Journal of Geophysical Research Atmospheres · 1989 · 48 citations · 22 references
Natural SciencesPhysicsComputational PhysicsElectromagnetismPlasma PhysicsMagnetohydrodynamicsPlasma InstabilitiesPlasma SimulationShock WavesHybrid SimulationMhd StabilityShock DynamicsShock Formation In PlasmasShock Wave ModelingShock Wave StabilityShock Wave StructureShock Waves In Magnetized Plasmas
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.
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The structure of perpendicular bow shocks
M. Leroy, D. Winske, C. C. Goodrich et al. · Journal of Geophysical Research Atmospheres · 1982 · 489 citations · Full text
Aerodynamic aspects of the magnetospheric flow
Richard Levy, H. E. Petschek, G. L. Siscoe · AIAA Journal · 1964 · 445 citations