Impact of ICRF fast-ions on core turbulence and MHD activity in ASDEX upgrade

A. Bilato, C. Angioni, A. Bañón Navarro, V. Bobkov, T. Bosman, A. Di Siena, E. Fable, R. Fischer, J. Galdon-Quiroga, T. Görler, J. Hidalgo-Salaverri, F. Jenko, T. Johnson, Ye O. Kazakov, O. Kudlacek, J. Manyer, M. Mantsinen, R. Ochoukov, E. Poli, J. Rueda-RuedaP. A. Schneider, S. Sipilä, W. Tierens, M. Usoltseva, M. Weiland

Research output: Contribution to journalConference articlepeer-review

4 Scopus citations

Abstract

Experiments in various tokamaks and their analysis identify the fast ions (FI) generated by NBI and/or ICRF heating as one of the main causes of the observed improvement in core confinement: fast ions can reduce core microturbulence (mainly Ion-Temperature-Gradient (ITG) driven modes) either electrostatically or electromagnetically, or they can resonate with fishbones and high-frequency Alfvén modes, which in turn contribute in stabilizing ITG. In this perspective, we discuss recent experiments done on ASDEX Upgrade (AUG) where ICRF is the main actuator for FI generation for energies above 100 keV. Additionally, ICRF-FIs can substantially impact the MHD activity and its consequent effects on fast ion losses (FILs) and ion-cyclotron emission (ICE). We present dedicated AUG experiments with NBI-D further accelerated by ICRF.

Original languageEnglish
Article number030010
JournalAIP Conference Proceedings
Volume2984
Issue number1
DOIs
StatePublished - Aug 18 2023
Externally publishedYes
Event24th Topical Conference on Radio-frequency Power in Plasmas - Annapolis, United States
Duration: Sep 26 2022Sep 28 2022

Funding

This work has been carried out within the framework of the EUROfusion Consortium, funded by the European Union via the Euratom Research and Training Programme (Grant Agreement No 101052200 — EUROfusion). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Commission. Neither the European Union nor the European Commission can be held responsible for them. We wish to acknowledge M. Bergmann, M. Brambilla, P. David, R. Mc Dermott, Ph. Lauber, U. Plank, M. Reisner, S. Sharapov, G. Staebler, G. Tardini, E. Viezzer, B. Zimmermann, and to thank A. Kappatou, E. Tsitrone and A. Hakola for their kind support. J. Galdon-Quiroga acknowledges funding from the Spanish Ministry of Science and Innovation under grant no. FJC2019-041092-I. See the author list of U. Stroth et al. 2022 Nucl. Fusion 62 042006 for the ASDEX Upgrade Team; see the author list of B. Labit et al. 2019 Nucl. Fusion 59 086020 for the EUROfusion MST1 team.

FundersFunder number
European Commission101052200 — EUROfusion
Ministerio de Ciencia e InnovaciónFJC2019-041092-I

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