Issues

 / 

1985

 / 

April

  

Reviews of topical problems


Kinematic dynamo in random flow

The growth of a magnetic field in a given random flow of a well-conducting liquid is considered. The known Lagrange solution for the transport of a frozen-in magnetic field is utilized. Magnetic diffusion is taken into account by averaging the result of this transport over a set of random trajectories. This permits a derivation of the equations for the mean magnetic field and its moments, as well as an investigation of the true (random) magnetic field. The field and its moments increase exponentially in the limit of large magnetic Reynolds numbers, and the field distribution becomes intermittent. The analysis is devoted mainly to streams that are restored after a definite time interval, but stationary flows with stochastic properties are also discussed.

Fulltext pdf (986 KB)
Fulltext is also available at DOI: 10.1070/PU1985v028n04ABEH003869
PACS: 47.65.−d, 47.27.Jv, 47.10.A− (all)
DOI: 10.1070/PU1985v028n04ABEH003869
URL: https://ufn.ru/en/articles/1985/4/b/
Citation: Molchanov S A, Ruzmaikin A A, Sokolov D D "Kinematic dynamo in random flow" Sov. Phys. Usp. 28 307–327 (1985)
BibTexBibNote ® (generic)BibNote ® (RIS)MedlineRefWorks

Оригинал: Молчанов С А, Рузмайкин А А, Соколов Д Д «Кинематическое динамо в случайном потоке» УФН 145 593–628 (1985); DOI: 10.3367/UFNr.0145.198504b.0593

Cited by (85) Similar articles (20) ↓

  1. S.I. Vainshtein, Ya.B. Zel’dovich “Origin of Magnetic Fields in Astrophysics (Turbulent ’Dynamo’ Mechanisms)15 159–172 (1972)
  2. Ya.B. Zel’dovich, S.A. Molchanov et alIntermittency in random media30 353–369 (1987)
  3. Ya.B. Zeldovich, A.A. Ruzmaikin “The hydromagnetic dynamo as the source of planetary, solar, and galactic magnetism30 494–506 (1987)
  4. O.G. Bakunin “Reconstruction of streamline topology, and percolation models of turbulent transport56 243–260 (2013)
  5. L.M. Zelenyi, A.I. Neishtadt et alQuasiadiabatic dynamics of charged particles in a space plasma56 347–394 (2013)
  6. G.M. Zaslavskii, B.V. Chirikov “Stochastic instability of non-linear oscillations14 549–568 (1972)
  7. V.I. Klyatskin “Integral characteristics: a key to understanding structure formation in stochastic dynamic systems54 441–464 (2011)
  8. A.Z. Dolginov “Origin of the magnetic fields of the earth and celestial bodies30 475–493 (1987)
  9. V.I. Klyatskin, D. Gurarie “Coherent phenomena in stochastic dynamical systems42 165 (1999)
  10. A.B. Severnyi “Magnetic fields of the Sun and stars9 1–30 (1966)
  11. F.V. Dolzhanskii, V.A. Krymov, D.Yu. Manin “Stability and vortex structures of quasi-two-dimensional shear flows33 (7) 495–520 (1990)
  12. A.N. Kolmogorov “Local structure of turbulence in an incompressible viscous fluid at very high Reynolds numbers10 734–746 (1968)
  13. K.P. Zybin, V.A. Sirota “Stretching vortex filaments model and the grounds of statistical theory of turbulence58 556–573 (2015)
  14. A.S. Mikhailov, I.V. Uporov “Critical phenomena in media with breeding, decay, and diffusion27 695–714 (1984)
  15. A.S. Monin “Hydrodynamic instability29 843–868 (1986)
  16. I.M. Lifshits, A.Yu. Grosberg, A.R. Khokhlov “Volume interactions in the statistical physics of a polymer macromolecule22 123–142 (1979)
  17. A.S. Monin “On the nature of turbulence21 429–442 (1978)
  18. A.A. Vedenov, E.P. Velikhov, R.Z. Sagdeev “STABILITY OF PLASMA4 332–369 (1961)
  19. A. Loskutov “Fascination of chaos53 1257–1280 (2010)
  20. A.S. Monin “ATMOSPHERIC DIFFUSION2 50–58 (1959)

The list is formed automatically.

© 1918–2024 Uspekhi Fizicheskikh Nauk
Email: ufn@ufn.ru Editorial office contacts About the journal Terms and conditions