Nonlinear magnetohydrodynamics in solar flares.

Details Nonlinear magnetohydrodynamics in solar flares. Nonlinear magnetohydrodynamics in solar flares.

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997jkps...31s.210k&link_type=abstract

Journal of the Korean Physical Society, Vol. 31, p. S210 - S213

Physics

Solar Flares: Magnetohydrodynamics

Scientific paper

The nonlinear magnetohydrodynamics (MHD) in solar flares is considered using two dimensional numerical simulations. The results are analyzed based on the bifurcation theory of the linear force-free field (Kusano, et al. (1995). The simulation results show that a transition from a loop type configuration into an island type configuration indeed takes place as the bifurcation theory predicted. The dependence of the transition dynamics on the resistivity is considered in detail.

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