHD model is used to simulate the general features of multiply-interacting, transient solar wind flows. The major advantage of the two-dimensional model over the one-dimensional one is the proper consideration of azimuthal gradients. In addition, the new model can provide contour maps for disturbed plasma properties in the equatorial plane, thereby enabling one to perform essential tests of the physical assumptions through direct comparison with space probe data.
Dryer Murray
Han Ming Sheng
Wu Shi Tsan
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