Stability of solar atmospheric structures harboring standing slow waves
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DOI: 10.1051/0004-6361/202140534
Abstract: Context. In the context of the solar coronal heating problem, one possible explanation for the high coronal temperature is the release of energy by magnetohydrodynamic (MHD) waves. The energy transfer is believed to be possible,… read more here.
Keywords: stability; standing slow; atmospheric structures; solar atmospheric ... See more keywords