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Spherically Polarized Alfvén Waves and the Gosling Boost

  • Authors: Yuliang Ding, Marco Velli, Zesen Huang, Chen Shi, Lorenzo Matteini, Nikos Sioulas, Stuart D. Bale, Anna Tenerani, Mingzhe Liu

Yuliang Ding et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 1.

Magnetic and velocity perturbations for spherically polarized Alfvén waves, under different deflection angles θ. The magnetic field is normalized to velocity units by using the Alfvén speed ﹩b=\frac{B}{\sqrt{{\mu }_{0}\rho }}﹩. The radius of the polarization circle is equal to the background magnetic field b0. The stack bar indicates the radial components δvr and br.

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