Plasma and Fusion Research
Volume 8, 2402176 (2013)
Regular Articles
- 1)
- Department of Fusion Science, Graduate University for Advanced Studies, Toki, Gifu 509-5292, Japan
- 2)
- National Institute for Fusion Science, Toki, Gifu 509-5292, Japan
Abstract
Two-dimensional distribution of impurity lines emitted from ergodic layer with stochastic magnetic field lines in Large Helical Device (LHD) has been observed using a space-resolved extreme ultraviolet (EUV) spectrometer. The two-dimensional electron temperature distribution in the ergodic layer is successfully measured using the line intensity ratio of Li-like NeVIII 2s-3p (2S1/2-2P3/2: 88.09 Å, 2S1/2-2P1/2: 88.13 Å) to 2p-3s (2P1/2-2S1/2: 102.91 Å, 2P3/2-2S1/2: 103.09 Å) transitions emitted from radial location near Last Closed Flux Surface (LCFS). The intensity ratio analyzed with ADAS code shows no dependence on the electron density below 1014 cm−3. The result indicates a little higher temperature, i.e., 220 eV, in the poloidal location at high-field side near helical coils called O-point compared to the temperature near X-point, i.e., 170 eV. The electron temperature profile is also measured at the edge boundary of ergodic layer using the line intensity ratio of Li-like CIV 2p-3d (2P1/2-2D3/2: 384.03 Å, 2P3/2-2D5/2: 384.18 Å) to 2p-3s (2P1/2-2S1/2: 419.53 Å, 2P3/2-2S1/2: 419.71 Å) transitions. The intensity ratios analyzed with CHIANTI, ADAS and T.Kawachi codes show a slightly higher temperature near O-point, i.e., 25 eV for CHIANTI, 21 eV for ADAS and 11 eV for T.Kawachi's codes, compared to the temperature at X-point, i.e., 15 - 21 eV for CHIANTI, 9 - 15 eV for ADAS and 6 - 9 eV for T.Kawachi codes. It suggests that the transport coefficient in the ergodic layer is varied with three-dimensional structure.
Keywords
line intensity ratio, electron temperature, Li-like CIV and NeVIII, EUV spectrometer
Full Text
References
- [1] H.E. Mason and B.C. Monsignori Fossi, Astron. Astrophys. Rev. 6, 123 (1994).
- [2] L. Heroux, Proc. Phys. Soc. 83, 121 (1964).
- [3] T. Kawachi and T. Fujimoto, Phys. Rev. E 51, 1428 (1995).
- [4] H.P. Summers, JET Joint Undertaking internal report, JET-IR 06 (1994).
- [5] K.P. Dere et al., Astron. Astrophys. Suppl. Ser. 125, 149 (1997).
- [6] K.P. Dere et al., Astron. Astrophys. 498, 915 (2009).
- [7] T. Morisaki et al., J. Nucl. Mater. 313, 548 (2003).
- [8] E.H. Wang et al., Rev. Sci. Instrum. 83, 043503 (2012).
- [9] C.F. Dong et al., Rev. Sci. Instrum. 82, 113102 (2011).
- [10] C.F. Dong et al., Phys. Plasmas 18, 082511 (2011).
- [11] S. Masuzaki et al., Nucl. Fusion 42, 750 (2002).
This paper may be cited as follows:
Erhui WANG, Shigeru MORITA, Chunfeng DONG, Motoshi GOTO, Izumi MURAKAMI and Tetsutarou OISHI, Plasma Fusion Res. 8, 2402176 (2013).