Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 672, Issue 2, Pages L135-L138Publisher
IOP PUBLISHING LTD
DOI: 10.1086/527297
Keywords
Sun : corona; Sun : UV radiation
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All theoretical models of nanoflare heating in the solar corona predict loops with an unresolved multistrand structure, which is in discrepancy with the quasi-isothermal cross sections of the finest coronal loop structures observed with TRACE, which have spatially resolved widths of km. We suggest modifying the w approximate to 1000 - 2000 theoretical models by relocating the hypothetical nanoflare events from their coronal location down to the chromosphere/ transition region.
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