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Visualizing electromagnetic fields in laser-produced counter-streaming plasma experiments for collisionless shock laboratory astrophysics

机译:在无碰撞冲击实验室天体物理学的激光产生的逆流等离子体实验中可视化电磁场

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摘要

Collisionless shocks are often observed in fast-moving astrophysical plasmas, formed by non-classical viscosity that is believed to originate from collective electromagnetic fields driven by kinetic plasma instabilities. However, the development of small-scale plasma processes into large-scale structures, such as a collisionless shock, is not well understood. It is also unknown to what extent collisionless shocks contain macroscopic fields with a long coherence length. For these reasons, it is valuable to explore collisionless shock formation, including the growth and self-organization of fields, in laboratory plasmas. The experimental results presented here show at a glance with proton imaging how macroscopic fields can emerge from a system of supersonic counter-streaming plasmas produced at the OMEGA EP laser. Interpretation of these results, plans for additional measurements, and the difficulty of achieving truly collisionless conditions are discussed. Future experiments at the National Ignition Facility are expected to create fully formed collisionless shocks in plasmas with no pre-imposed magnetic field.
机译:在快速移动的天体等离子体中通常会观察到无碰撞冲击,这种碰撞是由非经典粘度形成的,该非经典粘度被认为源于由动态等离子体不稳定性驱动的集体电磁场。但是,将小规模的等离子体工艺发展为大规模结构(例如无碰撞冲击)的方法尚未广为人知。还不知道无碰撞冲击在多大程度上包含具有长相干长度的宏观场。由于这些原因,在实验室等离子体中探索无碰撞激波的形成(包括磁场的增长和自组织)非常有价值。此处呈现的实验结果使质子成像一目了然,显示出如何从OMEGA EP激光器产生的超音速逆流等离子体系统中出现宏观场。讨论了这些结果的解释,其他测量计划以及实现真正无碰撞条件的难度。国家点火装置的未来实验有望在没有预先施加磁场的情况下在等离子体中形成完全形成的无碰撞冲击。

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