Fine Structures of Flaring Loops Seen in Fe XxIII 263.76 Å Line
Abstract
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.
- Publication:
-
First Results From Hinode
- Pub Date:
- September 2008
- Bibcode:
- 2008ASPC..397..139W