Dynamic modeling of the solar atmosphere

Details Dynamic modeling of the solar atmosphere Dynamic modeling of the solar atmosphere

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990eostr..71..791m&link_type=abstract

EOS (ISSN 0096-3941), vol. 71, July 10, 1990, p. 791-796. Research supported by NASA and U.S. Navy.

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Coronal Loops, Emission Spectra, Solar Atmosphere, Solar Corona, Solar Magnetic Field, Thermal Stability, Computational Grids, Computerized Simulation, Magnetic Field Reconnection, Magnetohydrodynamic Turbulence, Solar Wind

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A brief review is presented of work done over the last eight years investigating the fundamental physics of plasmas and magnetic fields under conditions similar to those that are thought to be present in the outer layers of the solar atmosphere, including the transition region and the corona. The models used to study the coronal structures and the thermal instability in the solar atmosphere are discussed. The results of studies of magnetic energy release in the corona and MHD turbulence in the solar wind are examined.

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