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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 6.

Radial evolution of magnetic and velocity fluctuation energy. The scatter points are colored by Alfvén Mach number MA. Panels (a) and (d) are for the radial component, panels (b) and (e) are for the transverse component, and panels (c) and (f) are for the sum of all components. The solid black lines exhibit the averaged data by 3 Rs bins. The green dashed lines are the results from least-squares linear fitting of the averaged data. Panels (g), (h), and (i) show the comparisons of linear fitting results for the three columns.

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