4.1 Article

INTERFEROMETER SYSTEMS ON LHD

期刊

FUSION SCIENCE AND TECHNOLOGY
卷 58, 期 1, 页码 352-363

出版社

AMER NUCLEAR SOC
DOI: 10.13182/FST10-8

关键词

LHD; interferometer; millimeter-wave; far-infrared and infrared laser

资金

  1. National Institute for Fusion Science [ULHH501, ULHH525]
  2. EPSRC [EP/I501045/1] Funding Source: UKRI

向作者/读者索取更多资源

This paper describes the interferometer systems on the Large Helical Device (LHD). LHD is equipped with five interferometer systems, each of which has a different operational purpose and measurable electron density range. A single-channel millimeter-wave interferometer is mainly used for low-density plasmas along a horizontal line of sight on the equatorial plane. Wavelengths of 1 and 2 mm are used for vibration compensation based on two-color interferometry, which has been used since the first operation of LHD. A 13-channel CH(3)OH laser interferometer (wavelength of 119,am) covers almost the whole poloidal cross sections of LHD plasmas with a chord separation of 90 mm. It routinely provides temporal behavior and profiles of the electron density. The laser has been developed as a collaboration between the National Institute for Fusion Science (NIFS) and Chubu University. An 80-channel CO(2) laser interferometer (10.6 mu m) is employed for high-density plasmas such as superdense core plasmas. It adopts an imaging technique with three slablike beams and array detectors to measure the density profile precisely. A phase contrast imaging interferometer, which measures density fluctuations, is combined with the CO(2) laser interferometer. Since LHD has strong magnetic shear, a distribution of the density fluctuations is evaluated by using shear technique. A conventional millimeter-wave (4 mm) interferometer is also installed at a divertor region to measure dynamic density responses in a divertor leg. The phase counter used on these interferometers was originally developed at NIFS. The phase resolution of a typical phase counter is 1/100 fringe with a temporal response of 10 mu s.

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