HR: 0800h
AN: SH22A-0841    [Abstracts]
TI: The Differential Emission Measure and Analysis of X-Ray Bright Points using Hinode's X-Ray Telescope (XRT)
AU: * Farid, S I
EM: sfarid@cfa.harvard.edu
AF: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Ma 02138, United States
AU: Saar, S
EM: ssaar@cfa.harvard.edu
AF: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Ma 02138, United States
AU: DeLuca, E
EM: edeluca@cfa.harvard.edu
AF: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Ma 02138, United States
AU: Golub, L
EM: golub@cfa.harvard.edu
AF: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Ma 02138, United States
AU: Weber, M
EM: mweber@cfa.harvard.edu
AF: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Ma 02138, United States
AB: 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.
DE: 7509 Corona
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2007 Fall Meeting