Comparison of tungsten nano-tendrils grown in Alcator C-Mod and linear plasma devices

Growth of tungsten nano-tendrils (“fuzz”) has been observed for the first time in the divertor region of a high-power density tokamak experiment. After 14 consecutive helium L-mode discharges in Alcator C-Mod, the tip of a tungsten Langmuir probe at the outer strike point was fully covered with a la...

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Bibliographic Details
Main Authors: Bystrov, K., De Temmerman, G., Wright, Graham, Brunner, Daniel Frederic, Labombard, Brian, Lipschultz, Bruce, Woller, Kevin Benjamin, Baldwin, M. J., Doerner, R. P., Terry, James L, Whyte, Dennis G
Other Authors: Massachusetts Institute of Technology. Department of Nuclear Science and Engineering
Format: Article
Language:en_US
Published: Elsevier 2015
Online Access:http://hdl.handle.net/1721.1/99468
https://orcid.org/0000-0002-9001-5606
https://orcid.org/0000-0002-8753-1124
https://orcid.org/0000-0002-7841-9261
https://orcid.org/0000-0002-0450-9731
Description
Summary:Growth of tungsten nano-tendrils (“fuzz”) has been observed for the first time in the divertor region of a high-power density tokamak experiment. After 14 consecutive helium L-mode discharges in Alcator C-Mod, the tip of a tungsten Langmuir probe at the outer strike point was fully covered with a layer of nano-tendrils. The depth of the W fuzz layer (600 ± 150 nm) is consistent with an empirical growth formula from the PISCES experiment. Re-creating the C-Mod exposures as closely as possible in Pilot-PSI experiment can produce nearly-identical nano-tendril morphology and layer thickness at surface temperatures that agree with uncertainties with the C-Mod W probe temperature data. Helium concentrations in W fuzz layers are measured at 1–4 at.%, which is lower than expected for the observed sub-surface voids to be filled with several GPa of helium pressure. This possibly indicates that the void formation is not pressure driven.