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 <math>3\sigma</math> significance level (dotted line) indicated. The arrow points to the significant frequency at <math>f \approx 0.244</math> Hz.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
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| current | 14:33, 1 November 2024 | | 618 × 1,227 (138 KB) | Maintenance script (talk | contribs) | == Summary == Importing file |
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