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Global Magnetohydrodynamic Simulations of Monster Shocks in Neutron Star Magnetospheres

  • Authors: Michael P. Grehan, Bart Ripperda, Andrei M. Beloborodov, Christopher Thompson, Elias R. Most

Michael P. Grehan et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 4.

The radial E × B velocity at t = 4RNS/c in spherical FMS wave simulation sigma100. White arrows show the direction of flow in regions with Lorentz factor over a fixed threshold. Solid white lines are placed at ﹩\sin \theta =\pm 2/\sqrt{5}﹩, the angle at which the radial velocity is expected to change sign for the Bw · Bbg < 0 portion of the wave.

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