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    請使用永久網址來引用或連結此文件: https://ir.lib.ncu.edu.tw/handle/987654321/102162


    題名: Effects of Hall current and electron temperature anisotropy on proton fire-hose instabilities
    作者: 郝玲妮;Hau, L.-N.;Wang, B.-J.
    貢獻者: 地球科學學院太空科學與工程學系
    關鍵詞: 70 PLASMA PHYSICS AND FUSION TECHNOLOGY;ALFVEN WAVES;ANISOTROPY;APPROXIMATIONS;Computational fluid dynamics;Cyclotrons;DISPERSION RELATIONS;Electron energy;ELECTRON TEMPERATURE;ELECTRONS;Fluid flow;HOSE INSTABILITY;ION TEMPERATURE;Linear polarization;MAGNETIC FIELDS;MAGNETOHYDRODYNAMICS;MOMENT OF INERTIA;OHM LAW;Ohm's Law;PLASMA;Plasma physics;POLARIZATION;Propagation modes;PROTONS;Stability;Two fluid models;Wave propagation;WHISTLERS
    日期: 2013-10-01
    上傳時間: 2026-04-23 11:03:37 (UTC+8)
    出版者: American Institute of Physics;Melville: American Institute of Physics
    摘要: 摘要: The standard magnetohydrodynamic (MHD) theory predicts that the Alfvén wave may become fire-hose unstable for β∥−β⊥>2. In this study, we examine the proton fire-hose instability (FHI) based on the gyrotropic two-fluid model, which incorporates the ion inertial effects arising from the Hall current and electron temperature anisotropy but neglects the electron inertia in the generalized Ohm's law. The linear dispersion relation is derived and analyzed which in the long wavelength approximation, λik→0 or αe=μ0(p∥,e−p⊥,e)/B2=1, recovers the ideal MHD model with separate temperature for ions and electrons. Here, λi is the ion inertial length and k is the wave number. For parallel propagation, both ion cyclotron and whistler waves become propagating and growing for β∥−β⊥>2+λi2k2(αe−1)2/2. For oblique propagation, the necessary condition for FHI remains to be β∥−β⊥>2 and there exist one or two unstable fire-hose modes, which can be propagating and growing or purely growing. For large λik values, there exists no nearly parallel FHI leaving only oblique FHI and the effect of αe>1 may greatly enhance the growth rate of parallel and oblique FHI. The magnetic field polarization of FHI may be reversed due to the sign change associated with (αe−1) and the purely growing FHI may possess linear polarization while the propagating and growing FHI may possess right-handed or left-handed polarization.
    出版者: Melville: American Institute of Physics
    出版日期: 2013-10-01
    出處: Physics of plasmas, 2013-10, Vol.20 (10)
    資源來源: AIP Journals (American Institute of Physics)
    版權: 2013 AIP Publishing LLC.
    識別號: ISSN: 1070-664X
    識別號: ISSN: 1527-2419
    識別號: ISSN: 1089-7674
    識別號: EISSN: 1089-7674
    識別號: DOI: 10.1063/1.4824333
    顯示於類別:[太空科學與工程學系] 期刊論文

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