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Interaction of a Fast Magnetoacoustic Wave with the Localized Coronal Null and Generation of the Energetic Alfvén Wave Packet

  • Authors: Akash Bairagi, Abhishekh K. Srivastava, Sripan Mondal, T. V. Zaqarashvili, Astrid Veronig, P. Bourdin, Ding Yuan, Ryun-Young Kwon

Akash Bairagi et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 8.

Top left panel: v/cA map of the fast magnetoacoustic perturbation at t = 5 s; the dotted red line represents a curved slit chosen from bottom to top through the null region. The FOV of the zoomed-in region of the numerical domain is x = [−20 Mm, 60 Mm], y = [0 Mm, 80 Mm], and the black circular contour represents the β = 1 layer. Top right panel: the spatial variation of the normalized Alfvén speed (cA/V*) along S1 at t = 0 s; the vertical blue dotted line represents the β = 1 layer on the path of S1. Bottom panels: the spatial characteristics of the ratio of magnetoacoustic perturbation amplitude and local Alfvén speed (v/cA) on the slit S1 at t = 5 s, t = 26 s, and t = 57 s (left to right).

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