• Nuclear Engineering and Technology
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• 제56권1호
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• pp.328-334
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• 2024

The activation method of metallic foils is an important technique to measure the flux and energy of proton beams. In this paper, the method was used to measure the CSNS APEP proton flux at seven nominal proton energies ranging from 10 MeV to 70 MeV for beam spot sizes of the 20 mm × 20 mm and 50 mm × 50 mm. The reactions of ^natTi(p, x)⁴⁸V, ^natNi(p, x)⁵⁷Ni, ^natCu(p, x)⁵⁸Co, and ²⁷Al(p, x)²⁴Na were employed to measure the proton beam flux with a range of 10⁷-10⁹ p/cm²/s. Furthermore, we also proposed a method using the activity ratio with a stacked-foil target to determine the energy spread of a Gaussian-like distribution for different nominal proton energies. The optimal combinations of Al, Cu, Ti, Ni, Mo, Fe, Nb, and In foils were adopted for the proton energies. The measured energy spreads for degraded beams of 30 MeV-70 MeV were found to be smaller than 10.00%.

• 한국원자력학회:학술대회논문집
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• 한국원자력학회 2005년도 춘계학술발표회
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• pp.903-904
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• 2005

• 한국수소및신에너지학회논문집
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• 제33권4호
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• pp.353-362
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• 2022

In this study, water diffusion in proton exchange membrane fuel cell at open circuit voltage (OCV) was analyzed through experiment. First, the reliability of the micro-sensor (SHT31) was verified. It was concluded the micro-sensor has an excellent reliability at 60℃ and 70℃. After the sensor reliability test, the temperature and relative humidity measurement in bipolar-plate was conducted at OCV. To analyze water distribution and water flux, the temperature and relative humidity was converted into dew point. To the end, it was found water concentration affects water diffusion.

• Nuclear Engineering and Technology
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• 제53권7호
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• pp.2075-2083
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• 2021

The article provides a review of the research results obtained during of more than 20 years concerning using the gaseous radiochemical method (GRCM) for detecting of ionizing radiation. This method based on threshold nuclear reactions with production of radioactive noble gas which does not interact with the materials of gaseous tract. The applications of GRCM in the diagnostics of neutrinos, neutrons, charged particles, thermonuclear plasma thermometry, and the study of the structure and dynamics of astrophysical objects, position-sensitive dosimetry of neutron targets with accelerator driving, spatial distribution of the fast neutron flux density in a nuclear reactor allowing the transformation of longitudinal coordinate of neutron flux distribution into a temporal distribution of the radiochemical gas decay counting rate ("barcode" semblance) and measurement of bombarding particles spectra are described. Experimental testing of the described technologies was made on the neutron target driven with the linear proton accelerator of Institute for Nuclear Research of Russian Academy of Sciences (INR RAS).

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2010년도 한국우주과학회보 제19권1호
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• pp.38.3-39
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• 2010

While major solar proton events (SPEs) come from the coronal mass eject (CME)-driven shocks in solar wind, there are many evidences that potentiality of CMEs to generate SPEs depends on its early evolution near the Sun and on different solar activities observed around the CME liftoff time. To decipher origin of SPE release, we have investigated onset time comparison of the SPE with CME, metric type II radio burst, and hard X-ray flare. For this, we select 30 SPEs observed from 1997 to 2006 by using the particle instrument ERNE onboard SOHO, which allows proton flux anisotropy measurement in the energy range ~10 - 50MeV. Onset time of the SPEs is inferred by considering the energy-dependent proton transport time. As results, we found that (1) SPE onset time is comparable to that of type II but later than type III onset time and HXR start time, (2) SPE onset time is mostly later than the peak time of HXR flare, (3) almost half of the SPE onsets occurred after the HXR emission, and (4) there are two groups of CME height at the onset time of SPE; one is the height below 5 Rs (low corona) and the other is above 5Rs (high corona). In this talk, we will present the onset time comparison and discuss about the origin of the SPE onset.

• Journal of Radiation Protection and Research
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• 제36권2호
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• pp.59-63
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• 2011

가속기 기반 중성자 표준장은 검출기 및 도시메터 교정, 핵자료 생산, 동위원소 생산등 에 필수적으로 필요한 기반 장비이다. 가속기 기반 중성자 표준장 실험실을 설계하는데 있어서 원하는 에너지의 직접적인 중성자 이외에 산란되어서 입사하는 산란 중성자를 줄이는 것은 매우 중요하다. 따라서 그러한 조건을 얻어내기 위하여 다양한 조건을 가정하여 MCNPX 모사계산을 수행하였다. 우선은 기존의 실험실 조건에서 양성자 운동방향인 0도 방향에 있는 중성자 Flux 측정용 공기로 이루어진 가상의 Chamber에 직접 입사하는 중성자 flux와 벽이나 바닥에 충돌을 한 후에 입사하는 간접적인 산란 중성자 flux를 각각 계산하였다. 그 결과 충돌 한 후에 0도 방향의 Chamber에 입사하는 산란 중성자 flux 중에 바닥에 충돌을 한 후 0도 방향의 Chamber로 입사하는 산란 중성자 flux가 가장 많다는 것을 알 수 있었다. 따라서 바닥의 콘크리트만을 없앴을 때와 콘크리트를 제거하고 땅을 1m 정도 파내려갔을 때를 가정하여 재계산을 하였고 그 결과 콘크리트를 없애고 땅을 1m 정도 파면 바닥에 충돌하고 Chamber로 들어오는 산란 중성자 flux가 다른 곳에 충돌하고 들어오는 것보다 낮아지는 정도까지 줄어드는 것을 알 수 있었다.

• Journal of Astronomy and Space Sciences
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• 제24권2호
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• pp.155-166
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• 2007

우주환경의 주 요소인 고에너지 입자를 검출하기 위한 고분해능 전자 및 양성자 검출기를 설계하였다. 전자와 양성자의 flux는 궤도상의 위치나 태양활동에 따라 급격하게 변할 수 있다. 이러한 상황에서 높은 에너지 분해능으로 입자환경을 검출, 연구하기 위한 검출기의 개념설계를 시도하였으며, 이를 실제 우주환경에서 어느 정도의 성능을 가질 수 있는지를 예측하여 보았다. 또한, 높은 입자 플럭스에도 정상적인 측정이 가능할 수 있도록 FPGA를 이용한 병렬 처리 알고리즘을 고안하고 전산모사 기법을 통하여 성능을 평가하였다.

• Journal of Astronomy and Space Sciences
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• 제31권3호
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• pp.277-283
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• 2014

Next Generation Small Satellite-1 (NEXTSat-1) is scheduled to launch in 2017 and Instruments for the Study of Space Storm (ISSS) is planned to be onboard the NEXTSat-1. High Energy Particle Detector (HEPD) is one of the equipment comprising ISSS and the main objective of HEPD is to measure the high energy particles streaming into the Earth radiation belt during the event of a space storm, especially, electrons and protons, to obtain the flux information of those particles. For the design of HEPD, the Geometrical Factor was calculated to be 0.05 to be consistent with the targets of measurement and the structure of telescope with field of view of $33.4^{\circ}$ was designed using this factor. In order to decide the thickness of the detector sensor and the classification of the detection channels, a simulation was performed using GEANT4. Based on the simulation results, two silicon detectors with 1 mm thickness were selected and the aluminum foil of 0.05 mm is placed right in front of the silicon detectors to shield low energy particles. The detection channels are divided into an electron channel and two proton channels based on the measured LET of the particle. If the measured LET is less than 0.8 MeV, the particle belongs to the electron channel, otherwise it belongs to proton channels. HEPD is installed in the direction of $0^{\circ}$, $45^{\circ}$, $90^{\circ}$ against the along-track of a satellite to enable the efficient measurement of high energy particles. HEPD detects electrons with the energy of 0.1 MeV to several MeV and protons with the energy of more than a few MeV. Thus, the study on the dynamic mechanism of these particles in the Earth radiation belt will be performed.

• Journal of Radiation Protection and Research
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• 제38권3호
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• pp.143-148
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• 2013

원자력발전소 및 입자 가속기 등 상용화된 원자력관계시설에서는 해당 시설 내부의 구조 및 위치 등에 따라 다양한 에너지를 가진 중성자스펙트럼을 나타내며 이에 대한 중성자선량 평가 및 작업자의 방사선방호 조치에 대한 수요는 점차 증가하고 있다. 중성자스펙트럼을 측정하기 위해서 일반적으로 보너구 스펙트로메터가 많이 이용된다. 보너구 스펙트로메터를 이용한 중성자 스펙트럼 측정의 경우 중성자검출기의 반응함수, 초기추정 스펙트럼, 계수율 측정값을 사용하여 중성자스펙트럼 언폴딩을 수행하게 된다. 본 연구에서는 MC50 사이클로트론에서 발생하는 중성자스펙트럼을 LiI 섬광검출기 기반의 보너구 스펙트로메터를 이용하여 측정하였으며 표적에 입사되는 양성자 에너지와 위치에 따른 중성자선속, 중성자 평균에너지 및 선량률 자료를 정량적으로 평가하였다.

• 대한방사선기술학회지:방사선기술과학
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• 제44권4호
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• pp.359-365
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• 2021

A heavy particle accelerator is a device that accelerates particles using high energy and is used in various fields such as medical and industrial fields as well as research. However, secondary neutrons and particle fragments are generated by the high-energy particle beam, and among them, the neutrons do not have an electric charge and directly interact with the nucleus to cause radiation of the material. Quantitative evaluation of the radioactive material produced in this way is necessary, but there are many difficulties in actual measurement during or after operation. Therefore, this study compared and evaluated the generated radioactive material in the concrete shield for protons and carbon ions of specific energy by using the simulation code FLUKA. For the evaluation of each energy of proton beam and carbon ion, the reliability of the source term was secured within 2% of the relative error with the data of the NASA Space Radiation Laboratory(NSRL), which is an internationally standardized data. In the evaluation, carbon ions exhibited higher neutron flux than protons. Afterwards, in the evaluation of radioactive materials under actual operating conditions for disposal, a large amount of short-lived beta-decay nuclides occurred immediately after the operation was terminated, and in the case of protons with a high beam speed, more radioactive products were generated than carbon ions. At this time, radionuclides of ⁴⁴Sc, ³H and ²²Na were observed at a high rate. In addition, as the cooling time elapsed, the ratio of long-lived nuclides increased. For nonparticulate radionuclides, ³H, ²²Na, and for particulate radionuclides, ⁴⁴Ti, ⁵⁵Fe, ⁶⁰Co, ¹⁵²Eu, and ¹⁵⁴Eu nuclides showed a high ratio. In this study, it is judged that it is possible to use the particle accelerator as basic data for facility maintenance, repair and dismantling through the prediction of radioactive materials in concrete according to the cooling time after operation and termination of operation.