The Coronal Power Spectrum from MHD Mode Conversion above Sunspots
Sunspots are intense regions of magnetic flux that are rooted deep below the photosphere. It is well established that sunspots host magnetohydrodynamic waves, with numerous observations showing a connection to the internal acoustic (or p-)modes of the Sun. The p-modes are fast waves below the equipartition layer and are thought to undergo a double
Miriyala, Hemanthi et al.
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2025