Numerical MHD simulation of interplanetary shock pairs

Details Numerical MHD simulation of interplanetary shock pairs Numerical MHD simulation of interplanetary shock pairs

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jgr....80.1223s&link_type=abstract

Journal of Geophysical Research, vol. 80, Apr. 1, 1975, p. 1223-1231.

Astronomy and Astrophysics

Astronomy

21

Computerized Simulation, Interplanetary Medium, Magnetohydrodynamic Flow, Shock Wave Propagation, Solar Wind, Astronomical Models, Electron Density (Concentration), Mathematical Models, Pressure Distribution, Radial Velocity, Solar Flares, Solar Wind Velocity

Scientific paper

Two types of theoretical model can be used to study the propagation of shock pairs through the ambient solar wind: ordinary fluid-dynamic (OFD) models and magnetohydrodynamic (MHD) models. In the present analysis, the full set of time-dependent MHD equations of motion is solved numerically. The initial conditions are given by a disturbance of specified form and duration near the sun. The coupling between the radial magnetic field and the polar current density is investigated in detail.

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