Plasma and Fusion Research

Volume 15, 1201004 (2020)

Rapid Communications


Microstructure and Retention in He-W Co-Deposition Layer
Kosuke ASAI, Naoaki YOSHIDA1), Noriyasu OHNO, Shin KAJITA2), Hirohiko TANAKA, Miyuki YAJIMA3) and Daisuke NAGATA3)
Graduate School of Engineering, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8603, Japan
1)
RIAM, Kyushu University, 6-1 Kasugakoen, Kasuga-shi, Fukuoka 816-8580, Japan
2)
IMaSS, Nagoya University, Nagoya 464-8603, Japan
3)
National Institute for Fusion Science, Oroshi-cho, Toki, Gifu 509-5292, Japan
(Received 9 December 2019 / Accepted 5 January 2020 / Published 17 February 2020)

Abstract

A tungsten (W) deposition layer is formed while a sample is exposed to a helium (He) plasma at the surface temperature of 473 or 573 K. The formed He-W co-deposition layer was composed of fine grains, the size of which increased with the surface temperature. The samples with the co-deposition layer was exposed to a deuterium (D2) plasma, and the D retention was investigated using thermal desorption spectroscopy. It was found that the co-deposition layer has quite different D retention characteristics compared with bulk W.


Keywords

He-W co-deposition, plasma-material interactions, Co-NAGDIS

DOI: 10.1585/pfr.15.1201004


References

  • [1] S. Takamura et al., Plasma Fusion Res. 1, 051 (2006).
  • [2] S. Kajita et al., Nucl. Fusion 49, 095005 (2009).
  • [3] M. Rubel et al., Fusion Eng. Des. 136, 579 (2018).
  • [4] G. De Temmerman et al., J. Nucl. Mater. 389, 479 (2009).
  • [5] X.H. Tang et al., J. Nucl. Mater. 446, 200 (2014).
  • [6] S. Iyyakkunel et al., ACS Appl. Mater. Interfaces 6, 11609 (2014).
  • [7] S. Kajita et al., Nucl. Fusion 58, 106002 (2018).
  • [8] S. Kajita et al., Scientific Reports 8, 9 (2018).
  • [9] M. Yajima et al., J. Nucl. Mater. 449, 9 (2014).
  • [10] D. Nishijima et al., J. Nucl. Mater. 337-339, 927 (2005).
  • [11] K. Tokunaga et al., J. Nucl. Mater. 313-316, 92 (2003).
  • [12] H.T. Lee et al., J. Nucl. Mater. 360, 196 (2007).