Spatial structure of flare-associated perturbations in the solar wind simulated by a two-dimensional numerical MHD model

Details Spatial structure of flare-associated perturbations in the solar wind simulated by a two-dimensional numerical MHD model Spatial structure of flare-associated perturbations in the solar wind simulated by a two-dimensional numerical MHD model

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jgr....86..525d&link_type=ejournal

Journal of Geophysical Research, vol. 86, Feb. 1, 1981, p. 525-534.

Physics

45

Magnetohydrodynamic Flow, Magnetohydrodynamic Stability, Plasma Oscillations, Solar Flares, Solar Wind Velocity, Two Dimensional Models, Interplanetary Magnetic Fields, Mathematical Models, Propagation Velocity, Shock Fronts, Shock Wave Propagation, Time Response

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