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Dynamics of plasma expansion and Shockwave formation in femtosecond laser-ablated aluminum plumes in argon gas at atmospheric pressures

机译:飞秒激光烧蚀的氩气中大气压下飞秒激光烧蚀的铝羽中等离子体膨胀和冲击波形成的动力学

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Plasma expansion with shockwave formation during laser ablation of materials in a background gasses is a complex process. The spatial and temporal evolution of pressure, temperature, density, and velocity fields is needed for its complete understanding. We have studied the expansion of femtosecond (fs) laser-ablated aluminum (Al) plumes in Argon (Ar) gas at 0.5 and 1 atmosphere (atm). The expansion of the plume is investigated experimentally using shadowgraphy and fast-gated imaging. The computational fluid dynamics (CFD) modeling is also carried out. The position of the shock front measured by shadowgraphy and fast-gated imaging is then compared to that obtained from the CFD modeling. The results from the three methods are found to be in good agreement, especially during the initial stage of plasma expansion. The computed time- and space-resolved fields of gas-dynamic parameters have provided valuable insights into the dynamics of plasma expansion and shockwave formation in fs-pulse ablated Al plumes in Ar gas at 0.5 and 1 atm. These results are compared to our previous data on nanosecond (ns) laser ablation of Al [S. S. Harilal et al., Phys. Plasmas 19, 083504 (2012)]. It is observed that both fs and ns plumes acquire a nearly spherical shape at the end of expansion in Ar gas at 1 atm. However, due to significantly lower pulse energy of the fs laser (5 mJ) compared to pulse energy of the ns laser (100 mJ) used in our studies, the values of pressure, temperature, mass density, and velocity are found to be smaller in the fs laser plume, and their time evolution occurs much faster on the same time scale. The oscillatory shock waves clearly visible in the ns plume are not observed in the internal region of the fs plume. These experimental and computational results provide a quantitative understanding of plasma expansion and shockwave formation in fs-pulse and ns-pulse laser ablated Al plumes in an ambient gas at atmospheric pressures.
机译:在背景气体中对材料进行激光烧蚀时,伴随冲击波形成的等离子体膨胀是一个复杂的过程。需要对其压力,温度,密度和速度场的时空演化进行全面了解。我们已经研究了在0.5和1个大气压(atm)下飞秒(fs)激光烧蚀的铝(Al)羽在氩(Ar)气体中的膨胀。使用阴影摄影和快速门控成像技术对烟羽的膨胀进行了实验研究。还进行了计算流体动力学(CFD)建模。然后将通过阴影摄影和快速门控成像测得的激波锋的位置与从CFD建模中获得的位置进行比较。发现这三种方法的结果吻合良好,尤其是在血浆膨胀的初始阶段。气体动力学参数在时间和空间上的解析场为在0.5和1 atm的Ar气中fs脉冲烧蚀的Al羽流中的等离子体膨胀和冲击波形成的动力学提供了有价值的见解。将这些结果与我们先前对Al [S. S.Harilal等,Phys。 Plasmas 19,083504(2012)]。可以看出,在1 atm的Ar气体膨胀结束时,fs和ns羽流都获得了近似球形的形状。然而,由于与我们研究中使用的ns激光(100 mJ)的脉冲能量相比,fs激光(5 mJ)的脉冲能量明显更低,因此发现压力,温度,质量密度和速度的值较小在fs激光羽中,它们的时间演化在相同的时间尺度上要快得多。在ns羽中清晰可见的振荡冲击波未在fs羽的内部区域中观察到。这些实验和计算结果提供了对大气压力下fs脉冲和ns脉冲激光烧蚀的Al羽流中等离子体膨胀和冲击波形成的定量理解。

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