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Nonlinear saturation of Rayleigh-Taylor instability and generation of shear flow in equatorial spread-F plasma

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Figure

Fig. 1. growth rate for the secondary instability against ky, for kx =1.0, νin = 0.3, D = 0.2, which indicates that secondary modegrows in the short scale regime.
Fig. 3. Temporal evolution of the anti-symmetric shear flow am-plitude for kx = 0.4, ky = 1.4, νin = 0.24 and D = 0.2, whichindicates that the initial seed flow has transient growth and then os-cillatory decay due to finite dissipation present in the system.
Fig. 4. Temporal evolution of the symmetric shear flow amplitudefor kx = 0.4, ky = 1.4, νin = 0.24 and D = 0.2, which indicatesthat the initial seed flow does not have significant growth.

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