title: Upgrade of Langmuir probe diagnostic in ITER-like tungsten mono-block divertor on experimental advanced superconducting tokamak.
abstract: In order to withstand rapid increase in particle and power impact onto the divertor and demonstrate the feasibility of the ITER design under long pulse operation, the upper divertor of the EAST tokamak has been upgraded to actively water-cooled, ITER-like tungsten mono-block structure since the 2014 campaign, which is the first attempt for ITER on the tokamak devices. Therefore, a new divertor Langmuir probe diagnostic system (DivLP) was designed and successfully upgraded on the tungsten divertor to obtain the plasma parameters in the divertor region such as electron temperature, electron density, particle and heat fluxes. More specifically, two identical triple probe arrays have been installed at two ports of different toroidal positions (112.5-deg separated toroidally), which can provide fundamental data to study the toroidal asymmetry of divertor power deposition and related 3-dimension (3D) physics, as induced by resonant magnetic perturbations, lower hybrid wave, and so on. The shape of graphite tip and fixed structure of the probe are designed according to the structure of the upper tungsten divertor. The ceramic support, small graphite tip, and proper connector installed make it possible to be successfully installed in the very narrow interval between the cassette body and tungsten mono-block, i.e., 13.5 mm. It was demonstrated during the 2014 and 2015 commissioning campaigns that the newly upgraded divertor Langmuir probe diagnostic system is successful. Representative experimental data are given and discussed for the DivLP measurements, then proving its availability and reliability.
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: J C
authors: JC
authors: Xu
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: L
authors: L
authors: Wang
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: G S
authors: GS
authors: Xu
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: G N
authors: GN
authors: Luo
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: D M
authors: DM
authors: Yao
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: Q
authors: Q
authors: Li
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: L
authors: L
authors: Cao
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: L
authors: L
authors: Chen
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: W
authors: W
authors: Zhang
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: S C
authors: SC
authors: Liu
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: H Q
authors: HQ
authors: Wang
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: M N
authors: MN
authors: Jia
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: W
authors: W
authors: Feng
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: G Z
authors: GZ
authors: Deng
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: L Q
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authors: Hu
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: B N
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authors: Wan
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: J
authors: J
authors: Li
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: Y W
authors: YW
authors: Sun
authors: Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031, China.
authors: H Y
authors: HY
authors: Guo