File:162f2.png
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Left: RHESSI light curves in three energy bands for the flare SOL2005-09-06. Middle: a GOES/SXI image during the rise phase; the contours show RHESSI emission at 8-9 keV with 10% contour levels. Right: RHESSI spectrum of the loop-top source at 20:37 UT. Horizontal bars correspond to the energy bin widths. The fit consists of a thermal component and two spectral line complexes (at 6.7 keV and 8.0 keV).
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 18:04, 26 October 2011 | | 1,200×347 (176 KB) | TomekMrozek (Talk | contribs) | |
| 16:38, 25 October 2011 |  | 690×225 (83 KB) | Hhudson (Talk | contribs) | (Left: RHESSI light curves in three energy bands for the flare SOL2005-09-06. Middle: a [http://en.wikipedia.org/wiki/Solar_X-ray_Imager GOES/SXI] image during the rise phase; the contours show RHESSI emission at 8-9 keV with 10% contour levels. Right: RHE) |
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