Numerical Simulations of Impulsively Heated Solar Flares

J. Mariska, A. Emslie, P. Li
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引用次数: 134

Abstract

The response of a model solar atmosphere to heating by an electron beam has been studied for electron beam flux spectra which are power laws with low-energy knees (rising linearly with time to a peak at 30 s and then falling linearly to 0 at 60 s) ranging from 10 to 20 keV. The results indicate that high peak electron beam fluxes, low-energy knees, and larger spectral indices all move the atmospheric response toward greater enhancements of the parameters in the coronal regions of the atmosphere. Coronal responses can thus be used as a diagnostic of the parameters of the electron beam. 23 refs.
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脉冲加热太阳耀斑的数值模拟
本文研究了模型太阳大气对电子束加热的响应,电子束通量谱在10 ~ 20 keV范围内具有低能膝(随时间线性上升,在30 s时达到峰值,在60 s时线性下降至0)的幂律。结果表明,较高的峰值电子束通量、低能屈膝和较大的光谱指数都使大气响应朝着日冕区域参数的更大增强方向发展。因此,日冕响应可以用来诊断电子束的参数。参23。
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