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arXiv · astro-ph/0309666

Non-local effects in the mean-field disc dynamo. I. An asymptotic expansion

Abstract

We reconsider thin-disc global asymptotics for kinematic, axisymmetric mean-field dynamos with vacuum boundary conditions. Non-local terms arising from a small but finite radial field component at the disc surface are consistently taken into account for quadrupole modes. As in earlier approaches, the solution splits into a local part describing the field distribution along the vertical direction and a radial part describing the radial (global) variation of the eigenfunction. However, the radial part of the eigenfunction is now governed by an integro-differential equation whose kernel has a weak (logarithmic) singularity. The integral term arises from non-local interactions of magnetic fields at different radii through vacuum outside the disc. The non-local interaction can have a stronger effect on the solution than the local radial diffusion in a thin disc, however the effect of the integral term is still qualitatively similar to magnetic diffusion.

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BibTeXRIS

Vladimir Priklonsky, Anvar Shukurov, Dmitry Sokoloff, Andrew Soward. 2003-09-24. Non-local effects in the mean-field disc dynamo. I. An asymptotic expansion. https://doi.org/10.1080/03091920008203723

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