Generation of coherent magnetic fields in sheared inhomogeneous turbulence: No need for rotation?

Nicolas Leprovost, Eun Jin Kim

Research output: Contribution to journalArticle

Abstract

Coherent magnetic fields are often believed to be generated by the combination of stretching by differential rotation and turbulent amplification of magnetic field, via the so-called α effect. The latter is known to exist in helical turbulence, which is envisioned to arise due to both rotation and convection in solar-type stars. In this contribution, a turbulent flow driven by a nonhelical inhomogeneous forcing and its kinematic dynamo action are studied for a uniform magnetic field in the background of a linear shear flow. By using a quasilinear analysis and a nonperturbative method utilizing a time-dependent wave number, turbulence property and electromotive force are computed for arbitrary shear strength. Due to the large-scale shear flow, the turbulence is highly anisotropic, as a consequence, so is the electromotive force. The latter is found to exist even without rotation due to the combined effect of shear flow and inhomogeneous forcing, containing not only the α effect but also magnetic pumping (the γ effect representing a transport of magnetic flux by turbulence). Specifically, without shear, only the magnetic pumping exists, aligned with the direction of inhomogeneity. For a weak but nonzero shear, the combined effects of shear and inhomogeneous forcing modify the structure of the magnetic pumping when the inhomogeneity is in the plane of the shear flow, the magnetic pumping becoming bidimensional in that plane. It also induces an α tensor which has nondiagonal components. When the inhomogeneity is perpendicular to the plane of the shear flow, the α effect has three nonzero diagonal components and one off-diagonal component. However, for a sufficiently strong shear, the γ and α effects are suppressed due to shear stabilization which damps turbulence. A simplified dynamo model is then proposed where a large-scale dynamo arises due to the combined effect of shear flow and inhomogeneous forcing. In particular, the growth of a large-scale axisymmetric magnetic field is demonstrated in case of an inhomogeneity which is perpendicular to the plane of the shear flow. Interesting implications of these results for the structure of magnetic fields in star with slow rotation are discussed.

Original languageEnglish
Article number022307
JournalPhysics of Plasmas
Volume18
Issue number2
DOIs
Publication statusPublished - 9 Feb 2011
Externally publishedYes

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shear flow
magnetic pumping
turbulence
magnetic fields
shear
inhomogeneity
electromotive forces
stars
shear strength
turbulent flow
magnetic flux
convection
kinematics
stabilization
tensors

ASJC Scopus subject areas

  • Condensed Matter Physics

Cite this

Generation of coherent magnetic fields in sheared inhomogeneous turbulence : No need for rotation? / Leprovost, Nicolas; Kim, Eun Jin.

In: Physics of Plasmas, Vol. 18, No. 2, 022307, 09.02.2011.

Research output: Contribution to journalArticle

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