File:139Fig2.png
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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)
(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)
Latest revision as of 17:24, 8 November 2010
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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current | 17:24, 8 November 2010 | ![]() | 1,224×628 (51 KB) | Hhudson (Talk | contribs) | (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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