pith. sign in

arxiv: 1003.1275 · v1 · pith:H26QBFEEnew · submitted 2010-03-05 · 🌌 astro-ph.HE · astro-ph.GA

Observation of the growth of a magnetic vortex in the transition layer of a mildly relativistic oblique plasma shock

classification 🌌 astro-ph.HE astro-ph.GA
keywords magneticfieldcollisionplasmasheetalongburstcloud
0
0 comments X
read the original abstract

A 2D particle simulation models the collision of two electron-ion plasma clouds along a quasi-parallel magnetic field. The collision speed is 0.9c and the density ratio 10. A current sheet forms at the front of the dense cloud, in which the electrons and the magnetic field reach energy equipartition with the ions. A structure composed of a solenoidal and a toroidal magnetic field grows in this sheet. It resembles that in the cross-section of the torus of a force-free spheromak, which may provide the coherent magnetic fields in gamma-ray burst (GRB) jets needed for their prompt emissions.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.