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- W2000503573 abstract "Despite some measure of theoretical and predictive success of the electron-heated model of solar flares, observations of low levels of soft X-ray emission prior to the detection of hard X-rays in most flares present a problem for the paradigm, since it suggests some sort of preheating of the chromospheric plasma before electron acceleration. Particularly troublesome are assertions that plasma flows have been observed prior to hard X-ray emission, because they imply significant and rapid energy input by some agent without leaving a (currently) detectable hard X-ray signature. Given this challenge to a prevailing paradigm, it is imperative to investigate more comprehensively the existence of precursor flows manifested in the asymmetry of X-ray spectral lines." @default.
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- W2000503573 date "1997-07-20" @default.
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- W2000503573 title "Investigating “Precursor Flows” in Solar Flares" @default.
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- W2000503573 doi "https://doi.org/10.1086/304312" @default.
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