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Numerical study of 3D Rayleigh-Taylor turbulence

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The Nature of High Reynolds Number Turbulence

The Rayleigh-Taylor turbulence in 3D space is numerically studied via the Boussinesq approximation along the same line as the 2D numerical study by Celani et al. (2006 Phys.Rev.Lett. 96 134504). A comparison with the phenomenology proposed by Chertkov (2003 Phys.Rev.Lett. 91 115001), in particular deviation from the phenomenology (intermittency), will be presented.

This talk is part of the Isaac Newton Institute Seminar Series series.

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