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Numerical simulations of fishbones driven by fast ions in negative triangularity tokamak

Ren Zhen-Zhen Shen Wei

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Numerical simulations of fishbones driven by fast ions in negative triangularity tokamak

Ren Zhen-Zhen, Shen Wei
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  • The discharges with negative triangularity have lower turbulence induced transport and better energy confinement, so the tokamak with negative triangularity is recognized to be a better choice for future fusion device. In order to explore the features of the energetic particle driven instabilities with negative triangularity, the kinetic-magnetohydrodynamic hybrid code M3D-K is used to investigate the linear instability and nonlinear evolution of the fishbone driven by energetic ions with different triangularity. Based on EAST-like parameters, it is found that the negative triangularity destabilizes the ideal internal kink mode, but stabilizes the fishbone instability. Nonlinear simulations show that the fishbone instability with negative triangularity is hard to saturate without fluid nonlinearity. The possible explanation is that the orbits of fast ions are located more centrally with negative triagularity, so the energy exchange between energetic ions and the fishbone is more efficient than that with positive triangularity. These simulation results demonstrate that the negative triangularity does not have an obvious advantage over the positive triangularity, with the fishbone driven by energetic particles considered.
      Corresponding author: Shen Wei, shenwei@ipp.ac.cn
    • Funds: Project supported by the National Key R&D Program of China (Grant No. 2019YFE03050002), the National Natural Science Foundation of China (Grant Nos. 12005003, 11975270), and the Science Foundation of Institute of Plasma Physics, Chinese Academy of Sciences (Grant No. DSJJ-2022-04).
    [1]

    Hofmann F, Sauter O, Reimerdes H, et al. 1998 Phys. Rev. Lett. 81 2918Google Scholar

    [2]

    Camenen Y, Pochelon A, Behn R, et al. 2007 Nucl. Fusion 47 510Google Scholar

    [3]

    Solomon W M, Snyder P B, Burrell K H, et al. 2014 Phys. Rev. Lett. 113 135001Google Scholar

    [4]

    Snyder P B, Solomon W M, Burrell K H, et al. 2015 Nucl. Fusion 55 083026Google Scholar

    [5]

    Reimerdes H, Pochelon A, Sauter O, et al. 2000 Plasma Phys. Control. Fusion 42 629Google Scholar

    [6]

    Marinoni A, Brunner S, Camenen Y, et al. 2009 Plasma Phys. Control. Fusion 51 055016Google Scholar

    [7]

    Austin M E, Marinoni A, Walker M L, et al. 2019 Phys. Rev. Lett. 122 115001Google Scholar

    [8]

    Medvedev S, Kikuchi M, Villard L, et al. 2015 Nucl. Fusion 55 063013Google Scholar

    [9]

    Chen W, Wang Z X 2020 Chin. Phys. Lett. 37 125001Google Scholar

    [10]

    McGuire K, Goldston R, Bell M, et al. 1983 Phys. Rev. Lett. 50 891Google Scholar

    [11]

    Chen L, White R B, Rosenbluth M N 1984 Phys. Rev. Lett. 52 1122Google Scholar

    [12]

    Coppi B, Porcelli F 1986 Phys. Rev. Lett. 57 2272Google Scholar

    [13]

    Heidbrink W W, Bol K, Buchenauer D, et al. 1986 Phys. Rev. Lett. 57 835Google Scholar

    [14]

    Heidbrink W W, Sager G 1990 Nucl. Fusion 30 1015Google Scholar

    [15]

    Nave M F F, Campbell D J, Joffrin E, et al. 1991 Nucl. Fusion 31 697Google Scholar

    [16]

    von Goeler S, Roquemore A L, Johnson L C, et al. 1996 Rev. Sci. Instrum 67 473Google Scholar

    [17]

    Kass T, Bosch H S, Hoenen F, et al. 1998 Nucl. Fusion 38 807Google Scholar

    [18]

    Chen W, Ding X T, Liu Y, et al. 2010 Nucl. Fusion 50 084008Google Scholar

    [19]

    Xu L Q, Zhang J Z, Chen K Y, et al. 2015 Phys. Plasmas 22 122510

    [20]

    Shi P W, Chen W, Duan X R 2021 Chin. Phys. Lett. 38 035202Google Scholar

    [21]

    Van Zeeland M A, Collins C S, Heidbrink W W, et al. 2019 Nucl. Fusion 59 086028Google Scholar

    [22]

    Park W, Belova E V, Fu G Y, et al. 1999 Phys. Plasmas 6 1796Google Scholar

    [23]

    Fu G Y, Park W, Strauss H R, et al. 2006 Phys. Plasmas 13 052517Google Scholar

    [24]

    Lang J Y, Fu G Y, Chen Y 2010 Phys. Plasmas 17 042309Google Scholar

    [25]

    Cai H S, Fu G Y 2012 Phys. Plasmas 19 072506Google Scholar

    [26]

    Shen W, Fu G Y, Sheng Z M, et al. 2014 Phys. Plasmas 21 092514Google Scholar

    [27]

    Shen W, Wang F, Fu G Y, et al. 2017 Nucl. Fusion 57 116035Google Scholar

    [28]

    Wang F, Fu G Y, Shen W 2017 Nucl. Fusion 57 016034Google Scholar

    [29]

    Wang F, Yu L M, Fu G Y, et al. 2017 Nucl. Fusion 57 056013Google Scholar

    [30]

    Ren Z Z, Wang F, Fu G Y, et al. 2017 Phys. Plasmas 24 052501Google Scholar

    [31]

    Ren Z Z, Fu G Y, Van Zeeland M A, et al. 2018 Phys. Plasmas 25 122504Google Scholar

    [32]

    Shen W, Porcelli F 2018 Nucl. Fusion 58 106035Google Scholar

    [33]

    Chen W, Zhu X L, Wang F, et al. 2019 Nucl. Fusion 59 096037Google Scholar

    [34]

    Shen W, Wang F, Fu G Y, et al. 2020 Nucl. Fusion 60 106016Google Scholar

    [35]

    Xu L Q, Shen W, Ren Z Z, et al. 2021 Nucl. Fusion 61 076005Google Scholar

    [36]

    Ren Z Z, Shen W, Li G Q, et al. 2022 AIP Advances 12 075318Google Scholar

    [37]

    Porcelli F 1991 Plasma Phys. Control. Fusion 33 1601Google Scholar

    [38]

    Wang X Q, Wang X G 2016 Nucl. Fusion 56 036024Google Scholar

    [39]

    Wang X Q, Wang X G 2017 Nucl. Fusion 57 016039Google Scholar

    [40]

    Eriksson H G, Wahlberg C 2002 Phys. Plasmas 9 1606Google Scholar

    [41]

    Martynov A, Graves J P, Sauter O 2005 Plasma Phys. Control. Fusion 47 1743Google Scholar

    [42]

    Bussac M N, Pellat R, Edery D, et al. 1975 Phys. Rev. Lett. 35 1638Google Scholar

  • 图 1  安全因子与总压强平衡剖面

    Figure 1.  Equilibrium profiles of safety factor and total pressure.

    图 2  不同三角形变下模频率和线性增长率与快离子压强比值$ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} $的关系

    Figure 2.  Mode frequency and linear growth rate as a function of the fast ion pressure fraction $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} $.

    图 3  不同高能量离子压强比值$ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} $下的流函数$ U $  (a) $ \delta = - 0.436 $, $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} = 0 $; (b) $ \delta = - 0.436 $, $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} = 0.15 $; (c) $ \delta = - 0.436 $, $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} = $$ 0.4 $; (d) $ \delta=0.436 $, $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} = 0.4 $

    Figure 3.  Velocity stream function $ U $ at different fast ion pressure fraction $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} $: (a) $ \delta = - 0.436 $, $ P_{{\rm{hot}}, 0}/ P_{{\rm{total}}, 0} = $$ 0 $; (b) $ \delta = - 0.436 $, $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} = 0.15 $; (c) $ \delta = - 0.436 $, $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} = 0.4 $; (d) $ \delta = 0.436 $, $ P_{{\rm{hot}}, 0}/ P_{{\rm{total}}, 0} $$ = 0.4 $.

    图 4  芯部压强剖面平坦下模频率和线性增长率与快离子压强比值$ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} $的关系

    Figure 4.  Mode frequency and linear growth rate as a function of the fast ion pressure fraction $ P_{{\rm{hot}}, 0}/P_{{\rm{total}}, 0} $ with flat pressure profile.

    图 5  没有磁流体非线性效应的鱼骨模非线性演化 (a) 动能的$ n = 1 $分量的演化; (b) 模频率演化

    Figure 5.  Time evolution of the fishbone without fluid nonlinearity: (a) $ n = 1 $ kinetic energy; (b) mode frequency.

    图 6  动能和磁能的$ n = 1 $分量随时间演化

    Figure 6.  Time evolutions of $ n = 1 $ kinetic energy and magnetic energy.

    图 7  不同三角形变参数下的鱼骨模动能的$ n = 1 $分量的演化 (a) $ \beta_{{\rm{total}}, 0} = $$ 4.61 {\text{%}}$; (b) $ \beta_{{\rm{total}}, 0} = 3.91{\text{%}} $

    Figure 7.  The $ n = 1 $ kinetic energy evolution of the fishbone with different triangularity: (a) $ \beta_{{\rm{total}}, 0} = 4.61{\text{%}} $; (b) $ \beta_{{\rm{total}}, 0} = $$ 3.91{\text{%}} $.

    图 8  不同三角形变位形下的捕获高能量离子轨道 (a) $ \delta = $$ - 0.436 $, $ \beta_{{\rm{total}}, 0} = 3.91{\text{%}}$; (b) $ \delta = 0.436 $, $ \beta_{{\rm{total}}, 0} = 4.61{\text{%}} $

    Figure 8.  Orbits of trapped fast ions with different triangularity: (a) $ \delta = - 0.436 $, $ \beta_{{\rm{total}}, 0} = 3.91{\text{%}} $; (b) $ \delta = 0.436 $, $ \beta_{{\rm{total}}, 0} = $$ 4.61{\text{%}} $.

  • [1]

    Hofmann F, Sauter O, Reimerdes H, et al. 1998 Phys. Rev. Lett. 81 2918Google Scholar

    [2]

    Camenen Y, Pochelon A, Behn R, et al. 2007 Nucl. Fusion 47 510Google Scholar

    [3]

    Solomon W M, Snyder P B, Burrell K H, et al. 2014 Phys. Rev. Lett. 113 135001Google Scholar

    [4]

    Snyder P B, Solomon W M, Burrell K H, et al. 2015 Nucl. Fusion 55 083026Google Scholar

    [5]

    Reimerdes H, Pochelon A, Sauter O, et al. 2000 Plasma Phys. Control. Fusion 42 629Google Scholar

    [6]

    Marinoni A, Brunner S, Camenen Y, et al. 2009 Plasma Phys. Control. Fusion 51 055016Google Scholar

    [7]

    Austin M E, Marinoni A, Walker M L, et al. 2019 Phys. Rev. Lett. 122 115001Google Scholar

    [8]

    Medvedev S, Kikuchi M, Villard L, et al. 2015 Nucl. Fusion 55 063013Google Scholar

    [9]

    Chen W, Wang Z X 2020 Chin. Phys. Lett. 37 125001Google Scholar

    [10]

    McGuire K, Goldston R, Bell M, et al. 1983 Phys. Rev. Lett. 50 891Google Scholar

    [11]

    Chen L, White R B, Rosenbluth M N 1984 Phys. Rev. Lett. 52 1122Google Scholar

    [12]

    Coppi B, Porcelli F 1986 Phys. Rev. Lett. 57 2272Google Scholar

    [13]

    Heidbrink W W, Bol K, Buchenauer D, et al. 1986 Phys. Rev. Lett. 57 835Google Scholar

    [14]

    Heidbrink W W, Sager G 1990 Nucl. Fusion 30 1015Google Scholar

    [15]

    Nave M F F, Campbell D J, Joffrin E, et al. 1991 Nucl. Fusion 31 697Google Scholar

    [16]

    von Goeler S, Roquemore A L, Johnson L C, et al. 1996 Rev. Sci. Instrum 67 473Google Scholar

    [17]

    Kass T, Bosch H S, Hoenen F, et al. 1998 Nucl. Fusion 38 807Google Scholar

    [18]

    Chen W, Ding X T, Liu Y, et al. 2010 Nucl. Fusion 50 084008Google Scholar

    [19]

    Xu L Q, Zhang J Z, Chen K Y, et al. 2015 Phys. Plasmas 22 122510

    [20]

    Shi P W, Chen W, Duan X R 2021 Chin. Phys. Lett. 38 035202Google Scholar

    [21]

    Van Zeeland M A, Collins C S, Heidbrink W W, et al. 2019 Nucl. Fusion 59 086028Google Scholar

    [22]

    Park W, Belova E V, Fu G Y, et al. 1999 Phys. Plasmas 6 1796Google Scholar

    [23]

    Fu G Y, Park W, Strauss H R, et al. 2006 Phys. Plasmas 13 052517Google Scholar

    [24]

    Lang J Y, Fu G Y, Chen Y 2010 Phys. Plasmas 17 042309Google Scholar

    [25]

    Cai H S, Fu G Y 2012 Phys. Plasmas 19 072506Google Scholar

    [26]

    Shen W, Fu G Y, Sheng Z M, et al. 2014 Phys. Plasmas 21 092514Google Scholar

    [27]

    Shen W, Wang F, Fu G Y, et al. 2017 Nucl. Fusion 57 116035Google Scholar

    [28]

    Wang F, Fu G Y, Shen W 2017 Nucl. Fusion 57 016034Google Scholar

    [29]

    Wang F, Yu L M, Fu G Y, et al. 2017 Nucl. Fusion 57 056013Google Scholar

    [30]

    Ren Z Z, Wang F, Fu G Y, et al. 2017 Phys. Plasmas 24 052501Google Scholar

    [31]

    Ren Z Z, Fu G Y, Van Zeeland M A, et al. 2018 Phys. Plasmas 25 122504Google Scholar

    [32]

    Shen W, Porcelli F 2018 Nucl. Fusion 58 106035Google Scholar

    [33]

    Chen W, Zhu X L, Wang F, et al. 2019 Nucl. Fusion 59 096037Google Scholar

    [34]

    Shen W, Wang F, Fu G Y, et al. 2020 Nucl. Fusion 60 106016Google Scholar

    [35]

    Xu L Q, Shen W, Ren Z Z, et al. 2021 Nucl. Fusion 61 076005Google Scholar

    [36]

    Ren Z Z, Shen W, Li G Q, et al. 2022 AIP Advances 12 075318Google Scholar

    [37]

    Porcelli F 1991 Plasma Phys. Control. Fusion 33 1601Google Scholar

    [38]

    Wang X Q, Wang X G 2016 Nucl. Fusion 56 036024Google Scholar

    [39]

    Wang X Q, Wang X G 2017 Nucl. Fusion 57 016039Google Scholar

    [40]

    Eriksson H G, Wahlberg C 2002 Phys. Plasmas 9 1606Google Scholar

    [41]

    Martynov A, Graves J P, Sauter O 2005 Plasma Phys. Control. Fusion 47 1743Google Scholar

    [42]

    Bussac M N, Pellat R, Edery D, et al. 1975 Phys. Rev. Lett. 35 1638Google Scholar

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  • Abstract views:  1044
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  • Cited By: 0
Publishing process
  • Received Date:  23 April 2023
  • Accepted Date:  17 July 2023
  • Available Online:  19 August 2023
  • Published Online:  05 November 2023

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