The importance of photospheric magnetic field complexity for coronal energy storage

Details The importance of photospheric magnetic field complexity for coronal energy storage The importance of photospheric magnetic field complexity for coronal energy storage

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...66...21v&link_type=abstract

Solar Physics, vol. 66, May 1980, p. 21-28. Research supported by the Nederlandse Organisatie voor Zuiver-Wettenschappelijk Onde

Physics

Electric Current, Energy Storage, Photosphere, Solar Corona, Solar Flares, Solar Magnetic Field, Equilibrium Equations, Magnetic Field Configurations, Solar Atmosphere, Solar X-Rays

Scientific paper

Possibilities for the storage of energy in coronal electric currents in different magnetic background field configurations are investigated in the framework of the solar flare energy build-up model of Van Tend and Kuperus (1978). The results are compared to characteristics of filaments and X-ray loops. Empirical flare predictors are interpreted theoretically.

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