Published December 2008 | Version v1
Journal article

Interaction of a thin shock with turbulence. I. Effect on shock structure: Analytic model

  • 1. Department of Physics and Institute of Geophysics and Planetary Physics, University of California, Riverside, California 92521 (United States) and Center for Space Plasma and Aeronomic Research, Huntsville, Alabama 35805 (United States)
  • 2. Institute of Geophysics and Planetary Physics, University of California, Riverside, California 92521 (United States) and Center for Space Plasma and Aeronomic Research, Huntsville, Alabama 35805 (United States)

Description

A two-dimensional magnetohydrodynamical model describing the interaction of thin shock waves with turbulence is developed by adopting a multiscale perturbation analysis. The interaction is found to be governed by a two-dimensional inviscid Burgers' equation that includes ''perturbation terms.'' Initially prescribed perturbation profiles are explored with numerical simulations to show how the shock front is modified by turbulence. Our numerical simulations show that magnetic field perturbations play a very important role in modifying the structure of perpendicular and parallel shocks. While turbulence can balance the nonlinear steepening of a shock wave at some regions, it can also help to create a larger jump in physical quantities such as the magnetic field at other regions. The plasma medium in these regions can therefore experience a higher compression, which will result in a downstream state that differs from the usual Rankine-Hugoniot state

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Fluids (1994)
Journal Volume
20
Journal Issue
12
Journal Page Range
p. 127102-127102.19
ISSN
1070-6631
CODEN
PHFLE6

Optional Information

Notes
(c) 2008 American Institute of Physics