Physics
Scientific paper
Jul 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86...33p&link_type=abstract
(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un
Physics
12
Magnetoplasmadynamics, Solar Flares, Solar Magnetic Field, Coronal Loops, Current Sheets, Magnetic Field Configurations, Magnetohydrodynamic Stability, Shock Waves, Solar Flux
Scientific paper
The basic processes of evaporation and magnetic reconnection have recently been developed in much greater detail. They may be important in the two main types of flaring event, namely simple-loop flares and two-ribbon flares. The first type could be produced by kink instability, thermal nonequilibrium, or emerging flux. The second type is thought to be the result of an eruptive MHD instability that is either spontaneous or triggered from outside. After the eruption the magnetic field lines that have been blown open reconnect back down in a way that has now been simulated numerically.
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