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Non-Maxwellian Velocity Distribution Functions Associated with Steep Temperature Gradients in the Solar Transition Region. Paper 1: Estimate of the Electron Velocity Distribution Functions

机译:太阳过渡区陡温梯度与非麦克斯韦速度分布函数关系。论文1:电子速度分布函数的估计

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摘要

It was shown that, in the presence of the steep temperature gradients characteristic of EUV models of the solar transition region, the electron and proton velocity distribution functions are non-Maxwellian and are characterized by high energy tails. The magnitude of these tails are estimated for a model of the transition region and the heat flux is calculated at a maximum of 30 percent greater than predicted by collision-dominated theory.

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