We report the first direct experimental observation of the ablative RichtmyerMeshkov instability. It manifests itself in oscillations of areal mass that occur during the shock transit time, which are caused by the rocket effect or dynamic overpressure characteristic of interaction between the laser absorption zone and the ablation front.With the 4 ns long Nike KrF laser pulse and our novel diagnostic technique (monochromatic x-ray imaging coupled to a streak camera) we were able to register a peak and a valley of the areal mass variation before the observed onset of the RayleighTaylor growth.PACS numbers: 52.57. Fg, 52.70.La,
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ABSTRACTWe report the first direct experimental observation of the ablative Richtmyer-Meshkov instability. It manifests itself in oscillations of areal mass that occur during the shock transit time, which are caused by the rocket effect or dynamic overpressure characteristic of interaction between the laser absorption zone and the ablation front. With the 4 ns long Nike KrF laser pulse and our novel diagnostic technique (monochromatic x-ray imaging coupled to a streak camera) we were able to register a peak and a valley of the areal mass variation before the observed onset of the Rayleigh-Taylor growth. Most of our knowledge in this field still comes from simulations and theory. The seed amplitudes are known to form during the early-time period that includes a shock wave transit from the front to the rear surface of the target, and a rarefaction wave transit in the opposite direction. During this time interval, the areal mass perturbations caused by all sources of non-uniformity are expected to oscillate [4][5][6][7][8][9]. The physical mechanisms driving the oscillations depend on whether the perturbations are initially at the front surface of the target (laser imprint, front surface roughness) or at its rear surface (feedout, see [9]). Here, we limit ourselves to the former case, where the oscillations are caused by the rocket effect, or the dynamic overpressure [6,8,10,11]. The oscillatory behavior is consistent with the expression for the growth rate Γ of ablative RT instability, which has recently been established [10,11] for the case of large Froude number (low acceleration): perturbed, and a part of it gets closer to the hot laser absorption zone, the temperature at the ablation front does not increase, but the temperature gradient in its vicinity, T ∇ , does. This, in turn, increases the local heat flux to the ablation front, T ∇ − κ , hence, the rate of mass ablation from it, thereby increasing the ablative pressure and pushing this part of the ablation front back. The physics of this rocket effect is explained in detail inRefs. 6,8,10. The rocket effect rat...