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

12.22 Initial operation results of NE213 scintillation detector for the time-resolved triton burnup measurements in KSTAR

18 Apr 2018, 20:30
2h 1m
Paradise Point Resort & Spa

Paradise Point Resort & Spa

1404 Vacation Rd, San Diego, CA 92109

Speakers

Jungmin Jo (Department of Energy System Engineering, Seoul National University) MunSeong Cheon Junghee Kim (National Fusion Research Institute) Mitsutaka Isobe (National Institute for Fusion Science, National Institutes of Natural Sciences) Kunihiro Ogawa (National Institute for Fusion Science, National Institutes of Natural Sciences) Takeo Nishitani (National Institute for Fusion Science, National Institutes of Natural Sciences) Seungil Park (National Fusion Research Institute) Isao Murata (Division of Sustainable Energy and Environmental Engineering, Graduate School of Engineering, Osaka University) Kyoung-Jae Chung (Department of Energy System Engineering, Seoul National University) Yong-Seok Hwang (Department of Energy System Engineering, Seoul National University)

Description

For the purpose of time-resolved triton burnup measurements in the KSTAR deuterium plasmas, an NE213 liquid scintillation detector has been installed and operated during the 2017 KSTAR campaign. The detector is composed of a 2-inch diameter NE213 scintillator and a photomultiplier tube (PMT). The PMT pulse signal is processed by the data acquisition system of which the field programmable gate array circuit and the pulse processing software can discriminate the pulse signals from gamma-ray and neutron. In order to achieve a good neutron and gamma-ray discrimination performance, the maximum count rate was retained under 10^5 counts per seconds by shielding the scintillator with 5 cm thick lead blocks and 20 cm thick borated polyethylene blocks. To determine an appropriate threshold level of 14 MeV neutron signal resulting from triton burnup, the NE213 scintillation detector has been calibrated by the 2.5 MeV neutron source in NFRI and the Intense 14 MeV Neutron Source Facility, OKTAVIAN, of Osaka University, Japan. The operation result is compared with the parameters related to the triton birth and confinement characteristics of KSTAR deuterium plasmas, e.g. 2.5 MeV neutron emission rate, plasma current, and electron Coulomb collision time.

Primary author

Jungmin Jo (Department of Energy System Engineering, Seoul National University)

Co-authors

MunSeong Cheon Junghee Kim (National Fusion Research Institute) Mitsutaka Isobe (National Institute for Fusion Science, National Institutes of Natural Sciences) Kunihiro Ogawa (National Institute for Fusion Science, National Institutes of Natural Sciences) Takeo Nishitani (National Institute for Fusion Science, National Institutes of Natural Sciences) Seungil Park (National Fusion Research Institute) Isao Murata (Division of Sustainable Energy and Environmental Engineering, Graduate School of Engineering, Osaka University) Kyoung-Jae Chung (Department of Energy System Engineering, Seoul National University) Yong-Seok Hwang (Department of Energy System Engineering, Seoul National University)

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