The kinetic Alfven wave instability driven by a sheared plasma flow and the associated anomalous transport
Abstract
It is shown that the kinetic Alfven wave instability can be driven by a sheared plasma flow. The dispersion relation is derived. The wave characteristics and associated anomalous transport are investigated. Calculations indicate that the cross-field diffusion coefficient can reach 10 to the 9th m sq/sec, while the magnetic field perturbations are only about 1 nT at the earth's magnetopause. Therefore, it can be expected that the kinetic Alfven wave turbulence may lead to strong anomalous transport, which is responsible for sustaining the quasi-static boundary-layer structure and the magnetospheric convection.
- Publication:
-
Scientia Sinica Series Mathematical Physical Technical Sciences
- Pub Date:
- March 1986
- Bibcode:
- 1986SSSMP..29..301P
- Keywords:
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- Magnetohydrodynamic Flow;
- Magnetohydrodynamic Stability;
- Plasma Waves;
- Shear Flow;
- Anomalies;
- Kinetic Theory;
- Magnetospheric Instability;
- Solar Wind;
- Space Plasmas;
- Viscosity;
- Wave Dispersion;
- Geophysics