Rayleigh Taylor instability



disk A case with strong interface deformation is investigated. It is described by the unstable situation of a heavy fluid resting upon a lighter one in a gravitational field. The density ratio of the fluids is 0.1383 and their viscosities are equal. This case is two-dimensional and no surface tension acts on the interface. A rectangular domain of dimensions 1x4 was used. The interface is initialized with a sinusoidal perturbation of amplitude A=0.05. Symmetry boundary conditions were used on all domain boundaries. The non-dimensional numbers are Re = 391.37 and Fr = 0.31928. The same conditions were simulated by Lopez et al. (2005) using an interface capturing method and by Popinet and Zaleski (1999) using a front tracking algorithm. The present results for the shape of the interface are displayed in fig. (3). The instability develops a typical mushroom shape. At larger times, thin filaments are generated which are clearly resolved by the mesh.