Abstract
We conduct experiments to investigate the rotations of freely moving particles in a homogeneous isotropic turbulent flow. The particles are nearly neutrally buoyant and the particle size exceeds the Kolmogorov scale so that they are too large to be considered passive tracers. Particles of several different shapes are considered including those that break axisymmetry and fore-aft symmetry. We find that regardless of shape the mean-square particle angular velocity scales as , where is the equivalent diameter of a volume-matched sphere. This scaling behavior is consistent with the notion that velocity differences across a length in the flow are responsible for particle rotation. We also find that the probability density functions (PDFs) of particle angular velocity collapse for particles of different shapes and similar . The significance of these results is that the rotations of an inertial, nonspherical particle are only functions of its volume and not its shape. The magnitude of particle angular velocity appears log-normally distributed and individual Cartesian components show long tails. With increasing , the tails of the PDF become less pronounced, meaning that extreme events of angular velocity become less common for larger particles.
- Received 8 March 2018
DOI:https://doi.org/10.1103/PhysRevFluids.3.054605
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