Topology of 2D turbulent structures based on intermittence in the TJII stellarator

dc.contributor.authorB.Ph. van Milligen1, A.V. Melnikov TJ-II Team
dc.contributor.authorB.A. Carreras, L. García
dc.contributor.authorA.S. Kozachek, C. Hidalgo
dc.contributor.authorJ.L. de Pablos, P.O. Khabanov
dc.contributor.authorL.G. Eliseev, M.A. Drabinskiy
dc.contributor.authorA. Chmyga, L. Krupnik
dc.contributor.authorHIBP Team, TJ-II Team
dc.date.accessioned2026-01-21T11:35:05Z
dc.date.available2026-01-21T11:35:05Z
dc.date.issued2021-10-14
dc.description.abstractThis work estimates the degree of turbulent intermittence of the plasma potential measured by a heavy ion beam probe in the core plasma region of the TJ-II stellarator. It is shown that the intermittence varies in a significant way with the plasma state (ion or electron root). In addition, radial minima of the intermittence are found to be associated with the location of topological structures of the flow associated with some important low-order rational surfaces. The local pressure gradient was also estimated, and a clear correlation was found between the steepening of the pressure gradient and the deepening of the minima of the intermittence, suggesting that the minima are associated with pressure gradient driven modes. By estimating the rotation velocity of the plasma from the measured plasma potential, it was possible to make a rough reconstruction of the two-dimensional radial–poloidal map of intermittence, thus clarifying the topological structure of the intermittence. The experimental results were put into context by comparing with simulations performed using a resistive magneto-hydrodynamic turbulence model.es_ES
dc.description.sponsorshiphis work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom Research and Training Program 2014–2018 and 2019–2020 under Grant Agreement No. 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission. Research sponsored in part by the Ministerio de Ciencia, Innovación y Universidades of Spain under Project Nos. PGC2018-097279-B-I00 and PID2019-110734RB-I00. The work of the Kurchatov team was funded by the Russian Science Foundation under Project 19-12-00312 and the work of A.V. Melnikov was partly supported by the Competitiveness program of NRNU MEPhI. BAC gratefully acknowledges support for the research from the DOE office of Fusion Energy under US Department of Energy Contract DE-SC0018076es_ES
dc.identifier.doihttps://doi.org/10.1088/1741-4326/ac27c9
dc.identifier.urihttps://hdl.handle.net/20.500.14855/5545
dc.language.isoenges_ES
dc.rights.accessRightsopen accesses_ES
dc.subjectturbulencees_ES
dc.subjectstellaratores_ES
dc.subjectintermittencees_ES
dc.titleTopology of 2D turbulent structures based on intermittence in the TJII stellaratores_ES
dc.typejournal articlees_ES

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