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A new way for turbulence to heat the corona
Nature Astronomy ( IF 12.9 ) Pub Date : 2022-06-20 , DOI: 10.1038/s41550-022-01716-w
Christopher H. K. Chen

Recent advances in plasma turbulence theory have led to a new way of explaining the heating of the solar corona and many of the observed features of the solar wind.

中文翻译:

湍流加热日冕的新方法

等离子体湍流理论的最新进展导致了一种解释太阳日冕加热和许多观测到的太阳风特征的新方法。
更新日期:2022-06-21
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