Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-30T05:27:23.217Z Has data issue: false hasContentIssue false
  • English
  • Français

Topological Magnetic Flux Pumping Revisited

Published online by Cambridge University Press:  04 August 2017

Wayne Arter
Wayne Arter*
Affiliation:
Department of Applied Mathematics and Theoretical Physics, Silver Street, Cambridge CB3 9EW, England

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.

Calculations by Drobyshevski and Yuferev (1974) suggest that magnetic flux is ‘topologically pumped’ to the bottom of a convecting Benard layer as the electrical conductivity is increased. This is shown to be mistaken: however, compressible flows where motion is mainly around fieldlines can confine flux near their base.

Type
III. Theory of Stellar Magnetic Field Generation
Information
Symposium - International Astronomical Union , Volume 102: Solar and Stellar Magnetic Fields: Origins and Coronal Effects , 1983 , pp. 243 - 246
Copyright
Copyright © Reidel 1983 

References

Arter, W.: 1983, in preparation.Google Scholar
Arter, W., Galloway, D.J. and Proctor, M.R.E.: 1982, submitted to Mon. Not. R. astr. Soc. Google Scholar
Drobyshevski, E.M., Kolesnikova, E.N. and Yuferev, V.S.: 1980, J. Fluid Mech. 101, p. 65–78.CrossRefGoogle Scholar
Drobyshevski, E.M. and Yuferev, V.S.: 1974, J. Fluid Mech. 65, p. 33–44.CrossRefGoogle Scholar
Galloway, D.J. and Proctor, M.R.E.: 1983, in preparation.Google Scholar
Parker, E.N.: 1975, Astrophys. J., 202, pp. 523–527.CrossRefGoogle Scholar
Proctor, M.R.E. and Weiss, N.O.: 1982, Rep. Prog. Phys., in press.Google Scholar
Roberts, K.V. and Weiss, N.O.: 1966, Math. Comp. 20, p. 272–299.CrossRefGoogle Scholar