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Volumn 9, Issue 12, 2002, Pages 4856-4862

Kelvin-Helmholtz instability in Beltrami fields

Author keywords

[No Author keywords available]

Indexed keywords

EIGENVALUES AND EIGENFUNCTIONS; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; PLASMA FLOW;

EID: 0036933482     PISSN: 1070664X     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.1518679     Document Type: Article
Times cited : (8)

References (25)
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    • J. B. Taylor, Phys. Rev. Lett. 33, 1139 (1974); Rev. Mod. Phys. 58, 741 (1986).
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    • J. A. Tataronis and W. Grossmann, Z. Phys. 261, 203 (1973); A. Hasegawa and C. Uberoi, The Alfvén Wave, DoE Critical Review Series DOE/TIC-11197 (Technical Information Center, U. S. Department of Energy, Springfield, VA, 1982); Z. Yoshida and S. M. Mahajan, Int. J. Mod. Phys. B 9, 2857 (1995).
    • (1973) Z. Phys. , vol.261 , pp. 203
    • Tataronis, J.A.1    Grossmann, W.2
  • 14
    • 0001036408 scopus 로고
    • Technical Information Center, U. S. Department of Energy, Springfield, VA
    • J. A. Tataronis and W. Grossmann, Z. Phys. 261, 203 (1973); A. Hasegawa and C. Uberoi, The Alfvén Wave, DoE Critical Review Series DOE/TIC-11197 (Technical Information Center, U. S. Department of Energy, Springfield, VA, 1982); Z. Yoshida and S. M. Mahajan, Int. J. Mod. Phys. B 9, 2857 (1995).
    • (1982) The Alfvén Wave, DoE Critical Review Series DOE/TIC-11197
    • Hasegawa, A.1    Uberoi, C.2
  • 15
    • 0001036408 scopus 로고
    • J. A. Tataronis and W. Grossmann, Z. Phys. 261, 203 (1973); A. Hasegawa and C. Uberoi, The Alfvén Wave, DoE Critical Review Series DOE/TIC-11197 (Technical Information Center, U. S. Department of Energy, Springfield, VA, 1982); Z. Yoshida and S. M. Mahajan, Int. J. Mod. Phys. B 9, 2857 (1995).
    • (1995) Int. J. Mod. Phys. B , vol.9 , pp. 2857
    • Yoshida, Z.1    Mahajan, S.M.2
  • 20
    • 0036536587 scopus 로고    scopus 로고
    • However, those "secular" behavior is at most algebraic in t. If KH mode is unstable (Im ω > 0 ), it dominates the long-term behavior
    • Due to the non-Hermitian property of the system, eigenfunctions of modes are not orthogonal with each other. Hence, KH-mode may couple with other modes (including continuous spectra). Such mode couplings may bring about rather complex time-asymptotic phenomena [see M. Hirota, T. Tatsuno, S. Kondoh, and Z. Yoshida, Phys. Plasmas 9, 1177 (2002)]. However, those "secular" behavior is at most algebraic in t. If KH mode is unstable (Im ω > 0 ), it dominates the long-term behavior.
    • (2002) Phys. Plasmas , vol.9 , pp. 1177
    • Hirota, M.1    Tatsuno, T.2    Kondoh, S.3    Yoshida, Z.4
  • 23
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    • G. D. Chagelishvili, T. S. Hristov, R. G. Chanishvili, and J. G. Lominadze, Phys. Rev. E 47, 366 (1993); G. D. Chagelishvili, A. D. Rogava, and I. N. Segal, ibid. 50, 4283 (1994).
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    • Chagelishvili, G.D.1    Rogava, A.D.2    Segal, I.N.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.