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imported>Hhudson (RHESSI images from the flare using two inversion techniques: CLEAN at the top, and MEM at the bottom. From left to right, increasing energies (6-12, 25-50, and 50-100 keV). the simple structure seen in soft X-rays becomes more complicated with time, reve) |
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Latest revision as of 14:35, 1 November 2024
RHESSI images from the flare using two inversion techniques: CLEAN at the top, and MEM at the bottom. From left to right, increasing energies (6-12, 25-50, and 50-100 keV). the simple structure seen in soft X-rays becomes more complicated with time, revealing a Masuda-type "above the loop top" source at high energies. Note that this appearance is in the early phase of the flare, as it was for Masuda's original event SOL1992-01-13 ([http://sprg.ssl.berkeley.edu/~tohban/browser/?show=qlpcr+qli02+qli03+qli04+qli05+ grwa&date=20020220&time=095921&bar=1 Browser).
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| current | 14:35, 1 November 2024 |  | 1,223 × 1,246 (57 KB) | Maintenance script (talk | contribs) | == Summary == Importing file |
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