Published online by Cambridge University Press: 17 February 2011
Through a comparison between experiments and numerical simulations, we have examined the dynamics of a cloud of spheres at a small but finite Reynolds number. The cloud is seen to flatten and to transition into a torus, which further widens and eventually breaks up into droplets. While this behaviour bears some similarity to that observed at zero inertia, the underlying physical mechanisms differ. Moreover, the evolution of the cloud deformation is accelerated as inertia is increased. Two inertial regimes in which macro-scale inertia and micro-scale inertia become successively dominant are clearly identified.
Movie 1. Typical evolution of a cloud in the macro-scale inertia regime: experiment with a cloud Reynolds number of 0.7, an initial number of particles of 16000, an inertial length normalised by the initial radius of the cloud of 179 (a particle Reynolds number of 0.00008, a ratio of cloud to particle radius of 66, a volume fraction of 6 %, and a particle Stokes number of 0.00002)
Movie 1. Typical evolution of a cloud in the macro-scale inertia regime: experiment with a cloud Reynolds number of 0.7, an initial number of particles of 16000, an inertial length normalised by the initial radius of the cloud of 179 (a particle Reynolds number of 0.00008, a ratio of cloud to particle radius of 66, a volume fraction of 6 %, and a particle Stokes number of 0.00002)
Movie 2. Typical evolution of the cloud in the micro-scale inertia regime: experiment with a cloud Reynolds number of 15, an initial number of particles of 600, an inertial length normalised by the initial radius of the cloud of 0.65 (a particle Reynolds number of 0.14, an ratio of cloud to particle radius of 11, a volume fraction of 50 %, and a particle Stokes number of 0.077)
Movie 2. Typical evolution of the cloud in the micro-scale inertia regime: experiment with a cloud Reynolds number of 15, an initial number of particles of 600, an inertial length normalised by the initial radius of the cloud of 0.65 (a particle Reynolds number of 0.14, an ratio of cloud to particle radius of 11, a volume fraction of 50 %, and a particle Stokes number of 0.077)
Movie 3. Typical evolution of the cloud in the micro-scale inertia regime: experiment with a cloud Reynolds number of 3.5, an initial number of particles of 7000, an inertial length normalised by the initial radius of the cloud of 21 (a particle Reynolds number of 0.002, an ratio of cloud to particle radius of 24, a volume fraction of 50 %, and a particle Stokes number of 0.0005)
Movie 3. Typical evolution of the cloud in the micro-scale inertia regime: experiment with a cloud Reynolds number of 3.5, an initial number of particles of 7000, an inertial length normalised by the initial radius of the cloud of 21 (a particle Reynolds number of 0.002, an ratio of cloud to particle radius of 24, a volume fraction of 50 %, and a particle Stokes number of 0.0005)
Movie 4. Flow field at succesive times in the vertical plane through the vertical axis of symmetry in the cloud reference frame. Oseenlet simulation with an initial number of particles of 2000 and an inertial length normalised by the initial radius of the cloud of 1. High (low) velocity is indicated in white (dark).
Movie 4. Flow field at succesive times in the vertical plane through the vertical axis of symmetry in the cloud reference frame. Oseenlet simulation with an initial number of particles of 2000 and an inertial length normalised by the initial radius of the cloud of 1. High (low) velocity is indicated in white (dark).