File:161fig2.png

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Upper panel: Summed and background subtracted light curve of the solar flare observed by RHESSI on January 1st, 2005. The inset shows the residual emission after subtracting a simple (boxcar) moving average. Middle panel: Periodogram analysis performed on the residual emission. Lower panel: PSD with best fit broken power-law (solid green line) and the Failed to parse (PNG conversion failed; check for correct installation of latex, dvips, gs, and convert): 3\sigma

significance level (dotted line) indicated. The arrow points to the significant frequency at Failed to parse (PNG conversion failed;

check for correct installation of latex, dvips, gs, and convert): f \approx 0.244

Hz.

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Date/TimeThumbnailDimensionsUserComment
current07:46, 16 October 2011Thumbnail for version as of 07:46, 16 October 2011618×1,227 (138 KB)Hhudson (Talk | contribs) (''Upper panel:'' Summed and background subtracted light curve of the solar flare observed by RHESSI on January 1st, 2005. The inset shows the residual emission after subtracting a simple (boxcar) moving average. ''Middle panel:'' Periodogram analysis perf)

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