arXiv Analytics

Sign in

arXiv:astro-ph/0012472AbstractReferencesReviewsResources

Large scale dynamos with helicity loss through boundaries

Axel Brandenburg, Wolfgang Dobler

Published 2000-12-22, updated 2001-01-29Version 2

Dynamo action is investigated in simulations of locally isotropic and homogeneous turbulence in a slab between open boundaries. It is found that a `pseudo-vacuum' boundary condition (where the field is vertical) leads to strong helicity fluxes which significantly reduce the amplitude of the resulting large scale field. On the other hand, if there is a conducting halo outside the dynamo-active region the large scale field amplitude can reach larger values, but the time scale after which this field is reached increases linearly with the magnetic Reynolds number. In both cases most of the helicity flux is found to occur on large scales. From the variety of models considered we conclude that open boundaries tend to lower the saturation field strength compared to the case with periodic boundaries. The rate at which this lower saturation field strength is attained is roughly independent of the strength of the turbulence and of the boundary conditions. For dynamos with less helicity, however, significant field strengths could be reached in a shorter time.

Comments: 9 pages, 10 figures, A&A (accepted)
Journal: Astron.Astrophys. 369 (2001) 329-338
Categories: astro-ph
Related articles: Most relevant | Search more
arXiv:astro-ph/0012053 (Published 2000-12-03)
Synthesis of Small and Large scale Dynamos
arXiv:astro-ph/0207394 (Published 2002-07-18)
The helicity issue in large scale dynamos
arXiv:astro-ph/0204497 (Published 2002-04-29, updated 2002-07-02)
Dynamic nonlinearity in large scale dynamos with shear