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重杂质(如钨)聚芯是未来托卡马克反应堆中等离子体高性能运行所面临的严峻挑战. 开展多流体及动力学模拟以研究氖杂质注入条件下, 东方超环EAST托卡马克中等离子体高约束时的钨杂质边界输运特性. 结果表明, 低电离态钨离子主要聚集在碰撞率较高的偏滤器区域, 流体近似可很好地满足; 高电离态钨离子密度相对较低且主要位于碰撞率相对较低的芯部, 多流体与动力学模拟结果差异显著; 但二者计算的钨杂质总密度差异较小(< 30%). 多流体模拟中, 除将钨离子考虑为74种流体外, 还将电离能接近的钨离子进行价态捆绑. 比较发现, 价态捆绑可显著降低计算成本, 但在高再循环(或部分脱靶)运行机制下可显著高估(低估)偏滤器区域等离子体温度(密度), 从而大幅低估钨电离源及钨密度, 其根源在于价态捆绑对钨离子平均电离态和偏滤器区域辐射功率损失的显著影响. 模拟结果还表明, 氖杂质注入促进偏滤器脱靶可有效缓解钨杂质聚芯.Accumulation of tungsten (W) in core is a serious challenge for achieving high-performance plasmas in future tokamak reactors, thus W impurity transport is a highly concerned topic in the tokamak physics researches. Multi-fluid model and kinetic model are the numerical tools widely used for investigating and/or predicting impurity behaviors in the boundary of tokamak plasma. Generally, the applicability of multi-fluid model for impurity transport modeling requires that the collision mean-free-path should be smaller than the gradient scale lengths of particles, which may not be always satisfied. It is performed and comparatively investigated to evaluate the applicability of multi-fluid model for W impurity transport modeling, multi-fluid (SOLPS-ITER) modeling and kinetic (DIVIMP) modeling of W impurity transport in the edge of high-confinement plasma in Experimental Advanced Superconducting Tokamak (EAST) during neon impurity seeding. It is found that low-charge-state W ions are mainly located in the divertor region near the target plate where plasma collisionality is relatively high due to the relatively low/high local plasma temperature/density. Hence, the fluid assumption for transport of lowly-charged W ions can be well satisfied. Consequently, the density of lowly-charged W ions predicted by SOLPS-ITER and that calculated by DIVIMP are almost similar. Owing to the fact that the density of highly-charged W ions is relatively low and these particles mainly exist in the upstream (e.g. the main SOL and core) where plasma collisionality is relatively low, the fluid approximation cannot be well satisfied. However, the total W impurity density calculated by the kinetic code DIVIMP and the multi-fluid model SOLPS-ITER are found to be in agreement with each other within a factor of 1.5 for the simulation cases presented in this contribution. Besides, the multi-fluid simulation with bundled charge state model has also been performed, the obtained results are compared with those from the multi-fluid modeling with W ions treated as 74 fluids. It is revealed that in simulation cases with neon impurity seeding and with divertor plasmas in high-recycling or partially detached regimes, the bundling scheme, which is commonly used for saving the computation cost in multi-fluid modeling, tends to overestimate the average charge state of W ions and thus tends to underestimate the radiation power loss, especially in the divertor region. Consequently, under the circumstance that W impurity radiation dominates the radiative power loss in divertor region, plasma temperature/density can be largely overestimated/underestimated, leading to the underestimation of W ion ionization source and W impurity density. Moreover, simulation results demonstrate that W accumulation in core can decrease effectively during divertor detachment promoted by neon seeding.
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Keywords:
- tokamak /
- tungsten impurity /
- multi-fluid model /
- kinetic modeling
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图 3 SOLPS-ITER采用不同钨离子流体方案(蓝色代表方案1, 即74种流体; 红色代表方案2, —价态捆绑减为23种流体)计算所得外中平面处等离子体密度(a)和温度(b)的径向分布
Fig. 3. Radial profiles of plasma density (a) and temperature (b) at the outer mid-plane calculated by SOLPS-ITER using the full-charge-states (blue, 74 fluids) and bundled-charge-states (red, 23 fluids) fluid models.
图 5 不同模型计算得到的钨杂质密度二维分布 (a) 流体模型(SOLPS-ITER)将钨离子看作74种流体; (b) 流体模型(SOLPS-ITER)将部分价态钨离子捆绑(bundled) ; (c) 动力学模型(DIVIMP)
Fig. 5. Two-dimensional distribution of tungsten impurity density calculated by different models: (a) SOLPS-ITER using full-charge-states fluid model; (b) SOLPS-ITER using bundled-charge-states model; (c) DIVIMP.
图 6 不同模型计算所得钨杂质沿(a)内偏滤器靶板、(b)外偏滤器靶板、(c)中平面等处的径向分布, (d)及其在刮削层中第一个磁通管上的极向分布(横轴为距外靶板的极向距离). 注意: 图6(d)纵轴为对数坐标
Fig. 6. Calculated radial profiles of tungsten impurity density at the inner/outer target plate (a)/(b) and outer mid-plane (c) together with the poloidal profile of tungsten impurity density along the flux surface in the SOL near the separatrix (d). It is notable that the vertical axis is logarithmically scaled in panel (d).
图 8 SOLPS-ITER和DIVIMP计算所得不同价态钨杂质离子密度沿磁面的极向分布 (a) W1+—W10+; (b) W11+—W15+; (c) W16+—W20+; (d) W21+—W74+. 图中横轴为到外靶板的极向距离
Fig. 8. Poloidal profiles for W ions at different charge states calculated by SOLPS-ITER and DIVIMP: (a) W1+—W10+; (b) W11+—W15+; (c) W16+—W20+; (d) W21+—W74+. The vertical coordinates represent the poloidal distance from the outer target measured in the upstream direction.
表 1 SOLPS-ITER采用不同流体方案计算所得+1价钨离子(W1+)电离源在外偏滤器区域(OD)、内偏滤器区域(ID)、刮削层(SOL)及芯部(core)的强度(单位: 1019 s–1)
Table 1. Strength of W1+ ionization source from neutrals in the outer divertor (OD), inner divertor (ID), scrape-off layer (SOL) and core calculated by SOLPS-ITER using different fluid models (in 1019 s–1).
Fluid models OD ID SOL Core Total Bundled-charge-states 9.31 0.93 0.002 $ \sim 0 $ 10.2 Full-charge-states 38.7 10.2 0.04 $ \sim 0 $ 48.9 表 2 SOLPS-ITER采用不同流体模型计算所得不同离子在内/外靶板(IT/OT)的通量及靶板总通量(单位: s–1)
Table 2. Total target fluxes of deuterium (D), neon (Ne) and tungsten (W) together with the D, Ne and W ion fluxes at the inner/outer divertor target (IT/OT) (in s–1), calculated by SOLPS-ITER.
Fluid model Species OT/1019 IT/1018 Total/1020 Bundled-charge-states D 2280 26500 493 Ne 7.46 43.2 1.18 W 9.26 9.20 1.02 Full-charge-states D 2360 24800 484 Ne 6.13 44.7 1.06 W 37.8 98.7 4.76 表 3 SOLPS-ITER采用不同流体模型计算所得氘(D)、氖(Ne)以及钨(W)辐射功率损失在内偏滤器区域(ID)、外偏滤器区域(OD)、刮削层(SOL)及芯部(Core)的分布(单位: kW)
Table 3. Contributions of deuterium (D), neon (Ne) and tungsten (W) to radiation power loss in the inner/outer divertor region (ID/OD), scrape-off layer (SOL) and core calculated by SOLPS-ITER using the full-charge-states model and bundled-charge-states model (in kW).
Fluid model ID OD SOL Core Total Bundled-charge-states D 20.76 25.03 13.59 1.75 61.13 Ne 23.56 26.50 73.57 89.08 212.71 W 46.07 31.07 10.08 1.28 88.50 Full-charge-states D 21.59 26.54 14.10 1.72 63.95 Ne 28.51 28.81 79.43 94.10 230.85 W 386.26 237.45 32.11 6.69 662.51 -
[1] Ye D W, Ding F, Li K D, Hu Z H, Zhang L, Chen X H, Zhang Q, Zhao P A, He T, Meng L Y, Ye K X, Zhong F B, Duan Y M, Ding R, Wang L, Xu G S, Luo G N, EAST team 2022 Chin. Phys. B 31 065201Google Scholar
[2] Wang F Q, Zha X J, Duan Y M, Mao S T, Wang L, Zhong F C, Liang L, Li L, Lu H W, Hu L Q, Chen Y P, Yang Z D 2018 Plasma Phys. Control. Fusion 60 125005Google Scholar
[3] Yamoto S, Bonnin, X, Homma Y, Inoue H, Hoshino K, Hatayama A, Pitts RA 2017 Nucl. Fusion 57 116051Google Scholar
[4] Kirschner A, Tskhakaya D, Brezinsek S, Borodin D, Romazanov J, Ding R, Eksaeva A, Linsmeier C 2018 Plasma Phys. Control. Fusion 60 014041Google Scholar
[5] Shi S Y, Chen J L, Bourdelle C, Jian X, Odstrcil T, Garofalo A M, Cheng Y X, Chao Y, Zhang L, Duan Y M, Wu M Q, Ding F, Li Y Y, Huang J, Qian J P, Gao X, Wan Y X 2022 Nucl. Fusion 62 066031Google Scholar
[6] Putterich T, Dux R, Neu R, Bernert M, Beurskens M N A, Bobkov V, Brezinsek S, Challis C, Coenen J W, Coffey I, Czarnecka A, Giroud C, Jacquet P, Joffrin E, Kallenbach A, Lehnen M, Lerche E, de la Luna E, Marsen S, Matthews G, Mayoral M L, McDermott R M, Meigs A, Mlynar J, Sertoli M, van Rooij G 2013 Plasma Phys. Control. Fusion 55 124036Google Scholar
[7] Robert A 1997 IEEE Trans. Plasma Sci. 25 1187Google Scholar
[8] Motojima O 2015 Nucl. Fusion 55 104023Google Scholar
[9] Hinnov E, Mattioli M 1978 Phys. Lett. A 66 109Google Scholar
[10] Isler R, Neidigh R, Cowan R 1977 Phys. Lett. A 63 295Google Scholar
[11] Neu R, Dux R, Geier A, Greuner H, Krieger K, Maier H, Pugno R, Rohde V, Yoon S W 2003 J. Nucl. Mater. 313–316 116
[12] Zhang L, Morita S, Xu Z, Zhang P F, Zang Q, Duan Y M, Liu H Q, Zhao H L, Ding F, Ohishi T, Gao W, Huang J, Yang X D, Chen Y J, Wu Z W, Xu P, Ding B J, Hu C D, Gong X Z, Chen J L, Hu L Q 2017 Nucl. Mater. Energy 12 774Google Scholar
[13] Wagner F, Becker G, Behringer K, Campbell D, Eberhagen A, Engelhardt W, Fussmann G, Gehre O, Gernhardt J, Vongierke G, Haas G, Huang M, Karger F, Keilhacker M, Klüber O, Kornherr M, Lackner K, Lisitano G, Lister G G, Mayer H M, Meisel D, Müller E R, Murmann H, Niedermeyer H, Poschenrieder W, Rapp H, Röhr H, Schneider F, Siller G, Speth E, Stäbler A, Steuer K H, Venus G, Vollmer O, Yü Z 1982 Phys. Rev. Lett. 49 1408Google Scholar
[14] 杜海龙, 桑超峰, 王亮, 孙继忠, 刘少承, 汪惠乾, 张凌, 郭后扬, 王德真 2013 62 245206Google Scholar
Du H L, Sang C F, Wang L, Sun J Z, Liu S C, Wang H Q, Zhang L, Guo H Y, Wang D Z 2013 Acta Phys. Sin. 62 245206Google Scholar
[15] Dux R, Peeters A G, Gude A, Kallenbach A, Neu R, ASDEX Upgrade Team 1999 Nucl. Fusion 39 1509Google Scholar
[16] 张文敏, 张凌, 程云鑫, 王正汹, 胡爱兰, 段艳敏, 周天富, 刘海庆 2022 71 115203Google Scholar
Zhang W M, Zhang L, Cheng Y X, Wang Z X, Hu A L, Duan Y M, Zhou T F, Liu H Q 2022 Acta Phys. Sin. 71 115203Google Scholar
[17] 沈勇, 董家齐, 徐红兵 2018 67 195203Google Scholar
Shen Y, Dong J Q, Xu H B 2018 Acta Phys. Sin. 67 195203Google Scholar
[18] Ciraolo G, Di Genova S, Yang H, Gallo A, Fedorczak N, Bufferand H, Gunn J P, Tamain P, Guirlet R, Guillemaut C, Desgranges C, Bourdelle C, Tsitrone E, Bucalossi J, D'Abusco M S, Serre E, Marandet Y, Raghunathan M, Sepetys A, Romazanov J, Kirschner A, Brezinsek S 2021 Nucl. Fusion 61 126015Google Scholar
[19] Geier A, Krieger K, Elder J D, Pugno R, Rohde V 2003 J. Nucl. Mater. 313–316 1216
[20] Lim K, Garbet X, Sarazin Y, Grandgirard V, Obrejan K, Lesur M, Gravier E 2021 Nucl. Fusion 61 046037Google Scholar
[21] van Vugt D C, Huijsmans G T A, Hoelzl M, Loarte A 2019 Phys. Plasmas 26 042508Google Scholar
[22] Sinclair G, Maurizio R, Ma X, Abrams T, Elder J D, Guo H Y, Thomas D M, Leonard A W 2022 Nucl. Fusion 62 106024Google Scholar
[23] Sang C F, Zhou Q R, Xu G S, Wang L, Wang Y L, Zhao X L, Zhang C, Ding R, Jia G Z, Yao D M, Liu X J, Si H, Wang D Z 2021 Nucl. Fusion 61 066004Google Scholar
[24] Schmid K, Krieger K, Kukushkin A, Loarte A 2007 J. Nucl. Mater. 363–365 674
[25] Wiesen S, Reiter D, Kotov V, Baelmans M, Dekeyser W, Kukushkin A S, Lisgo S W, Pitts R A, Rozhansky V, Saibene G, Veselova I, Voskoboynikov S 2015 J. Nucl. Mater. 463 480Google Scholar
[26] Bonnin X, Dekeyser W, Pitts R, Coster D, Voskoboynikov S, Wiesen S 2016 Plasma Fusion Res. 11 1403102Google Scholar
[27] Strachan J D, Corrigan G, Harting D, Lauro-Taroni L, Maggi C F, Matthews G F, O'Mullane M, Reiter D, Seebacher J, Spence J, Summers H, Wiesen S 2011 J. Nucl. Mater. 415 S501Google Scholar
[28] Harting D, Groth M, Beurskens M, Boerner P, Brix M, Coenen J W, Corrigan G, Lehnen M, Marsen S, van Rooij G, Reiter D, Wiesen S 2013 J. Nucl. Mater. 438 S480Google Scholar
[29] Stangeby P C, Elder J D 1995 Nucl. Fusion 35 1391Google Scholar
[30] Yamoto S, Homma Y, Hoshino K, Toma M, Hatayama A 2020 Comput. Phys. Commun. 248 106979Google Scholar
[31] Wang J, Chen Y P, Wang L, Gao W, Wu Z W, Zhang L 2023 Phys. Plasmas 30 043905Google Scholar
[32] Song Y T, Wan B N, Gong X Z, et al. 2022 IEEE Trans. Plasma Sci. 50 4330Google Scholar
[33] Wang F Q, Liang Y, Zha X J, Zhong F C, Mao S T, Duan Y M, Hu L Q, Wang L, Liu J B, Yan N, Liu S C 2022 Nucl. Fusion 62 056021Google Scholar
[34] Pan O, Bernert M, Lunt T, Cavedon M, Kurzan B, Wiesen S, Wischmeier M, Stroth U 2023 Nucl. Fusion 63 016001Google Scholar
[35] Kaveeva E, Rozhansky V, Veselova I, Senichenkov I, Giroud C, Pitts R A, Wiesen S, Voskoboynikov S 2021 Nucl. Mater. Energy 28 101030Google Scholar
[36] Koenders J T W, Wensing M, Ravensbergen T, Fevrier O, Perek A, van Berkel M 2022 Nucl. Fusion 62 066025Google Scholar
[37] Kaveeva E, Rozhansky V, Senichenkov I, Sytova E, Veselova I, Voskoboynikov S, Bonnin X, Pitts R A, Kukushkin A S, Wiesen S, Coster D 2020 Nucl. Fusion 60 046019Google Scholar
[38] Senichenkov I Y, Ding R, Molchanov P A, Kaveeva E G, Rozhansky V A, Voskoboynikov S P, Shtyrkhunov N V, Makarov S O, Si H, Liu X, Sang C, Mao S 2022 Nucl. Fusion 62 096010Google Scholar
[39] Kumpulainen H A, Groth M, Fontell M, Jaervinen A E, Corrigan G, Harting D 2020 Nucl. Mater. Energy 25 100784Google Scholar
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