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 Letters906L13.
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.