File:204f0.png: Difference between revisions
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imported>Hhudson (Left - an EUV image of the flare, essentially from above, showing the photospheric magnetic field as colored contours (two polarities), plus the line of a slit used to make plots of position vs. time. These are in the middle and right plots on different t) |
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Latest revision as of 14:34, 1 November 2024
Left - an EUV image of the flare, essentially from above, showing the photospheric magnetic field as colored contours (two polarities), plus the line of a slit used to make plots of position vs. time. These are in the middle and right plots on different time scales. The CME-related dimming is very obvious, as are the contracting and oscillating loops. The diagonal line shows a rough guess at the propagation sequence of excitation of the oscillations. Note the different periods for the different loops.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 14:34, 1 November 2024 |  | 679 × 210 (212 KB) | Maintenance script (talk | contribs) | == Summary == Importing file |
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