Quasi-perpendicular fast magnetosonic shock with wave precursor in collisionless plasma

Abstract

A one-dimensional particle-in-cell (PIC) simulation tracks a fast magnetosonic shock over time scales comparable to an inverse ion gyrofrequency. The magnetic pressure is comparable to the thermal pressure upstream. The shock propagates across a uniform background magnetic field with a pressure that equals the thermal pressure upstream at the angle 85${}^{\circ }$ at a speed that is 1.5 times the fast magnetosonic speed in the electromagnetic limit. Electrostatic contributions to the wave dispersion increase its phase speed at large wave numbers, which leads to a convex dispersion curve. A fast magnetosonic precursor forms ahead of the shock with a phase speed that exceeds the fast magnetosonic speed by about $\sim 30\%$. The wave is slower than the shock and hence it is damped.

arXiv comment4 pages, 3 figures

References in corpus (5)

• On Kinetic Slow Modes, Fluid Slow Modes, and Pressure-balanced Structures in the Solar Wind
• On the role of magnetosonic solitons in perpendicular collisionless shock reformation
• Expansion of a radially symmetric blast shell into a uniformly magnetized plasma
• Emergence of MHD structures in a collisionless PIC simulation plasma
• Particle-in-cell simulation study of a lower-hybrid shock