A Long-duration Flare Observed With Hinode EIS

Details A Long-duration Flare Observed With Hinode EIS A Long-duration Flare Observed With Hinode EIS

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.6802h&link_type=abstract

American Astronomical Society Meeting 210, #68.02; Bulletin of the American Astronomical Society, Vol. 39, p.175

Astronomy and Astrophysics

Astronomy

Scientific paper

Long-duration solar flares generally have a cusp apex at the loop top. The cusp shape reflects the topology of magnetic fields near the flare-loop top and it is one of the indirect pieces of evidence supporting the occurrence of the magnetic reconnection process above flare loops. The Hinode EUV Imaging Spectrometer (EIS) observed a long-duration flare that occurred on 2006 Dec 17. We present the first EIS spectroscopic observation of cusp-shaped flare loops. We also report velocity fields around the cusp structures and post-flare loops.

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