File:Sample eve chianti flare spec.png

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A sample of the EUV spectra from 6.5-105 nm taken with both the MEGS-A and MEGS-B components of EVE near the peak of the X2.2 flare that occurred on 15 February 2011. The locations of the recombination edges at 22.8, 50.4, and 91.2 nm are noted. Synthetic continuum emission from CHIANTI generated using arbitrary temperatures and scaling factors are overlaid in color.

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Date/TimeThumbnailDimensionsUserComment
current13:28, 13 January 2012Thumbnail for version as of 13:28, 13 January 20121,000×600 (15 KB)Rmilligan (Talk | contribs) (A sample of the EUV spectra from 6.5-105 nm taken with both the MEGS-A and MEGS-B components of EVE near the peak of the X2.2 flare that occurred on 15 February 2011. The locations of the recombination edges at 22.8, 50.4, and 91.2 nm are noted. Synthetic)

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