Time scales of solar microwave bursts and scenarios of flare energy release

Details Time scales of solar microwave bursts and scenarios of flare energy release Time scales of solar microwave bursts and scenarios of flare energy release

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.285..169k&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Reconnection in Space Plasma, Volume 2 p 169-173 (SEE N89-24974 1

Physics

1

Microwave Emission, Solar Flares, Solar Radio Bursts, Magnetic Flux, Magnetohydrodynamic Stability

Scientific paper

Based on observational evidence that characteristic time scales of different solar microwave burst types are distributed over a wide range (0.001 to 10.000 sec), different mechanisms of energy release are considered to account for the impulsive flux increase (time scale less than 1000 sec). The coalescence instability is found to be a promising candidate to combine sufficiently short time scales with substantial energy release.

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