File:145F1.png

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Left, the four passbands of the EUV/ESP instrument; right, their responses during the flare. Note the varying degrees of impulsive (early) and gradual (late) as the many different spectral lines contribute their counts to these broad-band photometric channels.

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current21:41, 8 February 2011Thumbnail for version as of 21:41, 8 February 20111,011×375 (20 KB)Hhudson (Talk | contribs) (Left, the four passbands of the EUV/ESP instrument; right, their responses during the flare. Note the varying degrees of impulsive (early) and gradual (late) as the many different spectral lines contribute their counts to these broad-band photometric chan)
21:21, 6 February 2011Thumbnail for version as of 21:21, 6 February 20111,001×391 (21 KB)Hhudson (Talk | contribs) (Left, the four passbands of the EUV/ESP instrument; right, their responses during the flare. Note the varying degrees of impulsive (early) and gradual (late) as the many different spectral lines contribute their counts to these broad-band photometric chan)

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