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Confinement of pure electron plasmas in the Columbia Non-neutral Torus

机译:哥伦比亚非中性环面中纯电子等离子体的限制

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The Columbia Non-neutral Torus (CNT) [T. S. Pedersen, J. P. Kremer, R. G. Lefrancois, Q. Marksteiner, N. Pomphrey, W. Reiersen, F. Dahlgreen, and X. Sarasola, Fusion Sci. Technol. 50, 372 (2006)] is a stellarator used to study non-neutral plasmas confined on magnetic surfaces. A detailed experimental study of confinement of pure electron plasmas in CNT is described here. Electrons are introduced into the magnetic surfaces by placing a biased thermionic emitter on the magnetic axis. As reported previously, the insulated rods holding this and other emitter filaments contribute to the radial transport by charging up negatively and creating ExB convective transport cells. A model for the rod-driven transport is presented and compared to the measured transport rates under a number of different conditions, finding good agreement. Neutrals also drive transport, and by varying the neutral pressure in the experiment, the effects of rod-driven and neutral-driven transport are separated. The neutral-driven electron loss rate scales linearly with neutral pressure. The neutral driven transport, presumably caused by electron-neutral collisions, is much greater than theoretical estimates for neoclassical diffusion in a classical stellarator with strong radial electric fields. In fact the confinement time is on the order of the electron-neutral collision time. Ion accumulation, electron attachment, and other effects are considered, but do not explain the observed transport rates. (c) 2007 American Institute of Physics.
机译:哥伦比亚非中性环面(CNT)[T. S. Pedersen,J.P。Kremer,R.G。Lefrancois,Q.Marksteiner,N.Pomphrey,W.Reiersen,F.Dahlgreen和X.Sarasola,融合科学。技术。 50,372(2006)]是一种用于研究局限于磁性表面的非中性等离子体的恒星探测器。在此描述了在CNT中限制纯电子等离子体的详细实验研究。通过在磁轴上放置偏置的热电子发射体,将电子引入磁性表面。如先前所报道,保持该发射极灯丝和其他发射极灯丝的绝缘棒通过负电荷充电并形成ExB对流传输单元而有助于径向传输。提出了杆驱动运输的模型,并将其与在许多不同条件下测得的运输速率进行比较,发现有很好的一致性。中性物也驱动运输,并且通过改变实验中的中性压力,将杆驱动运输和中性驱动运输的影响分开。中性驱动的电子损失率与中性压力成线性比例关系。中性驱动的传输,大概是由电子中性碰撞引起的,比具有强径向电场的经典恒星器中新古典扩散的理论估计要大得多。实际上,限制时间约为电子中性碰撞时间。考虑了离子积累,电子附着和其他影响,但不能解释观察到的传输速率。 (c)2007年美国物理研究所。

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