Microinstabilities associated with a high Mach number, perpendicular bow shock

Details Microinstabilities associated with a high Mach number, perpendicular bow shock Microinstabilities associated with a high Mach number, perpendicular bow shock

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ssrv...37...63w&link_type=abstract

Space Science Reviews (ISSN 0038-6308), vol. 37, Jan.-Feb. 1984, p. 63-109.

Computer Science

Sound

74

Bow Waves, Mach Number, Magnetohydrodynamic Stability, Normal Shock Waves, Plasma Waves, Solar Terrestrial Interactions, Computerized Simulation, Electric Field Strength, Electron Cyclotron Heating, Ion Motion, Magnetic Flux, Plasma Acceleration, Plasma Turbulence

Scientific paper

Instability analyses incorporating insights gained through ISEE observations and hybrid simulations are used in an examination of the instabilities associated with a high Mach number perpendicular shock akin to the earth's bow shock. In the regions in front of, and at, the shock transition the cross-field instabilities are subdivided into the ion-ion streaming, kinetic cross-field streaming, and drift lower hybrid instability low frequency modes, as well as the electron cyclotron drift, ion sound, and electron whisker instability high frequency modes. Further downstream, ion ring-like and anisotropy-driven instabilities are considered. The implications of these results for wave signatures, plasma heating and acceleration are noted.

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