Study on impurity hole plasmas by global neoclassical simulation

被引:12
|
作者
Fujita, Keiji [1 ]
Satake, S. [1 ,2 ]
Nunami, M. [1 ,2 ]
Garcia-Regana, J. M. [3 ]
Velasco, J. L. [3 ]
Calvo, I. [3 ]
机构
[1] Grad Univ Adv Studies SOKENDAI, 322-6 Oroshi Cho, Toki, Gifu, Japan
[2] Natl Inst Fus Sci, 322-6 Oroshi Cho, Toki, Gifu, Japan
[3] CIEMAT, Lab Nacl Fus, Ave Complutense 40, Madrid 28040, Spain
关键词
plasma confinement; neoclassical transport; impurity transport; stellarators; AMBIPOLAR ELECTRIC-FIELD; TRANSPORT; STELLARATORS; TRANSITION; EQUATION;
D O I
10.1088/1741-4326/ac0e72
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
An impurity hole observed in the large helical device (LHD) is a hollow density profile of an impurity ion species formed in the core plasma where the negative (inward-pointing) ambipolar radial electric field (E (r)) exists. Although local neoclassical models have predicted that the sign of E (r) in impurity hole plasmas is negative for the entire minor radius, an experimental measurement of an impurity hole plasma has shown that the E (r) changes the sign from negative to positive along the minor radius. In the present work, we investigate neoclassical impurity transport in an impurity hole plasma using a global neoclassical simulation code FORTEC-3D. The variation of electrostatic potential on each flux surface (phi(1)) is evaluated from the quasi-neutrality condition in multi-ion-species plasma by the global simulation. The ambipolar E (r) and neoclassical fluxes are determined in solving a global drift-kinetic equation including the effect of phi(1). By the global simulation, we show that an E (r) which changes the sign along the radius is obtained as a solution of the ambipolar condition and with such an E (r), impurity carbon flux can be outwardly directed even where E (r) < 0 and the carbon density profile is hollow around the magnetic axis. Furthermore, it is found that the outward carbon flux is only a factor 2-3 from balancing the modeled inward turbulent flux. Our result indicates that we have moved one step closer to reproducing the impurity transport in impurity hole plasmas by kinetic simulation.
引用
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页数:15
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