Cross-calibration Of EIS And XRT Using Coronal Bright Points

Details Cross-calibration Of EIS And XRT Using Coronal Bright Points Cross-calibration Of EIS And XRT Using Coronal Bright Points

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21822421k&link_type=abstract

American Astronomical Society, AAS Meeting #218, #224.21; Bulletin of the American Astronomical Society, Vol. 43, 2011

Other

Scientific paper

The Extreme Ultraviolet Imaging Spectrometer and the X-Ray Telescope aboard Hinode are designed to complement one another. This study uses X-Ray Bright Points, simple emission features in the Solar Corona, as sources of emission data for the purpose of obtaining a cross-calibration factor for the two instruments. After calibrating and co-aligning the data from each instrument individually, pixels are selected within several coronal Bright Points. By analyzing this equivalent data from both instruments, separate Differential Emission Measures and Emission Measure Loci Plots are produced. These results are then used to produce the desired instrument cross calibrations. The use of Bright Points eliminates the need for prolonged and uncertain background subtraction. Due to the simple thermal characteristics of the Bright Points, this method could be used to calibrate other instruments as well.

Affiliated with

Also associated with

No associations

Rating

Cross-calibration Of EIS And XRT Using Coronal Bright Points does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cross-calibration Of EIS And XRT Using Coronal Bright Points, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cross-calibration Of EIS And XRT Using Coronal Bright Points will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1740385