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9th RHESSI Workshop |
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Genova, Italy, September 1-5 2009 |
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Participants |
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Pascal Saint-Hilaire Space Sciences Laboratory, University of California, Berkeley, US Email: shilaire (at) ssl.berkeley.edu Group 4 Contribution: Using several hundred HXR-intense RHESSI flares, we have statistically derived HXR sources heights using a method similar to that used in Matsushita et al. (1992). From these, we have derived chromospheric densities, and attempted to fit different density models. Group 1 Contribution: Imaging Spectroscopy errors: In an attempt to better quantify the errors on feature flux measurements, I have added noise to the calibrated event list, before the usual imaging algorithms quick in.
__________________________________________________________________ Website created by Marco Prato Comments and suggestions to marco.prato (at) unimore.it |
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