Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-30T06:51:12.218Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Nature of Magnetohydrodynamic Turbulence in the Interstellar Medium

Published online by Cambridge University Press:  19 July 2016

V.N. Fedorenko
V.N. Fedorenko*
Affiliation:
A.F. Ioffe Physical Technical Institute 194021 Leningrad USSR

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Various mechanisms of creation of the extended spectrum of MHD turbulence in the interstellar medium are reviewed. Within the scales 1014 cm ≲ L ≲ 1019 cm the turbulence mostly consists of the ensemble of weak shock waves. At 1012 cm ≲ L ≲ 1014 cm the principle mechanism is generation of MHD waves by cosmic rays.

Type
4. Magnetohydrodynamics of Galactic Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 153 - 154
Copyright
Copyright © Kluwer 1990 

References

Bykov, A.M. and Toptygin, I.N. (1987) Astrophys. Space Sci. 138, 341–354.Google Scholar
Fedorenko, V.N., Fleischman, G.D., and Ostryakov, V.M. (1987) Proceed. 20th Int. Cosmic Ray Conference Moscow, Vol. 2, pp. 235–238.Google Scholar
Fedorenko, V.N., Ostryakov, V.M., Polyudov, A.N., and Shapiro, V.D. (1988) “Induced Scattering and Two-Quanta Absorption of Alfvén Waves in Plasmas With Arbitrary β”, Preprint No. 1267, A.F. Ioffe Physical Technical Institute, Leningrad.Google Scholar
McIvor, I. (1977) Mon. Not. Roy. Astron. Soc. 179, 13.Google Scholar
Wentzel, D.G. (1974) Ann. Rev. Astron. Astrophys. 12, 71.CrossRefGoogle Scholar