Weekly Report 8Apr2011: Difference between revisions
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*Clean Beam Width Factor = 2 | *Clean Beam Width Factor = 2 | ||
For each energy range (12keV-25keV and 25keV-50keV) an image was made for each detector combination. | 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 | ||
Revision as of 22:10, 11 April 2011
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
