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

P5.1077 Quasi-continuous low frequency edge fluctuations in the W7-X stellarator

Jul 6, 2018, 2:00 PM
2h
Mánes

Mánes

Speaker

Glen Anthony Wurden

Description

See the full Abstract at http://ocs.ciemat.es/EPS2018ABS/pdf/P5.1077.pdf Quasi-continuous low frequency edge fluctuations in the W7-X stellarator G. A. Wurden1, S. Bozhenkov2, C. Brandt2, B. Buttenschoen2, M. Endler2, S. Freundt2, K. Hammond2, M. Hirsch2, U. Hoefel2, G. Kocsis3, P. Kornejew2, M. Krychowiak2, S. Lazerson4, K. Rahbarnia2, L. Rudischhauser2, T. Szepesi3, V. Winters5, and the W7-X Team 1 Los Alamos National Laboratory, Los Alamos, USA 2 Max Planck Institute for Plasma Physics, Greifswald, Germany 3 Wigner Research Centre for Physics, Budapest, Hungary 4 Princeton Plasma Physics Laboratory, Princeton, USA 5 University of Wisconsin, Madison, USA We have observed quasi-continuous low frequency (150-400 Hz) n=0 edge oscillations via multiple diagnostics in Wendelstein 7-X for some magnetic configurations. These events appear to originate at mid-radius, losing energy outwards to the walls, while a weak cold wave propagates towards the core. They are characterized by easily observable decreases in plasma kinetic energy (via diamagnetic loops) and simultaneous large (∆I/I = 300%) transient plasma current increases, albeit on a small net plasma current (<1kA). Core and edge responses occurs after the initial (~1-3%) global energy drop on each event. Fast cameras and segmented Rogowski diagnostics show an overall m=0 edge brightening, while electron cyclotron emission show an electron temperature fluctuation inversion point at mid-to-outer-radii. Using fiber filterscopes at multiple toroidal locations, the n=0 nature of the edge response (H-alpha, Carbon-III emission) is determined. Langmuir probes in the divertor show an edge density increase with each burst. These events are especially visible in so-called “high iota” discharges, when iota-bar is nearly 1 in the core, rising to 5/4 at the edge. Their magnitude is larger with higher input power, and their frequency is increased at higher plasma density. Their associated sawtooth-like energy loss, integrated over one energy confinement time, accounts for ~30% of the total energy loss.

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