Fast magnetoacoustic waves steepen and dissipate nonlinearly before reaching coronal magnetic null points due to decreasing fast speed in the non-uniform magnetic field.
1994 What is the Condition for Fast Magnetic Reconnection?
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Nonlinear steepening of a fast magnetoacoustic wave in the vicinity of a coronal magnetic null point
Fast magnetoacoustic waves steepen and dissipate nonlinearly before reaching coronal magnetic null points due to decreasing fast speed in the non-uniform magnetic field.