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Generation of Large Scale Structures in Three-Dimensional Anisotropic Incompressible Flow Lacking Parity-Invariance

  • P.-L. Sulem
  • U. Frisch
  • H. Scholl
  • Z. S. She
Part of the NATO ASI Series book series (NSSB, volume 237)

Abstract

In MHD, an instability, called the alpha-effect, is believed to be at the origin of the generation of large-scale magnetic fields in many cosmical objects (Moffatt 1978, Zeldovich, Ruzmaikin and Sokoloff 1983).

References

  1. Frisch, U., She, Z.S. and Sulem, P.L. 1987 Physica 28D, 382.Google Scholar
  2. Moffatt, H.K. 1978 Magnetic Field Generation in Electrically Conducting Fluids. Cambridge Univ. Press.Google Scholar
  3. Sulem, P.L., She, Z.S., Scholl, H., Frisch, U. 1989 J. Fluid Mech. 205, 341.MathSciNetCrossRefGoogle Scholar
  4. Zeldovich, Ya.B., Ruzmaikin A.A. and Sokolov D.D. 1983 Magnetic fields in Astrophysics,Gordon and Breach.Google Scholar

Copyright information

© Plenum Press, New York 1990

Authors and Affiliations

  • P.-L. Sulem
    • 1
    • 2
  • U. Frisch
    • 1
  • H. Scholl
    • 1
    • 3
  • Z. S. She
    • 4
    • 5
  1. 1.Observatoire de NiceCNRSNice CedexFrance
  2. 2.School of Mathematical SciencesTel Aviv UniversityIsrael
  3. 3.Astron. Rechen-Inst.HeidelbergGermany
  4. 4.Appl. Comput. Math.Princeton UniversityUSA
  5. 5.Nanjing UniversityNanjingP.R. China

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