Wall conditioning by ECRH discharges and He-GDC in the limiter phase of Wendelstein 7-X

T. Wauters, R. Brakel, S. Brezinsek, A. Dinklage, A. Goriaev, H. P. Laqua, S. Marsen, D. Moseev, T. Stange, G. Schlisio, T. Sunn Pedersen, O. Volzke, U. Wenzel

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Résumé

Wendelstein 7-X (W7-X) relies on wall conditioning to control the density and the impurity content of the plasma. Wall conditioning in the first operation campaign of W7-X consisted of baking at 150 °C during 1 week prior to operation, glow discharge conditioning (GDC) in helium (He) and electron cyclotron resonance heating (ECRH) discharges. Additionally, the usage of He-GDC was limited to avoid sputtering and migration of metallic plasma facing components. This presented a unique opportunity for studying the applicability of ECRH discharges for initial wall conditioning on a stellarator, albeit in the carbon limiter configuration. A single envelope curve is observed in the normalised outgassing data that takes into account all ECRH discharges. This illustrates that the majority of discharges operates at the limits of a radiative collapse. Hydrogen recycling dominated the fuelling of ECRH discharges throughout while CO outgassing was found strongest at the start of the campaign. A reduction of recycling was observed throughout the campaign. Temporarily depleting the walls from H and impurities was possible by He-GDC. It was shown that the recycling coefficient in H2-ECRH plasmas could be reduced and the pulse duration significantly extended by He-recovery ECRH plasmas. Good wall conditions were defined by normalised outgassing values below 1 × 10-9 mbar kJ-1. In absence of H2-GDC, more than 311 cumulated discharge seconds of ECRH discharges are needed for obtaining lasting low outgassing levels. A release model with two trapping reservoirs could reproduce the normalised outgassing trend, including ECRH and GDC plasma wall interactions.

langue originaleAnglais
Numéro d'article066013
journalNuclear Fusion
Volume58
Numéro de publication6
Les DOIs
étatPublié - 20 avr. 2018

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