File:204f0.png
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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 | 15:09, 29 July 2013 | | 679×210 (212 KB) | Hhudson (Talk | contribs) | (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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