15-19 April 2018
Paradise Point Resort & Spa
America/Los_Angeles timezone

2.21 Signal to noise ratio of upgraded imaging bolometer for KSTAR

16 Apr 2018, 10:45
2h 15m
Paradise Point Resort & Spa

Paradise Point Resort & Spa

1404 Vacation Rd, San Diego, CA 92109

Speakers

Byron Jay Peterson (National Institute for Fusion Science) Seungtae Oh (National Fusion Research Institute) Dongcheol Seo (National Fusion Research Institute) Juhyeok Jang (Korea Advanced Institute of Science and Technology) Kiyofumi Mukai (National Institute for Fusion Science) Jae Sun Park (Korea Advanced Institute of Science and Technology) Wonho Choe (Korea Advanced Institute of Science and Technology)

Description

An InfraRed imaging Video Bolometer (IRVB) [1,2] that was previously used on the JT-60U device [3] was installed on KSTAR in 2012. The IRVB had a 2 micron x 7 cm x 9 cm Pt foil blackened with graphite and a 5 mm x 5 mm aperture located 7.5 cm from the foil and had 16 x 12 channels and a time resolution of 10 ms. In 2017 the IRVB was upgraded by replacing the IR camera with a FLIR SC7600 (InSb, 640 x 512 pixels, 105 fps, 25 mK). The aperture area was reduced by approximately half to 3.5 mm x 3.5 mm and the number of channels was quadrupled to 32 x 24. Assuming a uniformly radiating plasma of 15 m3 and 1 MW of radiated power and a viewing path length through the plasma of 3 m, the signal level on the foil was estimated to be 55 W/m2 in the previous case and 27 W/m2 with the upgrade. The resulting NEPDs (signal to noise ratios (SNR)) were 1.28 W/m2 (43) in the previous case and 2.35 W/m2 (12) with the upgrade. In the conference presentation synthetic images from SOLPS modelling will be compared with experimental images from the upgraded IRVB to give better estimates of the SNR. [1] B.J. Peterson, Rev. Sci. Instrum. 71(10) (2000) 3696. [2] B.J. Peterson et al., Rev. Sci. Instrum. 74(3) (2003) 2040. [3] B.J. Peterson et al., Rev. Sci. Instrum.79 (2008) 10E301.

Primary author

Byron Jay Peterson (National Institute for Fusion Science)

Co-authors

Seungtae Oh (National Fusion Research Institute) Dongcheol Seo (National Fusion Research Institute) Juhyeok Jang (Korea Advanced Institute of Science and Technology) Kiyofumi Mukai (National Institute for Fusion Science) Jae Sun Park (Korea Advanced Institute of Science and Technology) Wonho Choe (Korea Advanced Institute of Science and Technology)

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