Physics
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987alab.reptr....w&link_type=abstract
Annual Report, 1 Nov. 1985 - 31 Dec. 1986 Alabama Univ., Huntsville. Dept. of Mechanical Engineering.
Physics
Energy Transfer, Magnetohydrodynamics, Mathematical Models, Solar Activity Effects, Solar Flares, Magnetic Fields, Plasma Density, Solar Corona, Solar Wind
Scientific paper
Theoretical and numerical modeling of solar activity and its effects on the solar atmosphere within the context of magnetohydrodynamics were examined. Specifically, the scientific objectives were concerned with the physical mechanisms for the flare energy build-up and subsequent release. In addition, transport of this energy to the corona and solar wind was also investigated. Well-posed, physically self-consistent, numerical simulation models that are based upon magnetohydrodynamics were sought. A systematic investigation of the basic processes that determine the macroscopic dynamic behavior of solar and heliospheric phenomena was conducted. A total of twenty-three articles were accepted and published in major journals. The major achievements are summarized.
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