Microflaring at the Feet of Large Active Region Loops

Computer Science

Scientific paper

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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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