The Differential Emission Measure and Analysis of X-Ray Bright Points using Hinode's X-Ray Telescope (XRT)

Details The Differential Emission Measure and Analysis of X-Ray Bright Points using Hinode's X-Ray Telescope (XRT) The Differential Emission Measure and Analysis of X-Ray Bright Points using Hinode's X-Ray Telescope (XRT)

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh22a0841f&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH22A-0841

Physics

7509 Corona

Scientific paper

The X-Ray telescope aboard Hinode utilizes up to thirteen filter combinations with one arc second resolution to provide unprecedented temperature coverage. In this study, we have used eleven X-Ray filters to examine the statistical properties of X-ray bright points including temperature, emission, and size distributions. We have analyzed what appears to be a population of XRBs that are hotter than the main group in order to identify any distinguishing properties.We discuss the results of our analysis and their implications on XBP classification.

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