Generalisation of a nonlinear dynamo model

Studia Geophysica et Geodaetica

Volumn 42, Issue 3, 1998, Pages 343-349

  Tanner, Sarah E M ^a   Hughes, D W ^a  

^a UNIVERSITY OF LEEDS   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

FLUID DYNAMICS; MAGNETIC FIELD; ROTATION;

GEODYNAMO; MAGNETIC FIELD;

EID: 0031659559     PISSN: 00393169     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1023313005610     Document Type: Article

References (7)

1. Canuto, V.M., 1996: Turbulent convection - old and new models. Astrophys. J., 467, 385-396
2. Cattaneo, F., Hughes, D.W. and Kim, E.J., 1996: Suppression of chaos in a simplified nonlinear dynamo model. Phya. Rev. Lett., 76, 2057-2060
3. Galloway, D.J. and Proctor, M.R.E, 1992: Numerical calculations of fast dynamos in smooth velocity fields with realistic diffusion. Nature., 356, 691-693
4. Klapper, I. and Young, L.S., 1995: Rigorous bounds on the fast dynamo growth-rate involving topological entropy. Communications in Mathematical Physics, 175, 623-646
5. Vainshtein, S.I. and Zeldovich, Ya.B., 1972: Origin of magnetic fields in astrophysics. Sov. Phya. Usp., 15, 159-172
6. Vishik, M.M., 1989: Magnetic field generation by the motion of a highly conducting fluid. Geophys. Astrophys. Fluid Dyn., 48, 151-167
7. Zeldovich, Ya.B., Ruzmaikin, A.A. and Sokoloff, D.D., 1983: In: Magnetic Fields in Astrophysics. The Fluid Mechanics of Astrophysics and Geophysics. 3, Gordon and Breach.