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HMI intensity observations at three times during the flare SOL2013-05-13T16. These are difference images relative to a preflare frame, and the left portion of each has been multiplied by a factor 80 to enhance the visibility of the features in the corona. The red boxes mark particular features, specifically (on the right) the white-light flare sites.

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current14:35, 1 November 2024Thumbnail for version as of 14:35, 1 November 2024858 × 443 (114 KB)Maintenance script (talk | contribs)== Summary == Importing file

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