Figure 15 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 15.

Plasma β at the distance where the amplitude of the Alfvén waves reaches the maximum (﹩{\beta }_{\phi \max }﹩) as a function of T_co/v_wind. The solid line corresponds to Equation (72).

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