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 | 14:34, 1 November 2024 | | 850 × 850 (80 KB) | Maintenance script (talk | contribs) | == Summary == Importing file |
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