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Magnetic reconnection in the MST reversed field pinch.

机译:MST反向磁场夹中的磁性重新连接。

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摘要

Magnetic field line reconnection is a process whereby magnetic field lines which are otherwise topologically preserved by, and frozen into, a plasma can break and reconnect to form field lines with different topologies. It plays a significant role in a wide variety of plasmas, including stellar, space and laboratory plasmas. This dissertation focuses on the underlying dynamics of reconnection in one particular kind of laboratory plasma, the Reversed Held Pinch, where it takes the form of tearing mode activity. Specifically, it reports measurements of the spatial structure of tearing mode induced magnetic and parallel current density fluctuations in the edge of MST.; At least four significant results are obtained. First, we observe direct evidence of reconnection at the reversal surface of MST, in the form of a magnetic field fluctuation that causes reconnection there. Second, we observe the associated current sheet. Such current sheets are a characteristic feature of reconnection, but their thicknesses are sensitive to the specific physical effects that allow it to occur. We compare the thickness of the observed current sheet to expectations from models of reconnection that incorporate different physical effects, including, among others things, resistivity, electron inertia, electron pressure and ion inertia. Third, we obtain estimates of the radial current density due to streaming of charge carriers along magnetic field lines which have been perturbed by reconnection. We find that, in contradiction with the expectation for isolated tearing modes, it is non-vanishing, and large enough to imply the existence of some mechanism to maintain charge neutrality. Fourth, we measure the Lorentz force on the plasma associated with reconnection. We observe that, in agreement with expectation for interacting tearing modes, this force has a radial structure during sawtooth crashes that reduces the equilibrium toroidal velocity shear. We observe, also, that it is large enough to imply the existence of other forces on the plasma.
机译:磁场线重新连接是这样的过程,在该过程中,原本由等离子体保存并冻结成等离子体的磁场线可以破裂并重新连接以形成具有不同拓扑的场线。它在各种等离子,包括恒星,空间和实验室等离子中都起着重要作用。本文着眼于一种特定类型的实验室血浆,即“反向夹持”中的重新连接的潜在动力学,该形式以撕裂模式活动的形式出现。具体来说,它报告了在MST边缘撕裂模式感应的磁和平行电流密度波动的空间结构的测量结果。至少获得四个显着结果。首先,我们观察到MST反转表面上重新连接的直接证据,即磁场波动的形式导致在那里重新连接。其次,我们观察相关的电流表。这样的电流板是重新连接的特征,但是它们的厚度对允许其发生的特定物理效应敏感。我们将观察到的电流表的厚度与重新连接模型的期望值进行了比较,该模型结合了不同的物理效应,其中包括电阻率,电子惯性,电子压力和离子惯性等。第三,我们获得由于载流子沿着磁场线流过而引起的径向电流密度的估计,该磁场线已受到重新连接的干扰。我们发现,与孤立的撕裂模式的期望相反,它没有消失,并且足够大以暗示存在某种维持电荷中性的机制。第四,我们测量与重新连接相关的等离子体上的洛伦兹力。我们观察到,与相互作用的撕裂模式的预期一致,该力在锯齿碰撞期间具有径向结构,从而减小了平衡环向速度剪切。我们还观察到,它足够大以暗示在等离子体上存在其他力。

著录项

  • 作者

    Crocker, Neal Acker, II.;

  • 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 2001
  • 页码 251 p.
  • 总页数 251
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 等离子体物理学;
  • 关键词

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