Phys. Fluids B 2, 2001 (1990)https://ireap.umd.edu/10.1063/1.8594211990
Adil
Hassam
J.D.
Huba
Journal ArticlePlasma, Accelerator, and Nuclear PhysicsThe nonlinear evolution of the unmagnetized ion Rayleigh–Taylor instability is investigated. A nonlinear state corresponding to localized clumps of high‐density plasma is obtained analytically. The characteristic scale size of the clumps is given by Δ∼D(gLn)−1/2, where g is the gravitational acceleration, Ln is the density gradient scale length, and D is a diffusion coefficient associated with the short‐scale dissipation processes in the system. It is shown numerically that this nonlinear state may be both accessible and stable.
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