Shear dynamo problem: Quasilinear kinematic theory

Details Shear dynamo problem: Quasilinear kinematic theory Shear dynamo problem: Quasilinear kinematic theory

2008-12-17

arxiv.org/abs/0812.3269v2

Astronomy and Astrophysics

Astrophysics

4 pages; to appear in Physical Review E (Rapid Communication)

Scientific paper

Large-scale dynamo action due to turbulence in the presence of a linear shear flow is studied. Our treatment is quasilinear and kinematic but is non perturbative in the shear strength. We derive the integro-differential equation for the evolution of the mean magnetic field, by systematic use of the shearing coordinate transformation and the Galilean invariance of the linear shear flow. For non helical turbulence the time evolution of the cross-shear components of the mean field do not depend on any other components excepting themselves. This is valid for any Galilean-invariant velocity field, independent of its dynamics. Hence the shear-current assisted dynamo is essentially absent, although large-scale non helical dynamo action is not ruled out.

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