Moffatt drift driven large scale dynamo due to fluctuations with nonzero correlation times
arXiv:1506.00867 · doi:10.1017/jfm.2016.284
Abstract
We present a theory of large-scale dynamo action in a turbulent flow that has stochastic, zero-mean fluctuations of the parameter. Particularly interesting is the possibility of the growth of the mean magnetic field due to Moffatt drift, which is expected to be finite in a statistically anisotropic turbulence. We extend the Kraichnan-Moffatt model to explore effects of finite memory of fluctuations, in a spirit similar to that of Sridhar & Singh (2014), hereafter SS14. Using the first-order smoothing approximation, we derive a linear integro-differential equation governing the dynamics of the large-scale magnetic field, which is non-perturbative in the -correlation time . We recover earlier results in the exactly solvable white-noise (WN) limit where the Moffatt drift does not contribute to the dynamo growth/decay. To study finite memory effects, we reduce the integro-differential equation to a partial differential equation by assuming that the be small but nonzero and the large-scale magnetic field is slowly varying. We derive the dispersion relation and provide explicit expression for the growth rate as a function of four independent parameters. When , we find that: (i) in the absence of the Moffatt drift, but with finite Kraichnan diffusivity, only strong -fluctuations can enable a mean-field dynamo; (ii) in the general case when also the Moffatt drift is nonzero, both, weak or strong fluctuations, can lead to a large-scale dynamo; and (iii) there always exists a wavenumber () cutoff at some large beyond which the growth rate turns negative. Thus we show that a finite Moffatt drift can always facilitate large-scale dynamo action if sufficiently strong, even in case of weak fluctuations, and the maximum growth occurs at intermediate wavenumbers.
20 pages, 4 figures, submitted to the Journal of Fluid Mechanics
References in corpus (9)
- Generation of Magnetic Field by Combined Action of Turbulence and Shear
- Fluctuation dynamos and their Faraday rotation signatures
- Effects of fluctuation on alpha-omega dynamo models
- Memory effects in turbulent transport
- Non-linear galactic dynamos: A toolbox
- Mean-field dynamo in a turbulence with shear and kinetic helicity fluctuations
- Galactic dynamo action in presence of stochastic alpha and shear
- Coherent nonhelical shear dynamos driven by magnetic fluctuations at low Reynolds numbers
- Nonhelical mean-field dynamos in a sheared turbulence
Cited by in corpus (6)
- The supernova-regulated ISM. III. Generation of vorticity, helicity and mean flows
- Non-linear Galactic Dynamos and the Magnetic Rädler Effect
- On the shear-current effect: toward understanding why theories and simulations have mutually and separately conflicted
- Mean field dynamo action in shearing flows. II: fluctuating kinetic helicity with zero mean
- Generation of large-scale magnetic fields due to fluctuating in shearing systems
- Mean-field dynamo due to spatiotemporal fluctuations of the turbulent kinetic energy