Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 9.

The maximum Lorentz factor along rays of constant polar angle θ, as a function of time, for the simulations listed in Table 3. Shock dissipation pushes inward to a smaller radius, due to constructive interference between the FMS wave and the large-amplitude wiggles.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse