On the possibility of the solar flare energy accumulation in the vicinity of a singular line

Details On the possibility of the solar flare energy accumulation in the vicinity of a singular line On the possibility of the solar flare energy accumulation in the vicinity of a singular line

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..123..285p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 123, no. 2, 1989, p. 285-308.

Physics

14

Current Sheets, Magnetohydrodynamic Stability, Solar Flares, Solar Magnetic Field, Computerized Simulation, Magnetic Field Configurations, Magnetic Field Reconnection, Solar Corona

Scientific paper

The energy of a solar flare can be accumulated as the magnetic energy of the current sheet created in the vicinity of a magnetic field singular line by the focusing of disturbances. Conditions which define the singular line in general were obtained using the properties of a singular line as it focuses disturbances. Numerical simulations and an analytical model show the possibility of creating a stable current sheet which becomes unstable after quasi-stationary evolution.

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