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An M Dwarf’s Chromosphere, Corona, and Wind Connection via Nonlinear Alfvén Waves

  • Authors: Takahito Sakaue and Kazunari Shibata

2021 The Astrophysical Journal 919 29.

  • Provider: AAS Journals

Caption: Figure 11.

Coronal temperature (Tco) as a function of transmitted Alfvén wave energy flux into the corona (FA,co). The dotted lines represent ﹩y={\left[7{xl}/(2{\kappa }_{0})\right]}^{2/7}﹩, with l = (10−1, 10−2, 10−3)r.

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