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The Coronal Power Spectrum from MHD Mode Conversion above Sunspots

  • Authors: Hemanthi Miriyala, Richard J. Morton, Elena Khomenko, Patrick Antolin, Gert J.J. Botha

Hemanthi Miriyala et al 2025 The Astrophysical Journal 979 .

  • Provider: AAS Journals

Caption: Figure 5.

Velocity projections of slow (left), fast (middle), and Alfvén (right) waves at a snapshot at 1163 s. The green contour is the equipartition layer. The vertical dashed line is where θ = 30 and ϕ = 56 at the equipartition layer. The velocities are scaled by a factor of ﹩\sqrt{{\rho }_{0}{c}_{s}}﹩ for the left panel and ﹩\sqrt{{\rho }_{0}{v}_{{\rm{A}}}}﹩ for the middle and right panels.

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