2012Chinese Physics BOpen access

Directly driven Rayleigh—Taylor instability of modulated CH targets

Guo Jia, Jun Xiong, Dong Jia-Qin, Zhiyong Xie, Jiang Wu

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Abstract

Directly driven ablative Rayleigh—Taylor (R—T) instability of modulated CH targets was studied using the face-on X-ray radiography on the Shen-Guang II device. We obtained temporal evolution images of the R—T instability perturbation. The R—T instability growth factor has been obtained by using the methods of fast Fourier transform and seeking the difference of light intensity between the peak and the valley of the targets. Through comparison with the the theoretical simulation, we found that the experimental data had a good agreement with the theoretical simulation results before 1.8 ns, and was lower than the theoretical simulation results after that.

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Directly driven ablative Rayleigh—Taylor (R—T) instability of modulated CH targets was studied using the face-on X-ray radiography on the Shen-Guang II device. We obtained temporal evolution images of the R—T instability perturbation. The R—T instability growth factor has been obtained by using the methods of fast Fourier transform and seeking the difference of light intensity between the peak and the valley of the targets. Through comparison with the the theoretical simulation, we found that the experimental data had a good agreement with the theoretical simulation results before 1.8 ns, and was lower than the theoretical simulation results after that.

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Available abstract

Directly driven ablative Rayleigh—Taylor (R—T) instability of modulated CH targets was studied using the face-on X-ray radiography on the Shen-Guang II device. We obtained temporal evolution images of the R—T instability perturbation. The R—T instability growth factor has been obtained by using the methods of fast Fourier transform and seeking the difference of light intensity between the peak and the valley of the targets. Through comparison with the the theoretical simulation, we found that the experimental data had a good agreement with the theoretical simulation results before 1.8 ns, and was lower than the theoretical simulation results after that.

Key concepts: Rayleigh–Taylor instability, Instability, Perturbation (astronomy), Fourier transform, Physics, Richtmyer–Meshkov instability, Rayleigh scattering, Optics

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