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

P4.1010 New Diagnostics Developments on IShTAR

Jul 5, 2018, 2:00 PM
2h
Mánes

Mánes

Speaker

Kristel Crombe

Description

See the full Abstract at http://ocs.ciemat.es/EPS2018ABS/pdf/P4.1010.pdf New Diagnostics Developments on IShTAR K. Crombé1, 2, A. Kostic1, 3, A. Nikiforov1, R. Ochoukov3, I. Shesterikov3, M. Usoltceva1, 2, 3, T. Verstrynge1, H. Faugel3, H. Fünfgelder3, S. Heuraux4, J-M. Noterdaeme1, 3 and the IShTAR team 1 Department of Applied Physics, Ghent University, 9000 Ghent, Belgium 2 LPP-ERM-KMS, TEC partner, 1000 Brussels, Belgium 3 Max-Planck-Institut für Plasmaphysik, 85748 Garching, Germany 4 Université de Lorraine, 54506 Vandœuvre-lès-Nancy, France The diagnostics developed for IShTAR (Ion Cyclotron Sheath Test ARrangement) are oriented towards measurements of plasma parameters and electric fields in the vicinity of a Radio Frequency (RF) antenna in order to provide input for sheath modelling codes [1, 2]. In IShTAR the plasmas are created with a helicon antenna operated at a frequency of 11.76 MHz and with a power up to 3kW (the maximum power coupled to the plasma is around 2.7 kW). Recent improvements have been made for the density measurements in the helicon source and the main vessel. An optimised performance regime was found; by adjusting the magnetic topology the plasmas density can be increased by a factor 3 to 5, which is beneficial to the sheath studies. An additional array of RF compensated probes (Langmuir, B-dot…) has been installed to allow for a better characterization of the plasma parameters at different locations. The first results of an interferometer, installed to benchmark the electron density estimates of the Langmuir probes, will be presented. Two approaches are followed to measure the electric fields in the plasma caused by the RF antenna sheaths. Passive optical emission spectroscopy monitors Stark effects on spectral lines with a high-resolution spectrometer [3], provided that the local electric fields are strong enough to overcome the broadening of the lines. Doppler-free saturation spectroscopy is more powerful: a laser beam depletes the ground state, eliminates the line broadening effects and makes smaller electric fields visible. However, the more complicated set-up, with a careful alignment of laser beams, makes the measurements much more challenging. After a first test on a glow discharge plasma [4], the design of the optical path and the installation of the laser at IShTAR have started; the progress will be reported. This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 under grant agreement No 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission. The work received support from the Research Foundation Flanders (G0B3115N). [1] K. Crombé et al., “IShTAR: a helicon plasma source to characterize the interactions between ICRF and plasma”, 26th IAEA Fusion Energy Conference (2016), EXP6_48 [2] L. Lu et al., “Modelling of radio frequency sheath and fast wave coupling on the realistic ion cyclotron resonant antenna surroundings and the outer wall”, Plasma Phys. Control. Fusion, Vol. 60, No. 3, 035003 (2018) [3] A. Kostic et al.: "Feasibility study of Passive Optical Emission Spectroscopy for the electric field measurements in IShTAR”, EPJ Web of Conferences 157, 03025 (2017) [4] K. Crombé et al.: “Helium operation of IShTAR in preparation of E-field measurements”, ECA Vol. 41F, P5- 144 (2017)

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