Magnetohydrodynamic simulation of coronal mass ejections into the solar wind

Details Magnetohydrodynamic simulation of coronal mass ejections into the solar wind Magnetohydrodynamic simulation of coronal mass ejections into the solar wind

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978clus.nasa..367d&link_type=abstract

In JPL A Close-up of the Sun p 367-387 (SEE N78-32964 23-92)

Physics

Computerized Simulation, Density Wave Model, Magnetic Fields, Plasma Flux Measurement, Solar Corona, Magnetohydrodynamic Flow, Mathematical Models, Solar Activity, Solar Wind

Scientific paper

A state of the art fluid continuum technique to describe the MHD transient response of the corona below 10 solar radii during two well observed events (flares on 21 August 1973 and 5 September 1973) is reviewed. It is concluded that the computer simulation should be subjected to in situ verification of as many of its initial assumptions as possible. Its ability to provide a rational basis for physical understanding of mass ejections suggests its use as one of the tools used in the planning and analysis of such encounter missions.

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