File:151f0.png
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Three of the four ESP irradiance passbands, plus the zeroth-order (soft X-ray channel, lower right) for the SOL2011-02-24 limb event. A similar plot for a disk event (SOL2010-06-12, another white-light flare) is in a [previous Nugget]. The broad-band ESP channels have different profiles because they integrate different sets of emission lines, basically. Note that this event is not typical because of it proximity to the limb (and because it is a gamma-ray flare).
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 09:42, 9 May 2011 | | 1,400×1,000 (15 KB) | Hhudson (Talk | contribs) | (Three of the four ESP irradiance passbands, plus the zeroth-order (soft X-ray channel, lower right) for the SOL2011-02-24 limb event. A similar plot for a disk event (SOL2010-06-12, another white-light flare) is in a [previous Nugget]. The broad-band ESP ) |
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