A classification scheme for solar flare models

Details A classification scheme for solar flare models A classification scheme for solar flare models

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...67..385s&link_type=abstract

Solar Physics, vol. 67, Sept. 1980, p. 385-392.

Physics

4

Classifications, Free Energy, Magnetic Induction, Solar Flares, Stellar Models, Magnetic Field Configurations, Magnetic Flux, Magnetohydrodynamic Stability, Ohmic Dissipation, Plasma-Electromagnetic Interaction, Resistance Heating, Tables (Data)

Scientific paper

A classification scheme is presented for solar flare models that utilize magnetic free energy currents. The classification scheme is geometry independent and delineates models into two categories: those models utilizing currents flowing parallel to the magnetic induction and those utilizing currents flowing perpendicular to the magnetic induction. This delineation of drivers makes it possible to specify what kinds of plasma-magnetic field configurations should be expected for a given current driver. Further, the delineation of drivers allow identification of both the strengths and the weaknesses of the various models.

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