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(RHESSI views of the occulted flare SOL2010-11-03, estimated to have been at longitude W102 about. Left: 6-12 keV at flare peak; right, 25-50 keV. The soft X-ray source hugs the limb, as would be expected for a partially eclipsed source; the hard X-ray so)
 
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Latest revision as of 14:33, 1 November 2024

RHESSI views of the occulted flare SOL2010-11-03, estimated to have been at longitude W102 about. Left: 6-12 keV at flare peak; right, 25-50 keV. The soft X-ray source hugs the limb, as would be expected for a partially eclipsed source; the hard X-ray source extends into the corona.

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