Comparable energy release rates at the origin of small and large solar bursts

Details Comparable energy release rates at the origin of small and large solar bursts Comparable energy release rates at the origin of small and large solar bursts

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985stin...8617254k&link_type=abstract

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Physics

Microwaves, Solar Flares, Solar Flux, X Rays, Magnetohydrodynamic Stability, Solar Physics

Scientific paper

The discovery that the simplest impulsive solar bursts at microwaves and hard X-rays have time scales in the range of 10-100 milliseconds suggest that the energy release rates in such small events are comparable to rates attributed to large events. This condition may be reconciled to the concept that observed burst fluxes in solar events are the convolution of many fast primary energetic injections, at various repetition rates.

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