Collective plasma effects associated with the continuous injection model of solar flare particle streams
Collective plasma effects associated with the continuous injection model of solar flare particle streams
复制标题
与太阳耀斑粒子流连续注入模型相关的集体等离子体效应
DOI：
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发表时间：
1979
期刊：
影响因子：
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通讯作者：
K. Papadopoulos
中科院分区：
文献类型：
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作者：
L. Vlahos;K. Papadopoulos
基于边缘稳定性的概念，提出了一个包含自洽等离子体非线性的脉冲太阳耀斑连续注入模型。一个准定态的建立，由一个热截断电子麦克斯韦分布局限于顶部的环路上的声学湍流和高能电子束沉淀在色球层。结果表明，模式的辐射特性与观测结果是一致的。
A modified continous injection model for impulsive solar flares that includes self-consistently plasma nonlinearities based on the concept of marginal stability is presented. A quasi-stationary state is established, composed of a hot truncated electron Maxwellian distribution confined by acoustic turbulence on the top of the loop and energetic electron beams precipitating in the chromosphere. It is shown that the radiation properties of the models are in accordance with observations.