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Two-dimensional turbulence in magnetized plasmas

机译:磁化等离子体中的二维湍流

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In an inhomogeneous magnetized plasma the transport of energy and particles perpendicular to the magnetic field is in general mainly caused by quasi two-dimensional turbulent fluid mixing. The physics of turbulence and structure formation is of ubiquitous importance to every magnetically confined laboratory plasma for experimental or industrial application. Specifically, high-temperature plasmas for fusion energy research are also dominated by the properties of this turbulent transport. Self-organization of turbulent vortices to mesoscopic structures like zonal flows is related to the formation of transport barriers that can significantly enhance the confinement of a fusion plasma. This subject, of great importance in research, is rarely touched on in introductory plasma physics or continuum dynamics courses. Here a brief tutorial on 2D plasma turbulence is presented as an introduction to the field, appropriate for inclusion in undergraduate and graduate courses.
机译:在不均匀的磁化等离子体中,垂直于磁场的能量和粒子的传输通常主要是由准二维湍流混合引起的。湍流和结构形成的物理原理对于实验或工业应用中的每个磁场受限的实验室等离子体都至关重要。具体地说,用于聚变能研究的高温等离子体也受到这种湍流传输特性的支配。湍流涡流自组织成像纬向流这样的介观结构与传输壁垒的形成有关,传输壁垒可以显着增强聚变等离子体的约束。该学科在研究中具有重要意义,很少涉及等离子体物理入门课程或连续动力学课程。在这里,将简要介绍二维等离子体湍流,作为该领域的入门知识,适合纳入本科生和研究生课程。

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