Nonlinear computations of a solar flare model

Details Nonlinear computations of a solar flare model Nonlinear computations of a solar flare model

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phfl...27.2063s&link_type=abstract

Physics of Fluids (ISSN 0031-9171), vol. 27, Aug. 1984, p. 2063-2066. Research supported by the U.S. Department of Energy and NA

Physics

6

Solar Flares, Tearing Modes (Plasmas), Computerized Simulation, Equations Of Motion, Nonlinear Equations

Scientific paper

A cylindrical axisymmetric tearing mode model for solar flares is
investigated numerically. Large magnetic energy release only occurs when
there are at least two mode rational surfaces in the current-carrying
plasma.

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