Nonlinear simulations of the peeling-ballooning instability of super H-modes in the HL-3 tokamak

被引:1
|
作者
Zhu, Yiren [1 ]
Zhong, Wulyu [1 ]
Zou, Xiaolan [2 ]
Li, Jiaxian [1 ]
Xue, Miao [1 ]
Li, Zhengji [1 ]
Xue, Lei [1 ]
Xiao, Guoliang [1 ]
Tong, Ruihai [1 ]
Zou, Yunpeng [1 ]
Yin, Jiao [1 ]
Liang, Anshu [1 ]
Liu, Linzi [1 ]
Yuan, Boda [1 ]
Xu, Min [1 ]
机构
[1] Southwestern Inst Phys, POB 432, Chengdu 610041, Peoples R China
[2] CEA, IRFM, F-13108 St Paul Les Durance, France
基金
国家重点研发计划; 中国国家自然科学基金;
关键词
super H-mode; ELM; EPED; E x B velocity shear; HL-3; CONFINEMENT; TRANSPORT; PLASMA;
D O I
10.1088/1741-4326/ad5e94
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
As the newly built tokamak in China, HL-3 will explore high-performance operation scenarios, such as super H-mode. The energy confinement and core parameters in the super H-mode can be much larger than that in the normal H-mode. Based on the pedestal simulation code EPED, the operation space of the super H-mode is obtained in HL-3. Magnetic shear decreases with increasing triangularity; consequently, a super H-mode can be achieved. The threshold of triangularity for accessing a super H-mode in HL-3 is around 0.4. By using BOUT++, a nonlinear simulation study of the pedestal instabilities in the super H-mode equilibrium is executed for the first time. As expected, the low n peeling mode, which can cause much of the energy loss (17%) from the pedestal region, is dominant in the super H-mode. Such a large collapse in the pedestal region would lead to a transition from super H-mode to H-mode. It is crucial to expand the parameter space of the super H-mode or mitigate the edge-localized mode (ELM) size for sustaining the super H-mode operations. The E x B velocity shear is found to play an important role in controlling the ELMs in HL-3. The small E x B velocity shear leads to a large growth rate but results in a small ELM size around the peeling boundary. The ELM size is closely related to both the growth rate of peeling-ballooning mode and the duration time of the linear phase. In contrast, a large E x B velocity shear can stabilize the instabilities near the ballooning boundary. Next, the parameter space of the super H-mode can be enlarged.
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页数:14
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