File:145F2.png

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Revision as of 21:56, 7 February 2011 by imported>Hhudson (uploaded a new version of "File:145F2.png": Left, the faint line shows RHESSI hard X-rays (100-200 keV), a good proxy for the flare gamma-ray emission; right, the spectrum of the impulsive phase selected on this basis. The blue points are th)
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Left, RHESSI 100-200 keV emission (thin line) compared with He II 30.4 nm radiation; right, a broad-band spectrum of just the impulsive phase. The smooth line roughly describes the white-light flare continuum, the points the EUV background from EVE, and the diamonds, the EVE broad-band points.

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current14:34, 1 November 2024Thumbnail for version as of 14:34, 1 November 20241,742 × 716 (22 KB)Maintenance script (talk | contribs)== Summary == Importing file

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