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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 3.

2D and 1D plots of the diffusion profile. The dotted lines indicate the height at which the sigmoid is centered (zc). The dashed lines indicate the height we consider for computing the Alfvén power spectrum.

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