Numerical study of plasmas start-up by electron cyclotron waves in NCST spherical tokamak and CN-H1 stellarator

Yizhuohang Liu, P. Zheng, Xueyu Gong, Lan Yin, Xiaochang Chen, Yijun Zhong, Wenjun Yang
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Abstract

According to the physics of tokamak start-up, this paper constructs a zero-dimensional (0D) model applicable to electron cyclotron (EC) wave assisted start-up in NCST spherical torus (spherical tokamak) and CN-H1 stellarators. Using the constructed zero-dimensional model, the results obtained in this paper under the same conditions are compared and validated against references results for pure hydrogen plasma start-up in tokamak. The results are in good agreement, especially regarding electron temperature, ion temperature and plasma current. In the presence of finite Ohmic electric field in the spherical tokamak, a study on the EC wave assisted start-up of the NCST plasma at frequency of 28 GHz is conducted. The impact of the vertical magnetic field B v on EC wave assisted start-up, the relationship between EC wave injection power P inj, Ohmic electric field E, and initial hydrogen atom density nH0 is explored separately. It is found that under conditions of Ohmic electric field lower than ITER (~ 0.3 V m-1), EC wave can expand the operational space to achieve better plasma parameters. Simulating the process of 28 GHz EC wave start-up in the CN-H1 stellarator plasma, the plasma current in the zero-dimensional model is replaced with the current in the poloidal coil of the stellarator. Plasma start-up can be successfully achieved at injection powers in the hundreds of kilowatts range, resulting in electron densities on the order of 1017 to 1018 m-3.
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NCST 球形托卡马克和 CN-H1 恒星器中电子回旋波启动等离子体的数值研究
根据托卡马克启动的物理学原理,本文构建了一个零维(0D)模型,适用于 NCST 球形环(球形托卡马克)和 CN-H1 恒星器的电子回旋波辅助启动。利用所构建的零维模型,本文将在相同条件下获得的结果与托卡马克中纯氢等离子体启动的参考结果进行了比较和验证。结果非常吻合,尤其是在电子温度、离子温度和等离子体电流方面。在球形托卡马克中存在有限欧姆电场的情况下,对频率为 28 GHz 的 NCST 等离子体的欧共体波辅助启动进行了研究。分别探讨了垂直磁场 B v 对电子波辅助启动的影响、电子波注入功率 P inj、欧姆电场 E 和初始氢原子密度 nH0 之间的关系。研究发现,在欧姆电场低于国际热核聚变实验堆(约 0.3 V m-1)的条件下,EC 波可以扩大运行空间,获得更好的等离子体参数。模拟在 CN-H1 恒星器等离子体中启动 28 GHz EC 波的过程时,零维模型中的等离子体电流被替换为恒星器极性线圈中的电流。等离子体启动可在数百千瓦的注入功率范围内成功实现,电子密度约为 1017 至 1018 m-3。
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