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WANG Erhui (王二辉), S. MORITA, M. GOTO, DONG Chunfeng (董春凤). Observation of the Two-Dimensional Distribution of Impurity Line Emissions Using a Space-Resolved EUV Spectrometer in LHD[J]. Plasma Science and Technology, 2013, 15(2): 106-109. DOI: 10.1088/1009-0630/15/2/05
Citation: WANG Erhui (王二辉), S. MORITA, M. GOTO, DONG Chunfeng (董春凤). Observation of the Two-Dimensional Distribution of Impurity Line Emissions Using a Space-Resolved EUV Spectrometer in LHD[J]. Plasma Science and Technology, 2013, 15(2): 106-109. DOI: 10.1088/1009-0630/15/2/05

Observation of the Two-Dimensional Distribution of Impurity Line Emissions Using a Space-Resolved EUV Spectrometer in LHD

Funds: partially carried out under the LHD project ¯nancial support (NIFS12ULPP010) and also partly supported by the JSPS-NRF-NSFC A3 Foresight Program in the ¯eld of Plasma Physics (No. 11261140328)
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  • Received Date: January 06, 2012
  • A space-resolved EUV spectrometer for measuring the one-dimensional distribution of impurity line emissions in Large Helical Device (LHD) has been upgraded to measure two- dimensional distributions of impurity line emissions with an extension of working wavelength range to 30x650Å. The two-dimensional measurement is performed by scanning the observation chord horizontally. A rectangular plasma region of 520x700 mm2 in vertical and horizontal sizes can be observed during a single horizontal scan. The horizontal scan requires a time duration of 5 s at least. The spatial resolution is 10 mm in the vertical direction when a spatial-resolution slit of 0.2 mm in width is adopted. Although a spatial resolution in the toroidal direction is 75 mm, it is a function of CCD exposure time and horizontal scanning speed. Two-dimensional distribution of EUV line emissions from several impurities has been successfully observed for the first time from steady discharges in LHD. In this paper two-dimensional distributions of He II (303.78 Å), C V (40.27 Å), C VI (33.73 Å) and Fe XX (132.85 Å) located at di®erent radial positions are presented with simple analysis on the magnetic field structure of LHD.
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