Fine Structures of Flaring Loops Seen in Fe XxIII 263.76 Å Line

Details Fine Structures of Flaring Loops Seen in Fe XxIII 263.76 Å Line Fine Structures of Flaring Loops Seen in Fe XxIII 263.76 Å Line

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397..139w&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

Astronomy and Astrophysics

Astronomy

Scientific paper

EIS observed the highest temperature lines of Fe XXIII 263.76 Å and FeXXIV 192.10 Å, 255.10 Å in the EIS observing wavelengths for the first time during a C4.2 flare which occurred on 16-Jan-07. The raster scan of the flaring area took place during 2:36 - 2:41 UT, nearly at the maximum phase of the flare. Footpoints of fast chromospheric evaporation are compact with a size of a few arcseconds, and turbulence still remains around the top of flaring loops. Down flows of cooling origin are also seen in lower temperature lines, just outside the flaring loops.

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