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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 9.

Wind velocity (vwind) as a function of the maximum amplitude of the Alfvén waves in the stellar wind (﹩{v}_{\phi \max }﹩). The solid line represents the power-law fitting.

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