File:151f2.png: Difference between revisions

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imported>Hhudson
(Left: Comparison of the [ESP] zeroth-order signal ("QD"), in red, and the GOES low-energy channel (blue). Two features are striking: first, the EVE signal peaks later, and second, it has a substantial preflare excess. These both point to longer effective )
 
imported>Hhudson
(uploaded a new version of "File:151f2.png": Comparison of ESP soft X-ray band with the two standard GOES channels, each normalized to its maximum. The earliest to peak is GOES 0.5-4A (yellow), followed by GOES 1-8A (blue), and then ESP (red))
(No difference)

Revision as of 14:16, 10 May 2011

Left: Comparison of the [ESP] zeroth-order signal ("QD"), in red, and the GOES low-energy channel (blue). Two features are striking: first, the EVE signal peaks later, and second, it has a substantial preflare excess. These both point to longer effective wavelengths. Right: A blow-up of the preflare variation, showing how much better the ESP photometry (1/4 sec binning, much lower noise) than GOES is (3 sec binning, much greater noise).

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