Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-24T15:42:07.332Z Has data issue: false hasContentIssue false

On the measurement of turbulent magnetic diffusivities: the three-dimensional case

Published online by Cambridge University Press:  24 October 2013

F. Cattaneo
Affiliation:
Department of Astronomy and Astrophysics and The Computation Institute, University of Chicago, Chicago, IL 60637, USA
S. M. Tobias*
Affiliation:
Department of Applied Mathematics, University of Leeds, Leeds LS2 9JT, UK
*
Email address for correspondence: [email protected]

Abstract

It has been shown that it is possible to measure the turbulent diffusivity of a magnetic field by a method involving oscillatory sources. So far the method has only been tried in the special case of two-dimensional fields and flows. Here we extend the method to three dimensions and consider the case where the flow is thermally driven convection in a large-aspect-ratio domain. We demonstrate that if the diffusing field is horizontal the method is successful even if the underlying flow can sustain dynamo action. We show that the resulting turbulent diffusivity is comparable with, although not exactly the same as, that of a passive scalar. We were not able to measure unambiguously the diffusivity if the diffusing field is vertical, but argue that such a measurement is possible if enough resources are utilized on the problem.

Type
Papers
Copyright
©2013 Cambridge University Press 

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Ångström, Å, J. 1861 Neue methode, das wärmeleitungsvermögen der körper zu bestimmen. Ann. Phys. Chem. 114, 513530.Google Scholar
Canuto, C., Hussaini, M. Y., Quarteroni, A. & Zang, T. A. 1987 Spectral Methods in Fluid Dynamics. Springer.Google Scholar
Cattaneo, F. 1999 On the origin of magnetic fields in the quiet photosphere. Astrophys. J. Lett. 515, L39L42.Google Scholar
Cattaneo, F., Emonet, T. & Weiss, N. 2003 On the interaction between convection and magnetic fields. Astrophys. J. 588, 11831198.Google Scholar
Cattaneo, F. & Hughes, D. W. 2006 Dynamo action in a rotating convective layer. J. Fluid Mech. 553, 401418.Google Scholar
Cattaneo, F., Lenz, D. & Weiss, N. 2001 On the origin of the solar mesogranulation. Astrophys. J. Lett. 563, L91L94.Google Scholar
Cattaneo, F. & Vainshtein, S. I. 1991 Suppression of turbulent transport by a weak magnetic field. Astrophys. J. Lett. 376, L21L24.Google Scholar
Chandrasekhar, S. 1961 Hydrodynamic and Hydromagnetic Stability. Oxford (Clarendon).Google Scholar
Garabedian, P. R. 1998 Partial Differential Equations. AMS Chelsea Publishing.Google Scholar
Krause, F. & Raedler, K.-H. 1980 Mean-field Magnetohydrodynamics and Dynamo Theory. Pergamon.Google Scholar
Meneguzzi, M. & Pouquet, A. 1989 Turbulent dynamos driven by convection. J. Fluid Mech. 205, 297318.Google Scholar
Moffatt, H. K. 1974 The mean electromotive force generated by turbulence in the limit of perfect conductivity. J. Fluid Mech. 65, 110.Google Scholar
Moffatt, H. K. 1978 Magnetic Field Generation in Electrically Conducting Fluids. Cambridge University Press.Google Scholar
Ogilvie, G. I. & Lesur, G. 2012 On the interaction between tides and convection. Mon. Not. R. Astron. Soc. 422, 19751987.Google Scholar
Parker, E. N. 1979 Cosmical Magnetic Fields: Their Origin and Their Activity. Clarendon (Oxford University Press).Google Scholar
Rieutord, M. & Rincon, F. 2010 The Sun’s supergranulation. Living Rev. Solar Phys. 7, 2.CrossRefGoogle Scholar
Schrinner, M., Rädler, K.-H., Schmitt, D., Rheinhardt, M. & Christensen, U. 2005 Mean-field view on rotating magnetoconvection and a geodynamo model. Astron. Nachr. 326, 245249.Google Scholar
Tobias, S. M. & Cattaneo, F. 2013 On the measurement of the turbulent diffusivity of a large-scale magnetic field. J. Fluid Mech. 717, 347360.Google Scholar
Tobias, S. M., Cattaneo, F. & Brummell, N. H. 2008 Convective dynamos with penetration, rotation, and shear. Astrophys. J. 685, 596605.Google Scholar
Tobias, S. M., Cattaneo, F. & Brummell, N. H. 2011 On the generation of organized magnetic fields. Astrophys. J. 728, 153.Google Scholar