AN EXPLANATION ON TRANSIENT BRIGHTENING BY MAGNETIC RECONNECTION THEORY

  • LI BI-QIANG (Purple Mountain Observatory, Academia Sinica) ;
  • LI XIAO-QING (Purple Mountain Observatory, Academia Sinica) ;
  • AI GUO-XIANG (Beijing Astronomical Observatory, Academia Sinica)
  • Published : 1996.12.01

Abstract

It. has been discovered that. active regions commonly have numerous flare-like transient. loop brightenings. We use a magnetic reconnection theory driven by a ponderamotive force on account. of the basic properties of a transient. brightening: lifetime a few mins, total energy $10^{25}\~10^{29}$ erg. The numerical results are consistent with the observations.

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