In Bifrost simulations of the quiet Sun and coronal hole, acoustic waves near the cut-off frequency dissipate most of their energy as viscous heating at the plasma-beta=1 interface.
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Characteristics of acoustic-wave heating in simulations of the quiet Sun chromosphere
In Bifrost simulations of the quiet Sun and coronal hole, acoustic waves near the cut-off frequency dissipate most of their energy as viscous heating at the plasma-beta=1 interface.