On the fine-scale structure of vector fields convected by a turbulent fluid

DOI10.1017/S0022112063000987zbMath0126.22204OpenAlexW2108984213MaRDI QIDQ5333219

Philip G. Saffman

Publication date: 1963

Published in: Journal of Fluid Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1017/s0022112063000987

zbMATH Keywords

fluid mechanics

Related Items (14)

Spectral properties of exact random solutions to Burgers' equation for modified Thomas initial conditions ⋮ Towards the Applicability of the Modified von Kármán Spectrum to Predict Trailing Edge Noise ⋮ Effects of turbulence structure, molecular diffusion and source size on scalar fluctuations in homogeneous turbulence ⋮ Nonlocal triad interactions and the dissipation range of isotropic turbulence ⋮ Dynamo action in complex flows: the quick and the fast ⋮ Small-scale kinematic dynamo and non-dynamo in inertial-range turbulence ⋮ The Lagrangian spectral relaxation model for differential diffusion in homogeneous turbulence ⋮ High Schmidt number scalars in turbulence: Structure functions and Lagrangian theory ⋮ The viscous-convective subrange in nonstationary turbulence ⋮ A note on the vorticity spectrum ⋮ Analysis of scalar dissipation in terms of vorticity geometry in isotropic turbulence ⋮ Some topological aspects of fluid dynamics ⋮ Kinematic dynamo problem in a linear velocity field ⋮ Exact solutions for the probability density function of turbulent scalar fields

Cites Work

• Cosmic Radiation and Cosmic Magnetic Fields. II. Origin of Cosmic Magnetic Fields

This page was built for publication: On the fine-scale structure of vector fields convected by a turbulent fluid