A Solar Flare Model Based on Magnetic Reconnection between Current-carrying Loops

Melrose, D. B., A Solar Flare Model Based on Magnetic Reconnection between Current-carrying Loops, ApJ, 486, 521-533 (1997) (ADS)

The cartoon

(click on the image for a larger version)

A surprising twist on loop-loop interactions; it might not be obvious that the four footpoints in this model could re-link while not changing any of their respective fields and currents at the photosphere. Nevertheless the cited paper shows this and obtains an interesting "selection rule" for loop-loop current reconnection. That's the twist.

      The loop - loop geometry is often observed in solar flares, as probably shown originally by the Yohkoh/SXT observations.

Date: 1999 January 01

Update: 2019 February 17