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Latest revision as of 14:35, 1 November 2024

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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current14:35, 1 November 2024Thumbnail for version as of 14:35, 1 November 20241,200 × 347 (176 KB)Maintenance script (talk | contribs)== Summary == Importing file

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