Revision history of "File:204f2.png"

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  • (cur | prev) 15:41, 29 July 2013 Hhudson (Talk | contribs) (292 bytes) (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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