Microflaring at the feet of large active region loops

Details Microflaring at the feet of large active region loops Microflaring at the feet of large active region loops

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993stin...9670891p&link_type=abstract

Conference Paper, NASA Marshall Space Flight Center Huntsville, AL United States

Computer Science

Solar Flares, Coronal Loops, Magnetic Signatures, X Ray Imagery, Magnetic Variations, Energy Transfer, X Ray Telescopes, Solar Magnetic Field, Plasma Heating

Scientific paper

By superposing Yohkoh SXT images on an MSFC magnetogram of an active region, we find that the brightest loops in the bipolar magnetic envelope spanning the active region are rooted near a compact site of mixed polarity and microflaring. Apparently, the enhanced coronal heating in these high loops is a consequence of the microflaring and/or related magnetic activity at this end site.

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