Abstract
In the context of the classical Rayleigh-Taylor hydrodynamical instability, we examine the much debated question of models for initial conditions and the possible influence of unrecorded long wave length contributions to the instability growth rate α. © T. Kaman, J. Glimm, D.H. Sharp.
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APA
Kaman, T., Glimm, J., & Sharp, D. H. (2010). Initial conditions for turbulent mixing simulations. Condensed Matter Physics, 13(4). https://doi.org/10.5488/CMP.13.43401
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