X-ray imaging and electron temperature evolution in laser-driven magnetic reconnection experiments at the national ignition facility

被引:0
|
作者
Valenzuela-Villaseca, Vicente [1 ]
Molina, Jacob M. [1 ,2 ]
Schaeffer, Derek B. [3 ]
Malko, Sophia [2 ]
Griff-McMahon, Jesse [1 ,2 ]
Lezhnin, Kirill [2 ]
Rosenberg, Michael J. [4 ]
Hu, S. X. [4 ]
Kalantar, Dan [5 ]
Trosseille, Clement [5 ]
Park, Hye-Sook [5 ]
Remington, Bruce A. [5 ]
Fiksel, Gennady [6 ]
Uzdensky, Dmitri [7 ]
Bhattacharjee, Amitava [1 ,2 ]
Fox, William [1 ,2 ]
机构
[1] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[2] Princeton Plasma Phys Lab, Princeton, NJ 08540 USA
[3] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[4] Univ Rochester, Lab Laser Energet, Rochester, NY 14623 USA
[5] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[6] Univ Michigan, Ctr Ultrafast Opt Sci, Ann Arbor, MI 48109 USA
[7] Univ Colorado, Ctr Integrated Plasma Studies, Boulder, CO 80309 USA
基金
美国国家科学基金会;
关键词
ACCELERATION;
D O I
10.1063/5.0213598
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We present results from x-ray imaging of high-aspect-ratio magnetic reconnection experiments driven at the National Ignition Facility. Two parallel, self-magnetized, elongated laser-driven plumes are produced by tiling 40 laser beams. A magnetic reconnection layer is formed by the collision of the plumes. A gated x-ray framing pinhole camera with micro-channel plate detector produces multiple images through various filters of the formation and evolution of both the plumes and current sheet. As the diagnostic integrates plasma self-emission along the line of sight, two-dimensional electron temperature maps < Te >(Y) are constructed by taking the ratio of intensity of these images obtained with different filters. The plumes have a characteristic temperature < Te >(Y )= 240 +/- 20 eV at 2 ns after the initial laser irradiation and exhibit a slow cooling up to 4 ns. The reconnection layer forms at 3 ns with a temperature < Te >(Y )= 280 +/- 50 eV as the result of the collision of the plumes. The error bars of the plumes and current sheet temperatures separate at 4 ns, showing the heating of the current sheet from colder inflows. Using a semi-analytical model, we survey various heating mechanisms in the current sheet. We find that reconnection energy conversion would dominate at low density ( n(e )less than or similar to 7 x 10(18) cm(-3)) and electron-ion collisional drag at high-density ( greater than or similar to 10(19) cm(-3)).
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页数:19
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