File:204f2.png

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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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current14:35, 1 November 2024Thumbnail for version as of 14:35, 1 November 2024609 × 641 (80 KB)Maintenance script (talk | contribs)== Summary == Importing file

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