File:116 fig3.jpg
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The energy distribution derived from the TRACE images for the impulsive phase of the flare. This is very crude. It represents the photosphere as a blackbody (the solid line), and the flare as a slightly hotter but optically-thin source. This works for 1600A (the left asterisk) but not the EUV point at 171A (the right asterisk). Most of the flare energy is in the low-temperature continuum.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 02:48, 7 December 2009 | | 1,008×720 (82 KB) | Hhudson (Talk | contribs) | (The energy distribution derived from the TRACE images for the impulsive phase of the flare. This is very crude. It represents the photosphere as a blackbody (the solid line), and the flare as a slightly hotter but optically-thin source. This works for 160) |
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