旋转磁场下 REBCO 堆的交流损耗数值模拟

IF 5.6 Q1 ENGINEERING, ELECTRICAL & ELECTRONIC
Yuan Wang , Jin Fang , Timothy Haugan , Rodney A. Badcock , James G. Storey , Zhenan Jiang
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引用次数: 0

摘要

交流损耗是高温超导(HTS)旋转机器面临的一项重大挑战。迄今为止,人们已经探索了单个 HTS 磁带在旋转磁场 (RF) 下的总交流损耗 (Qtol)(有电流)和磁化损耗 (Qm)(无电流)的特性。然而,在了解这些发现如何转化为旋转机器中更复杂的 HTS 绕组方面,研究仍存在差距。要了解更复杂的 HTS 结构(如 HTS 叠层)的损耗行为,还需要进一步的探索。在这项工作中,对射频和垂直交流驻波磁场下 HTS 叠层中的 Qtol 和 Qm 进行了数值研究。研究考虑了两种不同的射频模型:一种是 Uni-RF 模型,其特点是均匀磁场,每个位置的磁场幅值和相位都相等;另一种是由旋转的哈尔巴赫阵列产生的非均匀磁场,称为 Hal-RF 模型。我们探讨了交流损耗与堆栈中磁带数量、磁带宽度 (2a) 和磁带倾斜角 (α)(指堆栈法线方向与垂直方向之间的夹角)等参数的关系。堆栈中的磁带数量从 1 到 16 不等,α 的范围从 0° 到 90°,磁带宽度包括 4 毫米和 40 毫米。此外,还考虑了不同的旋转磁场方向。有趣的是,根据 Brandt 和 Indenbom 方程得出的超导带(BI-strip)Qm 分析值接近于高场强下驻波堆的 Qm 结果,而在 1 T 时,它们比 Hal-RF 模型中的 Qm 高出两倍多。我们还在 Hal-RF 模型中发现,当应用非对称 Jc (B, θ) 数据时,不同的磁场旋转方向会导致 Qm 和 Qtol 不同。此外,我们还观察到,在均匀射频下,倾角对 Qm 没有影响,而在 Hal-RF 模型中,倾角对 Qm 和 Qtol 都有显著影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Numerical simulations on the AC loss of REBCO stacks under rotating magnetic fields

AC loss presents a significant challenge for high-temperature superconducting (HTS) rotating machines. To date, the behaviour of total AC loss (Qtol) (with current) and magnetization loss (Qm) (without current) in a single HTS tape under rotating magnetic fields (RF) have been explored. However, a research gap remains in understanding how these findings translate to the more complex HTS windings of rotating machines. Further exploration is needed to understand the loss behaviour of more complex HTS structures, such as HTS stacks. In this work, Qtol and Qm, in the HTS stacks under RF and a perpendicular AC standing wave magnetic field are numerically investigated. Two different RF models are considered: one is the Uni-RF model, characterized by a uniform field with equal field amplitudes and phases at each position, and the other is a non-uniform field created by a rotating Halbach array, referred to as the Hal-RF model. The dependence of AC loss on parameters such as the number of tapes in the stacks, tape width (2a), and the inclination angle (α) of tapes, which refers to the angle between the normal direction of the stack and the vertical direction, have been explored. The number of tapes in the stacks ranges from 1 to 16, α ranges from 0° to 90°, and the tape width includes 4 mm and 40 mm. Additionally, different rotating field directions are also considered. Interestingly, the analytical values from Brandt and Indenbom equation for Qm of a superconducting strip (BI-strip) are close to Qm results of the stacks under the standing wave at high fields, while they are over twice as high as those in the Hal-RF model at 1 T. This suggests the BI-strip equation is not reliable for predicting Qm under RF at high fields. We also show in the Hal-RF model that different rotation directions of the field lead to varying Qm and Qtol when asymmetric Jc (B, θ) data are applied. Moreover, it has been observed that the inclination angle has no impact on Qm under uniform RF while significantly impacts both Qm and Qtol in the Hal-RF model.

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