Measurements of scalar power spectra in high Schmidt number turbulent jets
نویسندگان
چکیده
منابع مشابه
Reynolds number dependence of scalar fluctuations in a high Schmidt number turbulent jet
The scalar rms fluctuations in a turbulent jet were investigated experimentally, using highresolution, laser-induced fluorescence techniques. The experiments were conducted in a high Schmidt nuinber fluid (water), on the jet centerline, over a jet Reynolds number range of 3000<Re<24 000. It was found that the normalized scalar rms fluctuations c’/ C decrease with increasing flow Reynolds number...
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Jörg Schumacher Fachbereich Physik, Philipps-Universität Marburg, D-35032 Marburg, Germany Herwig Zilken Visualization Laboratory, Zentralinstitut für angewandte Mathematik, Forschungszentrum Jülich, D-52425 Jülich, Germany Bruno Eckhardt Fachbereich Physik, Philipps-Universität Marburg, D-35032 Marburg, Germany Katepalli R. Sreenivasan International Centre for Theoretical Physics, 34014 Triest...
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The mixing of substances is present in various turbulent systems. Examples arise in reacting flows and combustion, mixing of salt and plankton in oceans and of chemical pollutants in the stratosphere [1]. The physics of scalar mixing depends strongly on the ratio of the kinematic viscosity ν of the fluid to the diffusivity κ of the scalar. It is given by the Schmidt number Sc = ν/κ. For the fol...
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We present results from an experimental investigation of turbulent transport and molecular mixing of a Sc S 1 conserved scalar in the fully developed self-similar far field of a steady, axisymmetric, momentum-driven, free turbulent jet issuing into a quiescent medium. Our experiments cover the axial range from the jet exit to 350 diameters downstream, and span the range of Reynolds numbers from...
متن کاملParticle method: an efficient tool for direct numerical simulations of a high Schmidt number passive scalar in turbulent flow
In this work, an efficient way to predict the dynamics of a scalar at high Schmidt numbers, advected by a turbulent flow, is presented. For high Schmidt numbers, the spatial resolution required for the scalar field has to be finer than the resolution required for the velocity field, leading to a significant computational cost due to the CourantFriedrichsLewy (CFL) constraint. We propose here a ...
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ژورنال
عنوان ژورنال: Journal of Fluid Mechanics
سال: 1996
ISSN: 0022-1120,1469-7645
DOI: 10.1017/s0022112096001425