File:216f1.png
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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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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 20:54, 19 December 2013 | 858×443 (114 KB) | Hhudson (Talk | contribs) | (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.) |
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