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Monster Radiative Shocks in the Perturbed Magnetospheres of Neutron Stars

  • Authors: Andrei M. Beloborodov

Andrei M. Beloborodov 2023 The Astrophysical Journal 959 .

  • Provider: AAS Journals

Caption: Figure 2.

A magnetosonic wave with wavevector k B bg at two oscillation phases: when the wave field B w = B B bg is aligned with B bg (left) and antialigned with B bg (right). The wave electric field E w = E is always orthogonal to B bg. The quantity B 2E 2 reaches zero when B w = − B bg/2. At this moment, the plasma drift speed v = c E × B /B 2 approaches c, so it experiences ultrarelativistic acceleration in the direction opposite to the wave propagation direction.

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