Global Magnetohydrodynamic Modeling of the Solar Corona

Details Global Magnetohydrodynamic Modeling of the Solar Corona Global Magnetohydrodynamic Modeling of the Solar Corona

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001stin...0188238l&link_type=abstract

Technical Report, SAIC-01/8007:APPAT-274; Rept-01-0157-04-1503-000

Computer Science

Solar Corona, Coronal Mass Ejection, Magnetohydrodynamics, Computerized Simulation, Three Dimensional Models, Magnetic Storms, Solar Wind, Solar Terrestrial Interactions, Solar Activity Effects

Scientific paper

This report describes the progress made in the investigation of the
solar corona using magnetohydrodynamic (MHD) simulations. Coronal mass
ejections (CME) are believed to be the primary cause of nonrecurrent
geomagnetic storms and these have been investigated through the use of
three-dimensional computer simulation.

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