File:145F2.png: Difference between revisions
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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) |
(Maintenance script uploaded File:145F2.png) Tag: Server-side upload |
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Latest revision as of 14:34, 1 November 2024
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 | 14:34, 1 November 2024 |  | 1,742 × 716 (22 KB) | Maintenance script (talk | contribs) | == Summary == Importing file |
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