File:Sample eve chianti flare spec.png: Difference between revisions
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imported>Rmilligan (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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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 | 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. | ||
noted. Synthetic continuum emission from CHIANTI generated using arbitrary temperatures and scaling factors are overlaid in color. | |||
Latest revision as of 14:34, 1 November 2024
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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