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Spinning an unmagnetized plasma for magnetorotational instability studies in the Plasma Couette Experiment.

机译:旋转未磁化的等离子体进行等离子Couette实验中的磁旋转不稳定性研究。

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摘要

A new concept for creating a large, steady-state, fast flowing, hot plasma which is weakly magnetized has been demonstrated experimentally, marking an important first step towards laboratory studies of a wide variety of phenomenon important in plasma astrophysics. In particular, the magnetorotational instability (MRI) mechanism is of great interest for its role in generating the turbulence necessary for efficient outward transport of angular momentum in accretion disks. The instability has been the subject of extensive analytical and numerical investigations for several decades, yet experimental verification of the MRI remains elusive.;In the Plasma Couette Experiment, plasma is confined by a cylindrical ``bucket'' assembly of permanent magnets, arranged in rings of alternating polarity, to form an axisymmetric cusp magnetic field. The field is localized to the boundaries, leaving a large, unmagnetized plasma in the bulk. Plasma is produced with 2.45 GHz microwave heating, reaching Te < 10 eV, Ti < 1 eV, and n = 1010--10 11 cm-3. The plasma is stirred using J x B forces in the magnetized edge region, where current is driven by toroidally localized, electrostatically biased hot cathodes. Torque can be applied at the inner or outer boundaries, resulting in a controlled, differentially rotating flow.;Mach probe measurements show that the azimuthal flow viscously couples momentum from the magnetized edge into the unmagnetized bulk. Collisional ion viscosity must overcome the drag due to ion-neutral collisions for the plasma to rotate. A self-consistent, rotation-induced radial electric field is also measured. Maximum speed limits have been observed for various gas species (He ~ 12 km/s, Ne ~ 4 km/s, Ar ~ 3.2 km/s, Xe ~ 1.4 km/s), consistent with a critical ionization velocity limit reported to occur in partially ionized plasmas. The experiment has achieved magnetic Reynolds numbers of Rm ∼ 65 and magnetic Prandtl numbers of Pm ~ 0.2-10, which are approaching regimes shown to excite the MRI in local linear analysis which incorporates dissipation, the Hall term, and momentum loss through ion-neutral collisions.
机译:实验证明了一种用于创建大的,稳态的,快速流动的,被弱磁化的热等离子体的新概念,这标志着实验室研究对等离子体天体物理学中各种重要现象的迈出了重要的第一步。尤其是,磁旋转不稳定性(MRI)机制因其在产生积聚盘中角动量的有效向外传输所必需的湍流中的作用而引起了极大的兴趣。数十年来,不稳定性一直是广泛的分析和数值研究的主题,但MRI的实验验证仍然难以捉摸。在等离子库埃特实验中,等离子体由永久磁铁的圆柱形``桶''组件限制,排列在交替极性的环,以形成轴对称的尖端磁场。磁场局限于边界,从而在主体中留下了较大的未磁化等离子体。通过2.45 GHz微波加热产生等离子体,达到Te <10 eV,Ti <1 eV和n = 1010--10 11 cm-3。使用J x B力在磁化的边缘区域搅拌等离子体,在该区域中,电流由环形定位的静电偏压热阴极驱动。可以在内部或外部边界处施加扭矩,从而产生可控的,不同方向的旋转流。马赫探针测量表明,方位流将动量从磁化边缘粘稠地耦合到未磁化的块体中。碰撞离子粘度必须克服由于离子中性碰撞而引起的阻力,以使等离子体旋转。还测量了自洽,旋转感应的径向电场。已观察到各种气体的最大速度限制(He〜12 km / s,Ne〜4 km / s,Ar〜3.2 km / s,Xe〜1.4 km / s),与据报导的临界电离速度限制一致在部分电离的等离子体中。该实验已经获得了Rm〜65的雷诺数和Pm〜0.2-10的普朗特数,这是在局部线性分析中激发MRI的一种接近机制,其中包括耗散,霍尔项和离子中性引起的动量损失。碰撞。

著录项

  • 作者

    Collins, Cami.;

  • 作者单位

    The University of Wisconsin - Madison.;

  • 授予单位 The University of Wisconsin - Madison.;
  • 学科 Physics Fluid and Plasma.
  • 学位 Ph.D.
  • 年度 2013
  • 页码 143 p.
  • 总页数 143
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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