On reconnection as an energy release mechanism in the solar atmosphere

Details On reconnection as an energy release mechanism in the solar atmosphere On reconnection as an energy release mechanism in the solar atmosphere

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..491s&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Sun: Magnetic Fields, Reconnection

Scientific paper

Basic principles and the fundamental ideas, which are under current use to model the magnetic reconnection process in the corona and photosphere, are briefly reviewed and demonstrated. The so-called 'rainbow reconnection' model is applied to solar observations with the HXT on board Yohkoh, the MDI instrument on the SOHO, TRACE, and Solar Magnetic Field Telescope of the Beijing Astronomical Observatory. In particular, an interpretation of the physical mechanism is given for the well-observed Bastille-day 2000 flare.

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