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On the Evolution of the Lower Energy Cutoff of Nonthermal Electrons in Solar Flares

On the Evolution of the Lower Energy Cutoff of Nonthermal Electrons in Solar Flares
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摘要 Using the method recently developed by Can et al. (2001a, 2002), We investigate the time variation of the lower energy cutoff (Ec) of nonthermal electrons for three BATSE/CGRO hard X-ray events. The result shows that Ec changes with time, from smaller before the peak flux, to larger at the peak, and then back to smaller after the peak. Such a variation of Ec, being a preliminary conclusion for the first time, should be checked in the future by using data with a higher energy resolution. Using the method recently developed by Can et al. (2001a, 2002), We investigate the time variation of the lower energy cutoff (Ec) of nonthermal electrons for three BATSE/CGRO hard X-ray events. The result shows that Ec changes with time, from smaller before the peak flux, to larger at the peak, and then back to smaller after the peak. Such a variation of Ec, being a preliminary conclusion for the first time, should be checked in the future by using data with a higher energy resolution.
出处 《Chinese Journal of Astronomy and Astrophysics》 CSCD 北大核心 2002年第2期103-105,共3页 中国天文和天体物理学报(英文版)
关键词 Sun: hard X-rays─Sun: gamma-rays─Sun: flares─Sun: PARTICLES Sun: hard X-rays─Sun: gamma-rays─Sun: flares─Sun: particles
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参考文献6

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