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Timing of the contraction of coronal loops and flare emission (top), and the rate of change dh/dt (middle), compared to the impulsive phase observed in hard X-rays by RHESSI, and at 9.4 GHz in the radio microwave spectrum by the Nobeyama Solar Radio Observatory.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 15:41, 29 July 2013 | | 609×641 (80 KB) | Hhudson (Talk | contribs) | (Timing of the contraction of coronal loops and flare emission (top), and the rate of change dh/dt (middle), compared to the impulsive phase observed in hard X-rays by RHESSI, and at 9.4 GHz in the radio microwave spectrum by the [http://solar.nro.nao.ac.j) |
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