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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 4.

From left to right: ﹩{v}_{xy}^{\mathrm{total}}﹩, vz, and compressibility (﹩{\boldsymbol{\nabla }}\cdot {\boldsymbol{v}}﹩) on the xy plane for four time steps. The yellow and blue contours represent the fast magnetoacoustic and Alfvén parts, respectively, to distinguish ﹩{v}_{xy}^{\mathrm{total}}﹩ and vz components of the velocity. The associated velocity amplitude range of the contour has been taken to be 30–35 km s−1. The field of view (FOV) of the entire panel shown here is equivalent to the yellow dotted box shown in Figure 3 with dimensions [X,Y] = [(−70 Mm to −10 Mm), (60 Mm to 110 Mm)]. An animation of the above variables from 0 to 1025 s is available in the online version with a real-time duration of 10 s.

(An animation of this figure is available in the online article.)

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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