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- W1630454002 abstract "Abstract We analyze data from 141 solar flares that were observed with the Yohkoh soft and hard X-ray telescopes to investigate the general characteristics of the soft X-ray high-temperature region above soft X-ray flare loops. We performed a careful analyses in order to obtain accurate temperature maps of the high-temperature regions, and found high-temperature regions of 15–35 million degrees above soft X-ray flare loops for 64 flares out of the 141 events. The region appears at the hard X-ray impulsive phase and its temperature reaches a maximum before the time of the soft X-ray peak. The volume emission measure of the region is 10 47–48 cm 3 on the average, which is about ten times smaller than that of the 10 million degree flare loop below it. The high-temperature regions tend to move outwards at a speed of 10–20 km s −1 , which is faster than the rising speed of the flare loops of 5–10 km s −1 ." @default.
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- W1630454002 date "2002-01-01" @default.
- W1630454002 modified "2023-09-22" @default.
- W1630454002 title "Soft X-ray high-temperature regions above solar flare loops" @default.
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- W1630454002 doi "https://doi.org/10.1016/s0964-2749(02)80096-8" @default.
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