The Structure and Dynamics of the Solar Corona and Inner Heliosphere

Details The Structure and Dynamics of the Solar Corona and Inner Heliosphere The Structure and Dynamics of the Solar Corona and Inner Heliosphere

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002stin...0267741m&link_type=abstract

Technical Report, SAIC-01/8013:APPAT-280

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Solar Corona, Magnetohydrodynamics, Heliosphere, Mathematical Models, Solar Eclipses, Stellar Structure, Computerized Simulation

Scientific paper

This report covers technical progress during the fourth quarter of the second year of NASA Sun-Earth Connections Theory Program (SECTP) contract "The Structure and Dynamics of the Solar Corona and Inner Heliosphere," NAS5-99188, between NASA and Science Applications International Corporation (SAIC), and covers the period May 16, 2001 to August 15, 2001. Under this contract SAIC and the University of California, Irvine (UCI) have conducted research into theoretical modeling of active regions, the solar corona, and the inner heliosphere, using the MHD (magnetohydrodynamic) model.

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