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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 7.

Temporal evolution of the WEF for the Alfvén wave packet at the different positions on the slit S3 (see Figure 5). Here the dotted line and the solid line respectively correspond to kinetic and total energy (kinetic+magnetic) associated with the WEF. At point “a” the packet has an energy flux of about 2140 W m−2, which then decreases gradually at the different points owing to the curved magnetic field. Thereafter it reaches a constant value of 860 W m−2 and propagates up to very far distance along the horizontal field line.

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