Weekly Report 8Apr2011
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===RHESSI Albedo Imaging Test=== | ===RHESSI Albedo Imaging Test=== | ||
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+ | 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: | ||
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+ | *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 | ||
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+ | For each energy range (12keV-25keV and 25keV-50keV) an image was made for each detector combination. | ||
Revision as of 21:50, 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.