An explanation for the flare frequency-energy dependence

Details An explanation for the flare frequency-energy dependence An explanation for the flare frequency-energy dependence

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..151..195l&link_type=abstract

Solar Physics, vol. 151, no. 1, p. 195-198

Physics

21

Current Sheets, Frequency Distribution, Mathematical Models, Plasma Currents, Solar Flares, Solar Corona, Solar Magnetic Field, Solar Wind

Scientific paper

The reconnecting current sheet model for energy accumulation and release during solar flares results in the flare frequency distribution that is a power-law function of total flare energy, with the index 7/4 for sufficiently large energies. The distribution is predicted to be much steeper in the low-energy region, implying the significance of micro- and nanoflares for coronal heating.

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