Methods of Analyzing Temperatures in Post-Flare Loops using the XRT on Hinode

Details Methods of Analyzing Temperatures in Post-Flare Loops using the XRT on Hinode Methods of Analyzing Temperatures in Post-Flare Loops using the XRT on Hinode

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh51c..08r&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH51C-08

Physics

7509 Corona, 7519 Flares, 7554 X-Rays, Gamma Rays, And Neutrinos

Scientific paper

The X-Ray Telescope on Hinode has unrivaled temperature coverage, with 9 X-Ray filters in the focal plane. Using 7 different filter combinations, XRT observed a C8.2 flare on July 10, 2007. We use two different methods to glean temperature information about the post-flare loop system in this event. First, we examine the flare loops using the combined filter ratio method, which is a ratio method that utilizes observations in multiple filters in order to optimize the signal quality. Secondly, we calculate temperatures based on a differential emission measure method, which is a forward fitting method of determining temperatures. The results of these two methods will be compared.

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