On the stability of rotational discontinuities and intermediate shocks
Open Access
- 1 July 1989
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 94 (A7) , 8813-8825
- https://doi.org/10.1029/ja094ia07p08813
Abstract
The stability of rotational discontinuities and intermediate shocks is studied based on a hybrid simulation code. The simulation results show that rotational discontinuities are stable and intermediate shocks are not stationary. Intermediate shocks tend to evolve to rotational discontinuities and waves. We employ several different initial profiles for the magnetic field in the transition region and find that the final structure of the discontinuities or shocks is not sensitive to the initial magnetic field profile. The present results are different from those obtained from the resistive MHD simulations. Furthermore, our study indicates that the kinetic effect of particles plays an important role in the structure and stability of rotational discontinuities and intermediate shocks.Keywords
This publication has 22 references indexed in Scilit:
- Increase of ion kinetic temperature across a collisionless shock: 2. A simulation studyJournal of Geophysical Research, 1987
- Magnetic field rotation through the magnetopause: ISEE 1 and 2 observationsJournal of Geophysical Research, 1982
- The structure of perpendicular bow shocksJournal of Geophysical Research, 1982
- Solar wind energy transfer through the magnetopause of an open magnetosphereJournal of Geophysical Research, 1982
- Structure of the magnetopause rotational discontinuityJournal of Geophysical Research, 1982
- Fine‐scale characteristics of interplanetary sector boundariesJournal of Geophysical Research, 1981
- Magnetic field directional discontinuities: 1. Minimum variance errorsJournal of Geophysical Research, 1980
- Nature and origin of directional discontinuities in the solar windJournal of Geophysical Research, 1971
- Discontinuities in an anisotropic plasma and their identification in the solar windPlanetary and Space Science, 1970
- Aerodynamic aspects of the magnetospheric flowAIAA Journal, 1964