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

P5.1084 Ion cyclotron emission properties in NBI-heated TUMAN-3M plasma

Jul 6, 2018, 2:00 PM
2h
Mánes

Mánes

Speaker

Leonid Askinazi

Description

See the full Abstract at http://ocs.ciemat.es/EPS2018ABS/pdf/P5.1084.pdf Ion cyclotron emission properties in NBI-heated TUMAN-3M plasma L.G. Askinazi, G.I.Abdullina, A.A. Belokurov, V.A. Kornev, S.V. Krikunov, S.V. Lebedev, D.V. Razumenko, A.I. Smirnov, A.S. Tukachinsky, N.A. Zhubr Ioffe Institute, St. Petersburg, Russian Federation Ion cyclotron emission (ICE) in routinely registered in many tokamaks. It was recently observed in the TUMAN-3M tokamak [1, 2] in ohmically and neutral beam injection (NBI)- heated regimes in D and H plasma. This presentation describes some characteristic features of NBI-induced ICE observed in TUMAN-3M, with emphasis on spectral structure of the emission. In contrast to many other observations, ICE frequency ωICE in the TUMAN-3M NBI scenario corresponds to a core location of a radiating body, close to the plasma center. In NBI-heated plasma, ICE generation is usually explained by the presence of fast particles (beam ions or fusion charged products) with high transversal kinetic energy. In the TUMAN- 3M, high energy charged fusion products are not confined due to the low toroidal field (BT=1 T) and small size (R/a = 0.55 m / 0.25 m) of the tokamak and could not effectively excite ICE. NBI in the TUMAN-3M is performed in co-current tangential direction; as a result the fast ions with high transversal energy are born predominantly in the plasma periphery and then move to the core plasma along drift trajectories. Among these trajectories, a class of potato- like ones features the strong deviation from magnetic surface. This kind of trajectories looks beneficial for central ICE generation, as they have long vertical part located close to plasma center; particle drifting along this vertical part spends a longer time in a region of constant toroidal field, i.e. constant ωICE. Thus, these particles could be a possible candidate for central NBI ICE excitation in the TUMAN-3M. This model reproduces qualitatively well other important features of NBI ICE observed in the deuterium plasma in TUMAN-3M, such as frequency line splitting (fine structure) and ICE frequency dependence on beam energy. The former is explained by the presence of different energy components (1/2E0, 1/3E0 etc ) in the beam, in addition to main energy E0; the latter ensues from (a weak) dependence of location of vertical part of the trajectory on the fast ion’s energy. Experimental study of the ICE was supported by Russian Science Foundation (Project # 16-12-10285). Modeling of the fast ion trajectories was supported by Ioffe Institute. References 1. Lebedev S.V. et al, EPJ Web of Conferences 149, 03010 (2017), https://doi.org/10.1051/epjconf/201714903010 2. L.G.Askinazi et al, 15th IAEA TM on Energetic Particles in Magnetic Confinement Systems, 5-8 Sept. 2017, Princeton, P2. https://nucleus.iaea.org/sites/fusionportal/Shared%20Documents/EP%2017th/BoA.pdf

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