Figure 12 from An M Dwarf’s Chromosphere, Corona, and Wind Connection via Nonlinear Alfvén Waves

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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 12.

Plasma pressure at the transition region (﹩{p}_{\mathrm{tr}}﹩) as a function of coronal temperature (T_co). The dotted lines represent ﹩y={\left(x/1.4\times {10}^{3}\right)}^{3}/l﹩, with l = (1, 10⁻¹, 10⁻²)r_⊙.

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