Two-fluid simulations show that decoupling of ions and neutrals damps fast magneto-acoustic waves in the chromosphere and produces frictional heating, with linear WKB theory matching the damping.
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Two-fluid simulations of waves in the solar chromosphere II. Propagation and damping of fast magneto-acoustic waves and shocks
Two-fluid simulations show that decoupling of ions and neutrals damps fast magneto-acoustic waves in the chromosphere and produces frictional heating, with linear WKB theory matching the damping.