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NASA NTRS · 19840057106

Ion viscous effects on magnetosonic shock

Abstract

Profiles of magnetic field and plasma bulk velocity associated with perpendicular shocks are investigated theoretically by solving magnetohydrodynamic equations. The main dissipation mechanism is assumed to be due to ion viscosity. Shock structures with zero temperatures and finite pressure are examined separately. The numerical solutions indicate that ion viscosity tends to smooth profiles of magnetic field and bulk velocity for high Mach number shocks. For smaller ion viscosity and lower Mach number, a damped wave train would appear downstream. The results suggest that kinetic effects such as ion reflections and microturbulence are necessary in order to explain magnetic field overshoots as well as oscillatory magnetic-field structure in high Mach number shocks.

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BibTeXRIS

Lin, C. S., Lee, L. C., Wu, C. S.. 1984-06-01. Ion viscous effects on magnetosonic shock. https://ntrs.nasa.gov/citations/19840057106

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