Skip to main content
Log in

Methods of Calculation of Turbulent Diffusivities

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

Different techniques of calculation and estimation of turbulentdiffusivities D\(^{^{\mathcal{D}_\mathcal{T} } } \) of passive fields in infinite incompressiblemedia showing isotropic, homogeneous and stationary turbulence areconsidered. The numerical comparison of the methods is made mostlyfor two representative limiting models of turbulence – withpeak-like spectrum and for vast Kolmogorov's type spectrum. The timedependence of two-point velocity correlators is assumed to beexponential. The backbone of the comparison is steady-state turbulentdiffusivities calculated in nonlinear DIA-approach with thecorrections due to contribution of four-order velocity correlators.As a result of this comparison the most satisfactory approximatemethods are proposed both for steady-state and time-dependentturbulent diffusivities. The results may be used for the most correctchoice of \(^{^{\mathcal{D}_\mathcal{T} } } \)-dependence in various astrophysical problems.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Bradshaw, P. (ed.): 1978, Turbulence, Springer Verlag, Berlin.

    Google Scholar 

  • Dolginov, A.Z. and Silant'ev, N.A.: 1992, Geophys. Astrophys. Fluid Dyn. 63, 139.

    Google Scholar 

  • Kraichnan, R.H.: 1959, J. Fluid Mech. 5, 497.

    Google Scholar 

  • Kraichnan, R.H.: 1970, Physics of Fluids 13, 22.

    Google Scholar 

  • Kraichnan, R.H.: 1976, J. Fluid Mech. 77, 753.

    Google Scholar 

  • Kraichnan, R.H.: 1977, J. Fluid Mech. 81, 385.

    Google Scholar 

  • Krause, F. and Raedler, K.-H.: 1980, Mean-field Magnetohydrodynamics and Dynamo Theory, Pergamon Press, Oxford.

    Google Scholar 

  • Parker, E.N.: 1979, Cosmical Magnetic Fields, Clarendon Press, Oxford.

    Google Scholar 

  • Phythian, R. and Curtis, W.D.: 1978, J. Fluid Mech. 89, 241.

    Google Scholar 

  • Roberts, P.H.: 1961, J. Fluid Mech. 11, 257.

    Google Scholar 

  • Silant'ev, N.A.: 1992, JETP (Soviet Physics) 74, 650.

    Google Scholar 

  • Silant'ev, N.A.: 1994, Geophys. Astrophys. Fluid Dyn. 75, 183.

    Google Scholar 

  • Tatarskii, V.I.: 1967, The Propagation of Waves in Turbulent Atmospheres, Nauka, Moscow (in russian).

    Google Scholar 

  • Taylor, G.I.: 1921, Proc. Lond. Math. Soc. 20, 196.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Silant'ev, N. Methods of Calculation of Turbulent Diffusivities. Astrophysics and Space Science 249, 95–109 (1997). https://doi.org/10.1023/A:1000328407621

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1023/A:1000328407621

Keywords

Navigation