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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Bibliographic Details
Published inJournal of Geophysical Research: Space Physics Vol. 115; no. A12
Main Authors Gary, S. Peter, Liu, Kaijun, Winske, Dan, Denton, Richard E.
Format Journal Article
LanguageEnglish
Published Washington, DC Blackwell Publishing Ltd 01.12.2010
American Geophysical Union
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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).
Bibliography:ark:/67375/WNG-BWBV8RLK-V
istex:7FEB89DF94A069989AA7A3D2D7956663A66B687F
ArticleID:2010JA015965
ISSN:0148-0227
2169-9380
2156-2202
2169-9402
DOI:10.1029/2010JA015965