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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 12.

The toroidal component of the magnetic and ideal electric field, Bϕ and Eϕ, for an MHD monster shock initiated through the launching of A waves from the stellar boundary. The outline of mesh blocks is shown in white, with each block containing 16 radial cells and 8 angular cells. The plotted simulation has domain r/RNS ∈ [1, 10] and θ ∈ [0, π] with a base grid of 2048 × 512 cells and three levels of mesh refinement for a maximum effective resolution of 16384 × 4096.

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