Ion Bernstein instability in the terrestrial magnetosphere: Linear dispersion theory
Linear kinetic dispersion theory for electromagnetic fluctuations in a homogeneous, magnetized, collisionless plasma is used to study the properties of an ion Bernstein mode instability driven by a proton velocity distribution fp(v) such that ∂fp(ν⊥)/∂ν⊥ > 0, where ⊥ denotes directions perpendicu...
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Published in | Journal of Geophysical Research: Space Physics Vol. 115; no. A12 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Washington, DC
Blackwell Publishing Ltd
01.12.2010
American Geophysical Union |
Subjects | |
Online Access | Get full text |
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Summary: | Linear kinetic dispersion theory for electromagnetic fluctuations in a homogeneous, magnetized, collisionless plasma is used to study the properties of an ion Bernstein mode instability driven by a proton velocity distribution fp(v) such that ∂fp(ν⊥)/∂ν⊥ > 0, where ⊥ denotes directions perpendicular to the background magnetic field Bo. Here fp(v) = f1(ν) − f2(ν), where f1 and f2 are Maxwellian velocity distributions with slightly different densities and temperatures; plasma parameters are taken from magnetospheric observations. Then the growth rate of this instability has relative maxima at ωr ≃ nΩp, where n = 1, 2, 3, … and Ωp is the proton cyclotron frequency; wave vector k at 0 < k∥ ≪ k⊥, where ∥ and ⊥ denote the directions parallel and perpendicular to Bo; and wavelengths of the order of or smaller than the proton gyroradius. The maximum instability growth rate is a monotonically decreasing function of the electron‐to‐proton temperature ratio but has its largest value at an intermediate value of the proton β (∼0.5 for the parameters considered here). |
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Bibliography: | ark:/67375/WNG-BWBV8RLK-V istex:7FEB89DF94A069989AA7A3D2D7956663A66B687F ArticleID:2010JA015965 |
ISSN: | 0148-0227 2169-9380 2156-2202 2169-9402 |
DOI: | 10.1029/2010JA015965 |