Published June 2011 | Version v1
Journal article

Development of two-grating spectrometer for the charge exchange spectroscopy system on KSTAR

  • 1. National Fusion Research Institute (NFRI), Gwahangno113, Daejeon 305-333 (Korea, Republic of)
  • 2. Department of Nuclear Fusion and Plasma Science, University of Science and Technology (UST), Gajungro 217, Daejeon 305-350 (Korea, Republic of)
  • 3. Division of Energy Systems Research, Ajou University, Suwon 443-749 (Korea, Republic of)
  • 4. Department of Chemistry, Ajou University, Suwon 443-749 (Korea, Republic of)

Description

The charge exchange spectroscopy (CES) system on Korea Superconducting Tokamak Advanced Research (KSTAR) was installed last year and had been applied to measure the C VI ion temperature and rotation velocity profiles. The ion temperature and rotation velocity profiles had been estimated from the C VI 5290.5 A (n = 8-7) charge-exchange spectrum signal measured by a Czerny-Turner type spectrometer and a thinned back-illuminated charge coupled device (CCD) camera. However, the Czerny-Turner type spectrometer used for the KSTAR CES system showed so low signal to noise ratio for KSTAR plasmas in the 2010 experimental campaign that the time resolution of the CES system had been limited to 100 ms due to the increased exposure time of the attached CCD camera. Then, new two-grating spectrometer had been developed in order to improve the time resolution of the CES system. The spectrometer consists of two gratings (1200 g/mm and 1800 g/mm each) with additive configuration, concave mirrors (f = 50 cm), and a cylindrical lens (f = 50 cm). The time resolution of the CES system increases by a factor of 2-4 with the two-grating spectrometer. The C VI ion temperature and rotation velocity profiles obtained by the two-grating spectrometer are compared to those by Czerny-Turner type spectrometer in this paper.

Additional details

Identifiers

Publishing Information

Journal Title
Review of Scientific Instruments
Journal Volume
82
Journal Issue
6
Journal Page Range
p. 063510-063510.5
ISSN
0034-6748
CODEN
RSINAK

Optional Information

Notes
(c) 2011 American Institute of Physics