2D distributions of potential and density mean-values and oscillations in the ECRH and NBI plasmas at the TJ-II stellarator

dc.contributor.authorA V Melnikov, L G Eliseev
dc.contributor.authorJ M Barcala, A Cappa
dc.contributor.authorA A Chmyga, M A Drabinskiy
dc.contributor.authorC Hidalgo, P O Khabanov
dc.contributor.authorN K Kharchev, A S Kozachek
dc.contributor.authorM Liniers, D López-Bruna
dc.contributor.authorU Losada, S E Lysenko
dc.contributor.authorF Medina, A Molinero
dc.contributor.authorJ L De Pablos, I Pastor
dc.contributor.authorand TJ-II Team
dc.date.accessioned2026-01-21T13:58:50Z
dc.date.available2026-01-21T13:58:50Z
dc.date.issued2022-04-12
dc.description.abstract2D plasma potential ϕ distribution was measured in the electron cyclotron resonance heating (ECRH) and neutral beam injection (NBI) plasmas of the TJ-II stellarator with the heavy ion beam probe for the whole radial range and wide area of the poloidal angle, and supported by Langmuir probe data at the edge. The whole operation domain for the on-axis ECRH was explored ( = 0.45–0.8 ×1019 m−3, PEC = 220–470 kW), in addition, NBI plasmas with = 0.9–1.3 × 1019 m−3 and PNBI = 510 kW were studied. In ECRH plasmas the density ramp-up is accompanied by the evolution of the potential from the bell-like to the Mexican hat profile, while the density profiles were flat or slightly hollow. The potential has the positive peak at the centre, and LFS-HFS (low field—high field sides) and up-down symmetry. Equipotential lines are consistent with vacuum magnetic flux surfaces. In the high-density NBI scenario, the ϕ profile was fully negative with a minimum up to −300 V at the centre, while at low-density ECRH plasma, ϕ has a maximum up to +0.9 kV at the centre. Fluctuations of potential and density are stronger in low-density scenarios and not poloidally symmetric. At the mid-radius (area of the maximum density), root mean square (RMS) of fluctuations were up to ϕ ∼ 15 V at LFS vs ∼20 V at HFS; RMS ne ∼ 2% at LFS vs ∼3% at HFS. In the NBI plasmas with the density rise, the asymmetry decreases and finally vanishing at = 1.2 × 1019 m−3. 2D distribution of the NBI-induced Alfvén eigenmodes (AEs) shows asymmetric ballooning structure: contrary to broadband turbulence, AE-associated potential perturbation dominates in the LFS with a factor up to 1.7 respect to the HFS. The electrostatic mode, excited in ECRH plasmas by suprathermal electrons also shows asymmetric structures: density perturbation dominates in the top-bottom direction compared to LFS-HFS direction.es_ES
dc.description.sponsorshipThis work has been carried out within the framework of the EUROfusion Grant Agreement No. 633053. Kurchatov team was supported by Russian Science Foundation, Project 19-12-00312. A V M was partly supported by Competitiveness program of NRNU MEPhI.es_ES
dc.identifier.doi10.1088/1361-6587/ac5b4c
dc.identifier.urihttps://hdl.handle.net/20.500.14855/5549
dc.language.isoenges_ES
dc.rights.accessRightsopen accesses_ES
dc.subjectHIBPes_ES
dc.subjectTJIIes_ES
dc.title2D distributions of potential and density mean-values and oscillations in the ECRH and NBI plasmas at the TJ-II stellaratores_ES
dc.typejournal articlees_ES

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