4.5 Article

Impact of negative triangularity plasma shaping on the n=0 resistive wall mode in a tokamak

期刊

NUCLEAR FUSION
卷 61, 期 9, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.1088/1741-4326/ac189a

关键词

MHD instability; negative triangularity plasma; resistive wall mode; tokamak; numerical simulations

资金

  1. National Research Foundation of Korea (NRF) - Korea government (MSIT) [NRF-2019R1F1A1058298, NRF-2019M1A7A1A03087584]
  2. R&D Program of 'Development of ITER non-procurement key-technologies through the Korea Institute of Fusion Energy (KFE) - Government fund [IN1904-2]
  3. U.S. Department of Energy
  4. National Research Council of Science & Technology (NST), Republic of Korea [IN1904] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)
  5. National Research Foundation of Korea [2019M1A7A1A03087584] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)

向作者/读者索取更多资源

The axisymmetric (n=0) resistive wall mode instability in negative triangularity plasma shape is influenced by plasma characteristics and geometric effects, with higher poloidal beta leading to more instability in negative triangularity compared to positive triangularity. Non-conformal wall shapes have been found to be helpful in stabilizing the n=0 mode, unless the plasma is too close to the walls at the nulls for the opposite triangularity.
The axisymmetric (n = 0) resistive wall mode instability is numerically investigated for the negative triangularity plasma shape, which has shown several benefits in terms of improved confinement time and fusion engineering. To evaluate the shape effects, we modified a MHD instability code AVSTAB (Axisymmetric Vertical STABility), which calculates the marginally controllable elongation in a simplified feedback capability parameter. The plasma characteristics (poloidal beta and internal inductance) as well as the geometric effects (wall shape and plasma location) are important to determine the instability. In contrast to positive triangularity, the higher poloidal beta provides more instability drive for the negative triangularity because of the higher Shafranov shift and the higher elongation of the inner flux surface of the MHD equilibrium. Non-conformal wall shapes to the plasmas (positive triangularity wall and negative triangularity plasma) are found to be rather helpful to stabilize the n = 0 mode, unless the plasma is too close to the walls at the nulls for the opposite triangularity.

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