File:15 fe eqwidth.gif

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How the equivalent width of the Fe feature compares with theory for many points during a particular solar flare. Basically the flare evolution moves the points up in temperature rapidly, then more slowly downwards. At this level, the discrepancy is probably not significant yet.

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current14:33, 1 November 2024Thumbnail for version as of 14:33, 1 November 2024800 × 677 (48 KB)Maintenance script (talk | contribs)== Summary == Importing file

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