Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT 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 4.

The frequency dependence of the wave driver, comparing the broadband driver (blue dots) used in the simulation with the observed p-mode power spectrum (red solid line) from Michelson Doppler Imager of the Solar and Heliospheric Observatory (E. J. J. Rhodes et al. 1997). The black line is the average trend fitted to the observed p-mode power spectrum.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse