An explanation of transient brightenings by magnetic reconnection theory

Details An explanation of transient brightenings by magnetic reconnection theory An explanation of transient brightenings by magnetic reconnection theory

Jun 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997soph..173..103l&link_type=abstract

Solar Physics, Vol. 173, No. 1, p. 103 - 109

Physics

Solar Active Regions: X-Ray Transients, Solar Activity: Magnetohydrodynamics

Scientific paper

It has been discovered that active regions commonly have numerous flare-like transient loop brightenings. The authors use a magnetic reconnection theory driven by a ponderomotive force with transverse plasmons on account of the basic properties of a transient brightening: lifetime a few minutes and total energy 1025 - 1029ergs. The numerical results are consistent with the observations.

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