Improved operating space of the ICRF system in ASDEX upgrade

ASDEX Upgrade Team, EUROfusion MST1 Team

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

7 Scopus citations

Abstract

Following the improvements of compatibility of ICRF system with the tungsten (W) wall in ASDEX Upgrade (AUG) by using the boron-coated limiters on the 2-strap ICRF antennas and the 3-strap antennas with the W-limiters, the ICRF operating space was further extended in 3 areas: power, phase control between the antennas and frequency range. The available ICRF power in AUG was increased by using an additional RF generator to feed the central straps of the 3-strap antennas which require a 1.5:1 or 2:1 power ratio between the central strap and the two outer straps (combined) to minimize the ICRF-specific W sources. This increases the total experimentally achievable launched ICRF power in the optimized configuration to ~ 5.7 MW. A new phase control system enabled phase-locked operation of all 4 AUG ICRF antennas. This allows a better control of the launched k|| spectrum which on its turn is modified when both neighboring antennas are active, as well as of the structure of the global RF field distribution within the AUG vessel. Measurements by the RF magnetic field (B-dot) probes show that the RF field distribution can indeed be significantly affected by the variation of the phasing between the ICRF antenna pairs. However, its effect on the core plasma and on the residual ICRF specific plasma-wall interactions is small, for the cases so far limited to the H-modes at medium plasma densities. The available frequency range was extended and now covers four discrete frequencies (f): 30.0, 36.5, 41.8 and 55.1 MHz. In addition to the standard hydrogen (H) minority in deuterium (D) on-axis heating scheme at the magnetic field (Bt) of 2.0, 2.5, 2.8 and 3.1 T, the RF frequency range allows the use of the 3-ion D-(3He)-H and 4He-(3He)-H heating schemes at Bt=2.5-3.1 T (f=30 MHz – off-axis and on-axis), on-axis 3ωc D heating at Bt=1.9 T (f=41.8 MHz) and at Bt=2.5 T (f=55.1 MHz) and 2ωc H heating at Bt=1.9T (f=55.1 MHz).

Original languageEnglish
Title of host publication23rd Topical Conference on Radiofrequency Power in Plasmas
EditorsPaul T. Bonoli, Robert I. Pinsker, Xiaojie Wang
PublisherAmerican Institute of Physics Inc.
ISBN (Electronic)9780735420137
DOIs
StatePublished - Sep 16 2020
Externally publishedYes
Event23rd Topical Conference on Radiofrequency Power in Plasmas - Hefei, China
Duration: May 14 2019May 17 2019

Publication series

NameAIP Conference Proceedings
Volume2254
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

Conference23rd Topical Conference on Radiofrequency Power in Plasmas
Country/TerritoryChina
CityHefei
Period05/14/1905/17/19

Bibliographical note

Publisher Copyright:
© 2020 American Institute of Physics Inc.. All rights reserved.

Fingerprint

Dive into the research topics of 'Improved operating space of the ICRF system in ASDEX upgrade'. Together they form a unique fingerprint.

Cite this