File:151f2.png
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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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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 14:16, 10 May 2011 | | 850×850 (80 KB) | Hhudson (Talk | contribs) | (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). This is in the sequence expected for longer and longer w) |
| 09:47, 9 May 2011 |  | 1,573×787 (24 KB) | Hhudson (Talk | contribs) | (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 ) |
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