Biermann-battery driven magnetized collisionless shock precursors in laser produced plasmas

Timothy Johnson, Graeme Sutcliffe, Jacob Pearcy, Andrew Birkel, Gabriel Rigon, Neel Kabadi, Brandon Lahmann, Patrick Adrian, Benjamin Reichelt, Justin Kunimune, Skylar Dannhoff, Matt Cufari, Frank Tsung, Hui Chen, Joseph Katz, Vladimir Tikhonchuk, Chikang Li
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Abstract

This letter reports the first complete observation of magnetized collisionless shock precursors formed through the compression of Biermann-battery magnetic fields in laser produced plasmas. At OMEGA, lasers produce a supersonic CH plasma flow which is magnetized with Biermann-battery magnetic fields. The plasma flow collides with an unmagnetized hydrogen gas jet plasma to create a magnetized shock precursor. The situation where the flowing plasma carries the magnetic field is similar to the Venusian bow shock. Imaging 2$\omega$ Thomson scattering confirms that the interaction is collisionless and shows density and temperature jumps. Proton radiographs have regions of strong deflections and FLASH magnetohydrodynamic (MHD) simulations show the presence of Biermann fields in the Thomson scattering region. Electrons are accelerated to energies of up to 100 keV in a power-law spectrum. OSIRIS particle-in-cell (PIC) simulations, initialized with measured parameters, show the formation of a magnetized shock precursor and corroborate the experimental observables.
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激光产生的等离子体中的比尔曼电池驱动的磁化无碰撞冲击前体
这封信首次报告了对激光产生的等离子体中通过比尔曼电池磁场压缩而形成的磁化无碰撞冲击前兆的完整观测。在欧米茄,激光产生的超音速CH等离子体流被比尔曼电池磁场磁化。等离子体流与未磁化的氢气喷射等离子体碰撞,产生磁化的冲击前体。流动等离子体携带磁场的情况类似于金星的弓形冲击。成像2Ω汤姆逊散射证实了这种相互作用是无碰撞的,并显示出密度和温度的跃迁。质子射线照片有强偏转区域,FLASH 磁流体力学(MHD)模拟显示汤姆逊散射区域存在比尔曼场。在幂律频谱中,电子被加速到高达 100 keV 的能量。用测量参数初始化的 OSIRIS 粒子在胞(PIC)模拟显示了磁化冲击前体的形成,并证实了实验观测数据。
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