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The relative diffusion of a cloud of passive contaminant in incompressible turbulent flow

Published online by Cambridge University Press:  19 April 2006

P. C. Chatwin
Affiliation:
Department of Applied Mathematics and Theoretical Physics, University of Liverpool
Paul J. Sullivan
Affiliation:
Department of Applied Mathematics and Theoretical Physics, University of Liverpool Permanent address: Department of Applied Mathematics, University of Western Ontario, London, Canada.

Abstract

A problem of major practical interest is the variation with x and t of the statistical properties of Γ(x, t), the distribution of concentration of a contaminant in a cloud containing a finite quantity Q of contaminant, released in a specified way at t = 0 over a volume of order L30. Of particular relevance is the case of relative diffusion (when x is measured throughout each realization relative to the centre of mass of the cloud), when important properties are L(t), the linear dimension of the cloud, C(x, t), the ensemble mean concentration, $\overline{c^2}({\bf x}, t)$, the variance of the concentration, and p(y, t), the distance-neighbour function. Much fundamental work has led to a knowledge of the way L varies with t, but not of the way the other properties vary. Hitherto therefore, prediction of such variation has normally used unjustifiable empirical concepts such as eddy diffusivities, but this is ultimately unsatisfactory, practically as well as theoretically. Hence the exact equations have been used to obtain a quite new description of the structure of a dispersing cloud, which it is hoped will serve as a basis for future practical work.

When κ = 0 (where κ is the molecular diffusivity) the magnitude of p(y, t) is of order Q/L3 for most y, but of order Q/L30 when |y| is very small. By a variety of arguments it is shown that these facts can be explained (for many, if not all, flows) only if the distributions of C and $\overline{c^2}$, as well as that of p, have a core-bulk structure. In the bulk of the cloud C and $\overline{c^2}$ have magnitudes of order Q/L3 and Q2/L30L3 respectively, but there is a core region of thickness decreasing to zero surrounding the centre of mass within which they have much greater magnitudes. In one case, examined in some detail, the magnitudes in the core are of order Q/L30 and Q2/L60.

It is then shown that the core and bulk exist even in the real case when κ ≠ 0. In the real case the core thickness no longer tends to zero but to a constant of order λc, the conduction cut-off length. As a consequence almost entirely of molecular diffusion acting in the core region, the magnitudes of C and $\overline{c^2}$ in both the core and the bulk decay to zero in a way which depends on the details of the fine-scale structure of the velocity field. Several examples of the decay are discussed.

Type
Research Article
Copyright
© 1979 Cambridge University Press

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References

Batchelor, G. K. 1952a Diffusion in a field of homogeneous turbulence. II. The relative motion of particles. Proc. Camb. Phil. Soc. 48, 345.Google Scholar
Batchelor, G. K. 1952b The effect of homogeneous turbulence on material lines and surfaces. Proc. Roy. Soc. A 213, 349.Google Scholar
Batchelor, G. K. 1959 Small-scale variations of convected quantities like temperature in turbulent fluid. Part I. General discussion and the case of small conductivity. J. Fluid Mech. 5, 113.Google Scholar
Csanady, G. T. 1967 Concentration fluctuations in turbulent diffusion. J. Atm. Sci. 24, 21.Google Scholar
Csanady, G. T. 1973 Turbulent Diffusion in the Environment. Dordrecht: Reidel.
Gibson, C. H. & Schwarz, W. H. 1963 The universal equilibrium spectra of turbulent velocity and scalar fields. J. Fluid Mech. 16, 365.Google Scholar
Kraichnan, R. H. 1974 Convection of a passive scalar by a quasi-uniform random straining field. J. Fluid Mech. 64, 737.Google Scholar
Lumley, J. L. 1964 The mathematical nature of the problem of relating Lagrangian and Eulerian statistical functions in turbulence. In The Mechanics of Turbulence. Gordon & Breach.
Monin, A. S. & Yaglom, A. M. 1975 Statistical Fluid Mechanics: Mechanics of Turbulence. Vol. 2 (ed. J. L. Lumley). M.I.T. Press.
Richardson, L. F. 1926 Atmospheric diffusion shown on a distance-neighbour graph. Proc. Roy. Soc. A 110, 709.Google Scholar
Saffman, P. G. 1963 On the fine-scale structure of vector fields convected by a turbulent fluid. J. Fluid Mech. 16, 545.Google Scholar
Sullivan, P. J. 1971 Some data on the distance-neighbour function for relative diffusion. J. Fluid Mech. 47, 601.Google Scholar
Townsend, A. A. 1951 The diffusion of heat spots in isotropic turbulence. Proc. Roy. Soc. A 209, 418.Google Scholar