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Combined display of all available logs of RHESSI Wiki. You can narrow down the view by selecting a log type, the user name (case-sensitive), or the affected page (also case-sensitive).- 15:41, 29 July 2013 Hhudson (Talk | contribs) uploaded "File:204f2.png" (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)