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Statistical Method for Astrophysical Turbulence Investigation

  • A. Lazarian (a1)
Abstract

Present-day galactic dynamo theories widely use a concept of the ISM turbulence. In the present paper a statistical method of MHD turbulence study is discussed. The method is based on the solution of the inverse problem for the observational data. It is shown that in many important cases the inverse problem has a unique analytical solution. Examples, including the study of a random density field and a random magnetic field, are discussed.

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References
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Kaplan, S.A. and Pickelner, S.B.: 1970, The Interstellar Medium , Harvard University Press.
Kleiner, S.C. and Dickman, R.L.: 1984, ApJ. , 286, 255.
Lazarian, A. and Chibisov, G.V.: 1987, Preprint FIAN 283.
Lazarian, A. and Shutenkov, V.R.: 1991, Sov. Astron. Lett. , 16, 297.
Lazarian, A.: 1991, in Fragmentation of Molecular Clouds and Star Formation , eds. Falgarone, E., Boulanger, F. and Dubert, G., Kluwer, p. 65.
Lazarian, A.: 1992a, Astron and Astrophys Transactions , 3, 33.
Lazarian, A.: 1992b, in Proc. of the ESA Colloquium, Targets for Space-Based Interferometry , 13–16 October, Beaulieu, France.
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0074-1809
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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