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Electron Pressure Profiles in High-Density Neutral Beam Heated Plasmas in the Large Helical Device

机译:大型螺旋装置中高密度中性束加热等离子体中的电子压力分布

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摘要

In the Large Helical Device (LHD), electron pressure profiles in gas-fueled high-density discharges tend to have a similar shape, as if these were frozen. This frozen profile is insensitive to variations in the magnetic field strength and moderate changes in the neutral beam heat deposition profile. At the same time, however, the absolute value of the electron pressure itself increases with the heating power, the electron density, and the magnetic field strength. In this study, a reference model for the electron pressure is proposed which consists of the frozen profile and parametric dependences derived from experimental observations. It is possible to define an operational regime where this typical profile appears by comparing the electron pressure profiles with this model. In the standard configuration, at which the maximum plasma stored energy in LHD has been obtained, the frozen profile appears in the plateau to the Pfirsh-Schl?ter regimes. As the collisionality decreases to the collisionless regime, the electron pressure becomes smaller than the prediction of the model and the deterioration is significant in the plasma core region. This tendency is enhanced in the configuration with the outward-shifted magnetic axis. The global energy confinement time, τE, in the high-collisionality regime has a weaker density dependence together with the mitigated power degradation, scaling as τE∝nebar0.28P-0.43 (nebar and P are the line-averaged density and the heating power, respectively), compared with the International Stellarator Scaling 95, where τE∝nebar0.51P-0.59.
机译:在大型螺旋装置(LHD)中,以气体为燃料的高密度放电中的电子压力曲线往往具有相似的形状,就好像它们被冻结了一样。这种冻结的轮廓对磁场强度的变化和中性束热沉积轮廓的适度变化不敏感。但是,与此同时,电子压力本身的绝对值随着加热功率,电子密度和磁场强度而增加。在这项研究中,提出了一种电子压力的参考模型,该模型包括冻结的轮廓和从实验观察中得出的参数依赖性。通过将电子压力曲线与该模型进行比较,可以定义一个运行状态,在该运行状态下该典型曲线会出现。在标准配置下,在该配置下已获得LHD中最大的血浆存储能量,其冻结曲线出现在Pfirsh-Schlter模式的稳定期。当碰撞性降低到无碰撞状态时,电子压力变得小于模型的预测,并且等离子体核心区域的劣化显着。这种趋势在磁轴向外移动的配置中得到增强。高碰撞状态下的全局能量约束时间τE具有较弱的密度依赖性以及缓和的功率退化,缩放为τE∝nebar0.28P-0.43(nebar和P是线平均密度和加热功率,分别与国际Stellarator Scaling 95(其中τEbarnebar0.51P-0.59)进行比较。

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