Fuzzy hot post-flare loops versus sharp cool post-flare loops

Details Fuzzy hot post-flare loops versus sharp cool post-flare loops Fuzzy hot post-flare loops versus sharp cool post-flare loops

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.505..207p&link_type=abstract

In: SOLMAG 2002. Proceedings of the Magnetic Coupling of the Solar Atmosphere Euroconference and IAU Colloquium 188, 11 - 15 Jun

Physics

7

Post-Flare Loops

Scientific paper

By using high spatial resolution TRACE EUV observations we show that hot (≍2 MK) post-flare loops are fuzzier than the cooler (≍1 MK) ones. A simple 0d model of a cooling loop arcade, where different loops in the arcade start to cool down at slightly different initial conditions, is sufficient to reproduce qualitatively the observed behavior of the EUV post-flare loops.

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