Fast magnetoacoustic waves steepen and dissipate nonlinearly before reaching coronal magnetic null points due to decreasing fast speed in the non-uniform magnetic field.
2012 Modelling the Propagation of a Weak Fast-Mode MHD Shock Wave near a 2D Magnetic Null Point Using Nonlinear Geometrical Acoustics.Solar Phys.280, 561–574
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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.