论文标题

电子芯片不稳定性诱导光场离子化等离子体中的磁场

Electron Weibel instability induced magnetic fields in optical-field ionized plasmas

论文作者

Zhang, Chaojie, Wu, Yipeng, Sinclair, Mitchell, Farrell, Audrey, Marsh, Kenneth A., Hua, Jianfei, Petrushina, Irina, Vafaei-Najafabadi, Navid, Kupfer, Rotem, Kusche, Karl, Fedurin, Mikhail, Pogorelsky, Igor, Polyanskiy, Mikhail, Huang, Chen-Kang, Lu, Wei, Mori, Warren B., Joshi, Chan

论文摘要

等离子体中的磁场的产生和扩增是一个长期以来血浆和空间物理学引起的兴趣的长期话题。电子芯片不稳定性是一种众所周知的机制,负责具有温度各向异性的等离子体中的自生磁场,并且在理论和仿真中都进行了广泛的研究,但是对这种不稳定性的实验验证却是具有挑战性的。最近,我们展示了一个新的实验平台,该平台能够通过光场电离进行高度非热和/或各向异性等离子体电子速度分布的受控初始化。据我们所知,使用线性加速器的外部电子探针束,首次测量了由于电子芯片不稳定性而引起的自生磁场的发作,饱和和衰减。 In this paper, we will first present experimental results on time-resolved measurements of the Weibel magnetic fields in non-relativistic plasmas produced by Ti:Sapphire laser pulses (0.8 $μm$) and then discuss the feasibility of extending the study to quasi-relativistic regime by using intense $\rm CO_2$ (e.g., 9.2 $μm$) lasers to produce更热的等离子体。

Generation and amplification of magnetic fields in plasmas is a long-standing topic that is of great interest to both plasma and space physics. The electron Weibel instability is a well-known mechanism responsible for self-generating magnetic fields in plasmas with temperature anisotropy and has been extensively investigated in both theory and simulations, yet experimental verification of this instability has been challenging. Recently, we demonstrated a new experimental platform that enables the controlled initialization of highly nonthermal and/or anisotropic plasma electron velocity distributions via optical-field ionization. Using an external electron probe bunch from a linear accelerator, the onset, saturation and decay of the self-generated magnetic fields due to electron Weibel instability were measured for the first time to our knowledge. In this paper, we will first present experimental results on time-resolved measurements of the Weibel magnetic fields in non-relativistic plasmas produced by Ti:Sapphire laser pulses (0.8 $μm$) and then discuss the feasibility of extending the study to quasi-relativistic regime by using intense $\rm CO_2$ (e.g., 9.2 $μm$) lasers to produce much hotter plasmas.

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