Jul 2 – 6, 2018
Žofín Palace
Europe/Prague timezone

P4.1089 Gyrokinetic Simulation for Trapped Electron Mode during dominant electron heating in EAST Tokamak

Jul 5, 2018, 2:00 PM
2h
Mánes

Mánes

Speaker

Xianmei Zhang

Description

See the full Abstract at http://ocs.ciemat.es/EPS2018ABS/pdf/P4.1089.pdf Gyrokinetic Simulation for Trapped Electron Mode during dominant electron heating in EAST Tokamak X.M. Zhang1*, W.D. Chen1, E.B. Xue 1, L.M. Yu1, and the EAST Team2 1 Department of Physics, School of Science, East China University of Science and Technology, Shanghai 200237, China 2 Institute of Plasma Physics, Chinese Academy of sciences, Hefei 230031, China The mechanism and behavior of trapped electron mode (TEM) is very important to study confinement and transport during electron dominant heating in tokamak [1-3]. Simulations of TEM have been performed for some typical discharges with dominant electron heating by using gyro-kinetic simulation code GTC in EAST. Calculation results show that the ratio of electron temperature to ion temperature Te/Ti and logarithmic density gradient R/Ln are main factors of affecting on TEM linear growth rate 𝛾 rather than electron temperature Te individually and normalized electron ion temperature logarithmic gradient R/LTe. For safety factor q and magnetic shear 𝑠̂ , the dependences of TEM linear growth rate are complex with different 𝑠̂ value in the range of normalized minor radius  <0.6. When 𝑠̂ is larger than 0.5 within  <0.6, 𝛾 increases with q while decreases with 𝑠̂ , which is consistent with theoretical analysis by the reduced model. However, when 𝑠̂ is smaller than 0.5 within  <0.6, the opposite results are obtained, namely 𝛾 decreases with q while increases with 𝑠̂ . References: [1] Horton W. 1999 Rev. Mod. Phys. 71 735 [2] Ryter F et al. 2005 Phys. Rev. Lett. 95 085001 [3] Bonanomi N et al. 2015 Nucl. Fusion. 55 113016 [4] Xie H S et al. 2017 Phys. Rev. Lett. 118 095001 [5] Xiao Y et al. 2007 Phys. Plasmas. 14 055910 [6] Bravenec R V et al. 2013 Phys. Plasmas. 20 104506 [7] Anderson J et al. 2006 Plasma Phys. Contr. F. 48 651

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