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- W1995135052 abstract "An occulted solar flare occurred at about 06:07 UT on 2002, November 2. The RHESSI X-ray images show two separate parts. The lower part consists of a complete loop and the upper part a coronal source which well extends above the solar limb. The loop source shrank for about 3 min with a speed of ∼24 km s −1 during the early impulsive phase and then expanded at ∼7 km s −1 , while the coronal source presented an upward motion at about 6 km s −1 . We obtained the temperature map of the loop source from RHESSI image spectrum. The temperature of the loop increases with altitude, indicating that the reconnection X-point of this flare is located above the loop source. However, the apparent coronal source is the top of another independent large-scale loop." @default.
- W1995135052 created "2016-06-24" @default.
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- W1995135052 date "2007-01-01" @default.
- W1995135052 modified "2023-09-24" @default.
- W1995135052 title "The temperature map of the loop and coronal sources of an occulted solar flare" @default.
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- W1995135052 doi "https://doi.org/10.1016/j.asr.2007.04.009" @default.
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