Pressure anisotropy generation in a magnetized plasma configuration with a shear flow velocity
Year: 2016
Authors: De Camillis S., Cerri S.S., Califano F., Pegoraro F.
Autors Affiliation: Univ Pisa; Queens Univ Belfast; Max Planck Inst Plasmaphys Garching
Abstract: The nonlinear evolution of the Kelvin Helmholtz instability in a magnetized plasma with a perpendicular flow close to, or in, the supermagnetosonic regime can produce a significant parallel-to-perpendicular pressure anisotropy. This anisotropy, localized inside the flow shear region, can make the configuration unstable either to the mirror or to the firehose instability and, in general, can affect the development of the KHI. The interface between the solar wind and the Earth?s magnetospheric plasma at the magnetospheric equatorial flanks provides a relevant setting for the development of this complex nonlinear dynamics.
Journal/Review: PLASMA PHYSICS AND CONTROLLED FUSION
Volume: 58 (4) Pages from: to:
KeyWords: pressure anisotropy, shear flow, plasma instabilitiesDOI: 10.1088/0741-3335/58/4/045007ImpactFactor: 2.392Citations: 11data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2024-10-13References taken from IsiWeb of Knowledge: (subscribers only)Connecting to view paper tab on IsiWeb: Click hereConnecting to view citations from IsiWeb: Click here