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Nonlinear Alfvén Wave Model of Stellar Coronae and Winds from the Sun to M Dwarfs

  • Authors: Takahito Sakaue, and Kazunari Shibata

2021 The Astrophysical Journal Letters 906 L13.

  • Provider: AAS Journals

Caption: Figure 1.

Schematic image of axisymmetric magnetic flux tube, the surface of which is defined by the poloidal x and toroidal ϕ axes. The winding thin lines represent the magnetic field lines, which illustrate the nonlinear propagation of the Alfvén wave.

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