The role of initial conditions in affecting the evolution toward self-similarity of an axisymmetric turbulent jet is examined. The jet’s near-field coherence was manipulated by non-circular exit geometries of identical open area, , including a square and a fractal exit, for comparison with a classical round orifice jet. Hot-wire anemometry and 2D-planar particle image velocimetry experiments were performed between the exit and a location 26De downstream, where the Reynolds stress profiles are self-similar. This study shows that a fractal geometry significantly changes the near-field structure of the jet, breaking up the large-scale coherent structures, thereby affecting the entrainment rate of the background fluid into the jet stream. It is found that many of the jet’s turbulent characteristics scale with the number of eddy turnover times rather than simply the streamwise coordinate, with the entrainment rate (amongst others) found to be comparable across the different jets after approximately 3-4 eddies have been overturned. The study is concluded by investigating the jet’s evolution toward a self-similar state. No differences are found for the large-scale spreading rate of the jets in the weakly self-similar region, so defined as the region for which some, but not all of the terms of the mean turbulent kinetic energy equation are self-similar. However, the dissipation rate of the turbulent kinetic energy was found to vary more gradually in x than predicted according to the classical equilibrium theories of Kolmogorov. Instead, the dissipation was found to vary in a non-equilibrium fashion for all three jets tested.
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March 2018
Research Article|
March 29 2018
Influence of coherent structures on the evolution of an axisymmetric turbulent jet
Massimiliano Breda
;
Massimiliano Breda
Department of Aeronautics, Imperial College London, South Kensington Campus
, London SW7 2AZ, United Kingdom
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Oliver R. H. Buxton
Oliver R. H. Buxton
a)
Department of Aeronautics, Imperial College London, South Kensington Campus
, London SW7 2AZ, United Kingdom
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a)
Electronic mail: o.buxton@imperial.ac.uk
Physics of Fluids 30, 035109 (2018)
Article history
Received:
December 15 2017
Accepted:
March 02 2018
Citation
Massimiliano Breda, Oliver R. H. Buxton; Influence of coherent structures on the evolution of an axisymmetric turbulent jet. Physics of Fluids 1 March 2018; 30 (3): 035109. https://doi.org/10.1063/1.5019668
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