Speaker
Dr
Cormac Corr
(Australian National University)
Description
Tungsten has been chosen as the material for the ITER divertor and is a contender for the wall of DEMO, which will experience temperatures in excess of 1000 K. The interaction between high-flux helium plasmas with tungsten can lead to plasma-induced surface modifications. In particular helium retention in tungsten is problematic, since helium is known to form nano-scale bubbles beneath the surface, and are thought to be responsible for the formation of nano-fuzz and surface pitting [1,2].
Results from Grazing Incidence Small Angle X-Ray Scattering (GISAXS) measurements [3] performed at the Australian Synchrotron show that in tungsten exposed to pure helium plasmas in linear plasma devices, such as the MAGnetised Plasma Interaction Experiment (MAGPIE) [4], nano-sized bubbles of between 1.5 – 2.5 nm diameter are formed in near-surface layers of approximately 30 nm thickness. The findings are in excellent agreement with a direct observation by transmission electron microscopy. Depth distributions were estimated by taking successive measurements across a range of x-ray incidence angles. As an example, for tungsten at 700°C, the bubble layer is observed to be 31 +/- 4 nm deep.
A helium ion energy threshold of approximately 9eV has been identified, above which helium nano-bubbles are formed and is strongly correlated with an increase in helium retention. The effects of surface temperature and plasma fluence on nano-bubble formation will also be presented.
[1] S. Kajita, N. Yoshida, R. Yoshihara, et al., J. Nucl. Mater. 418, 152-158 (2011)
[2] D. Nishijima, M. Y. Ye, N. Ohno, et al., J. Nucl. Mater. 313-316, 97 (2003)
[3] M. Thompson, P. Kluth, R. Doerner, N. Kirby, C. Corr, Nuclear Fusion, 55, 042001 (2015)
[4] B.D. Blackwell, J.F. Caneses, C.M. Samuell, J. Wach, J. Howard and C.S. Corr, Plasma Sources Sci. Technol. 21, 055033 (2012)
Country or International Organization | Australia |
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Paper Number | PDP-21 |
Primary author
Dr
Cormac Corr
(Australian National University)
Co-authors
Dr
Daniel Riley
(Australian Nuclear Science and Technology Organisation)
Mr
Matt Thompson
(Australian National University)
Dr
Patrick Kluth
(Australian National University)