Image Details

Choose export citation format:

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 7.

Cutoff frequency across the background condition. The white contours refer to the magnetic field lines. The vertical white dashed–dotted line refers to the slit we considered to achieve the results in Figure 6. The solid black line across the domain is the equipartition layer (cs = vA). The dashed and dotted lines refer to the cutoff layers where vac = 4 mHz and 3 mHz, respectively. We have clipped the regions within the yellow dashed rectangular box to achieve the plot on right for better visualization purposes.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse