DEM Temperature Analysis of Post-Flare Loops Using Hinode's X-Ray Telescope

Details DEM Temperature Analysis of Post-Flare Loops Using Hinode's X-Ray Telescope DEM Temperature Analysis of Post-Flare Loops Using Hinode's X-Ray Telescope

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..415..443r&link_type=abstract

The Second Hinode Science Meeting: Beyond Discovery-Toward Understanding ASP Conference Series, Vol. 415, proceedings of a meeti

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We investigate the temperature structure of the post-flare loops from two small flares by utilizing a differential emission measure (DEM) method that takes advantage of the many X-ray filters available on the X-Ray Telescope (XRT) on Hinode. This method allows us to observe multi-thermal plasma along the line of sight. Using this method, we see clear evidence of multiple temperatures in the post-flare loops systems. We also find that intensity changes in the XRT images are due to cooling plasma in one of the flares, and decreasing emission measure in the other flare.

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