Unusual large-scale flaring structure

Details Unusual large-scale flaring structure Unusual large-scale flaring structure

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..569c&link_type=abstract

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

Physics

Solar Bright Point, Soft X-Ray Jet, Magnetic Reconnection

Scientific paper

The Yohkoh/SXT data of August 21, 1999 displayed a spectacular transient brightening of a large-scale double whip-like structure extending through the corona to a length greater than 950 Mm. The transient originated at a relatively small middle-latitude soft X-ray bright point (XBP), which was also visible in the EUV range and had a small underlying Hα plage with a bipolar magnetic configuration. The structure developed in the high-temperature (>2.5 MK) soft X-ray emission to both sides of the XBP during a few tens of minutes and could be recognized for about two hours. The observations suggest sudden energy release during the interaction of the magnetic structures of the XBP and the filament channel.

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