Matter and Radiation at Extremes, Volume. 9, Issue 1, 016603(2024)
Growth of ablative Rayleigh-Taylor instability induced by time-varying heat-flux perturbation
Fig. 1. Simulation setup for
Fig. 2. (a) Ratio of bubble velocity to corresponding classical value
Fig. 3. Density contours of ARTI induced by time-varying heat-flux (TVHF) perturbation for different
Fig. 4. Temporal evolution of bubble velocity for ARTI induced by TVHF and SHF perturbations for (a)
Fig. 5. (a) Simulation (red triangles) and theoretical (black solid line) results for linear growth rate and (b) average effective acceleration (blue dots) and ablation pressure (red squares) in linear stage of ARTI induced by TVHF perturbation for different
Fig. 6. Linear growth rate of ARTI vs phase velocity of TVHF perturbation for different
Fig. 7. Average phase difference of density and temperature fluctuations traveling along
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Yang Liu, De-Hua Zhang, Jing-Fei Xin, Yudong Pu, Jun Li, Tao Tao, Dejun Sun, Rui Yan, Jian Zheng. Growth of ablative Rayleigh-Taylor instability induced by time-varying heat-flux perturbation[J]. Matter and Radiation at Extremes, 2024, 9(1): 016603
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Received: May. 7, 2023
Accepted: Sep. 17, 2023
Published Online: Mar. 27, 2024
The Author Email: Rui Yan (ruiyan@ustc.edu.cn)