File:142f02.png

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Six panels comparing RHESSI and Hinode imaging of the Dec. 6 2006 flare. The top row shows (a, b, c) Hinode in color, in contours, and a UV image; the bottom row shows RHESSI integrated for 4, 8, and 16 seconds. The longer integrations have more photon counts and are cleaner.

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current19:44, 19 December 2010Thumbnail for version as of 19:44, 19 December 2010911×624 (578 KB)Hhudson (Talk | contribs) (Six panels comparing RHESSI and Hinode imaging of the Dec. 6 2006 flare. The top row shows (a, b, c) Hinode in color, in contours, and a UV image; the bottom row shows RHESSI integrated for 4, 8, and 16 seconds. The longer integrations have more photon co)

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