Weekly Report 8Apr2011

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Revision as of 22:10, 11 April 2011 by imported>Agopie
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RHESSI Albedo Imaging Test

RHESSI Clean Imaging techniques were used to image large groups of flares using different detector combinations and energy ranges. The following were used to create the Clean images:

  • Time: Decided by the peak of a flare in the 25keV - 50keV range
  • Energy: 12kev - 25keV, or 25keV - 50KeV
  • Detectors: 3 to 9, or 3 to 6, or 6 to 9
  • Clean Beam Width Factor = 2

For each energy range (12keV-25keV and 25keV-50keV) an image was made for each detector combination. Using the images the flux was measured for detector combinations. The


DiffvsDistance 2003 15 25 detcom1 detcom0.jpg


DiffvsDistance 2003 15 25 detcom2 detcom0.jpg


Diff dist 25to50 dcob1 minus dcomb0.jpg


Dif dist 25to50 dcomb2 minus dcomb0.jpg


DiffvsDistance 2003 15 25 50 ratio.jpg