File:Eve hsi goes plot.png: Difference between revisions
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imported>Rmilligan (Top panel: lightcurves of free-free, free-bound, and bound-bound emission as observed by EVE during the 15 February 2011 flare. The vertical dashed lines in each panel denote the time of peak emission in each band. Also shown is the GOES 0.1-0.8 nm lightc) |
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Latest revision as of 14:34, 1 November 2024
Top panel: lightcurves of free-free, free-bound, and bound-bound emission as observed by EVE during the 15 February 2011 flare. The vertical dashed lines in each panel denote the time of peak emission in each band. Also shown is the GOES 0.1-0.8 nm lightcurve (solid black line). The inset shows the cumulative energy radiated throughout the course of the flare by each process. Bottom panel: RHESSI 6-100 keV lightcurves of the same event. The vertical solid black line in each panel marks the approximate onset time of the continuum emission.
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