File:145F2.png
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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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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:56, 7 February 2011 | | 1,742×716 (22 KB) | Hhudson (Talk | contribs) | (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 the EVE background EUV spectrum; the red diamonds the EVE/ES) |
| 21:23, 6 February 2011 |  | 1,742×716 (22 KB) | Hhudson (Talk | contribs) | (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 t) |
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