• Journal of Radiation Protection and Research
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• 제28권1호
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• pp.19-24
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• 2003

해석적인 방법과 MCNP 로드를 사용하여 $^{198}Au$ 선원시료에 대한 자체감쇠인자와 검출기의 원반형 Al 덮개에 대한 0.412 MeV 감마선의 투과율을 구하였다. 그 결과, 비교적 반경이 큰 Au 시료를 제외하고 모든 경우에서 해석적인 해가 MCNP 코드의 결과와 잘 일치하는 것으로 나타났다. 이때 두 방법의 최대 편차는 약 9 %로서 Au 시료의 반경이 1.5 mm인 경우에 나타났다. 검출기 Al 덮개의 직경이 7.62 cm인 경우에 대한 0.412 MeV 감마선의 투과율에 대한 해석적인 해는 HCNP 코드의 결과와 표준편차의 범위내에서 잘 일치하는 것으로 나타났다.

• Journal of Welding and Joining
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• 제25권5호
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• pp.64-71
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• 2007

The aim of this paper is to investigate the effects of welding parameters on the weld shape in seal-welding of STS304L capsule for manufacturing a radioisotope source which is widely used in nondestructive testing of metal structures using gamma ray. Pulsed gas tungsten arc (Pulsed GTA) welding is performed for thin cross sectional area of the capsule. Seven welding parameters including current waveform parameters and arc length etc. are selected as main process parameters using design of experiment. The weld shape such as bead width, penetration depth, weld area, aspect ratio and area rate is investigated to assess the effects of welding parameters. As results, the combination of pulse duty/welding speed largely affects on bead width, penetration depth, area and aspect ratio. Finally, it is concluded that the key parameters are the combination of pulse duty/welding speed, base current and arc length, and their optimal conditions are 50%/1.77mm/s, 6.4A and 1 mm.

• Journal of Radiation Protection and Research
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• 제48권4호
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• pp.167-174
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• 2023

Background: A nondestructive test is commonly used to inspect the surface defects and internal structure of an object without any physical damage. X-rays generated from an electron accelerator or a tube are one of the methods used for nondestructive testing. The high penetration of X-rays through materials with low atomic numbers makes it difficult to discriminate between these materials using X-ray imaging. The interaction characteristics of neutrons with materials can supplement the limitations of X-ray imaging in material discrimination. Materials and Methods: The radiation image acquisition process for air-cargo security inspection equipment using X-rays and neutrons was simulated using a GEometry ANd Tracking (Geant4) simulation toolkit. Radiation images of phantoms composed of 13 materials were obtained, and the R-value, representing the attenuation ratio of neutrons and gamma rays in a material, was calculated from these images. Results and Discussion: The R-values were calculated from the simulated X-ray and neutron images for each phantom and compared with those obtained in the experiments. The R-values obtained from the experiments were higher than those obtained from the simulations. The difference can be due to the following two causes. The first reason is that there are various facilities or equipment in the experimental environment that scatter neutrons, unlike the simulation. The other is the difference in the neutron signal processing. In the simulation, the neutron signal is the sum of the number of neutrons entering the detector. However, in the experiment, the neutron signal was obtained by superimposing the intensities of the neutron signals. Neutron detectors also detect gamma rays, and the neutron signal cannot be clearly distinguished in the process of separating the two types of radiation. Despite these differences, the two results showed similar trends and the viability of using simulation-based radiation images, particularly in the field of security screening. With further research, the simulation-based radiation images can replace ones from experiments and be used in the related fields. Conclusion: The Korea Atomic Energy Research Institute has developed air-cargo security inspection equipment using neutrons and X-rays. Using this equipment, radiation images and R-values for various materials were obtained. The equipment was reconstructed, and the R-values were obtained for 13 materials using the Geant4 simulation toolkit. The R-values calculated by experiment and simulation show similar trends. Therefore, we confirmed the feasibility of using the simulation-based radiation image.

• Journal of Crop Science and Biotechnology
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• 제10권3호
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• pp.193-200
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• 2007

Mungbean plants generally have a relatively close canopy, thus a large amount of self-shading can reduce yield due to poor light penetration. Modification of leaflet type can affect leaf canopy and could alter seed yield. Two multiple leaflet mutants were obtained from gamma-ray irradiation and used to study the mode of inheritance related to leaflet types and to evaluate their agronomic features. The cross between large-heptafoliate leaflet with small-pentafoliate leaflet mutants produce all $F_1$ plants with normal trifoliate leaflets. The $F_2$ plants segregated in leaflet size and leaflet number into a 9:3:3:1 ratio of large-trifoliate: large-heptafoliate: small-pentafoliate: small-heptafoliate plants, suggesting that independent loci control leaflet size and leaflet number. Regarding leaflet number, the $F_2$ population can be classified into normal-trifoliate, small-pentafoliate, large-heptafoliate, and small-heptafoliate at the dihybrid ratio of 9:3:3:1. The gene symbols $N_1,n_1$ and $N_2,n_2$ are proposed to represent leaflet number. Since no plant was found with large-pentafoliate leaflets, we hypothesize that the $N_2$ allele expresses pleiotropic effect on both leaflet number and leaflet size. Another possibility is that an additional locus with S and s alleles controls leaflet size and S is tightly linked with $N_2$. The effect of multifoliate leaflet on yield and yield components was evaluated in four mungbean families each with four leaflet isolines under three environments. Averaging across the families and environments, the normal-trifoliate and large-heptafoliate lines gave higher yield than small pentafoliate and heptafoliate ones. These two large leaflet lines also had higher leaf area per plant than the other multifoliate lines. Therefore, the mungbean lines with a greater leaf area, which were likely to intercept more sunlight, gave greater yield. Three AFLP markers that were found to be linked to number of leaflets per leaf, corresponded to the N1 allele of the smallpentafoliate parent.

• Journal of Astronomy and Space Sciences
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• 제36권1호
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• pp.21-33
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• 2019

This paper focuses on the interpretation of radiation fluxes from active galactic nuclei. The advantage of positron annihilation spectroscopy over other methods of spectral diagnostics of active galactic nuclei (therefore AGN) is demonstrated. A relationship between regular and random components in both bolometric and spectral composition of fluxes of quanta and particles generated in AGN is found. We consider their diffuse component separately and also detect radiative feedback after the passage of high-velocity cosmic rays and hard quanta through gas-and-dust aggregates surrounding massive black holes in AGN. The motion of relativistic positrons and electrons in such complex systems produces secondary radiation throughout the whole investigated region of active galactic nuclei in form of cylinder with radius R= 400-1000 pc and height H=200-400 pc, thus causing their visible luminescence across all spectral bands. We obtain radiation and electron energy distribution functions depending on the spatial distribution of the investigated bulk of matter in AGN. Radiation luminescence of the non-central part of AGN is a response to the effects of particles and quanta falling from its center created by atoms, molecules and dust of its diffuse component. The cross-sections for the single-photon annihilation of positrons of different energies with atoms in these active galactic nuclei are determined. For the first time we use the data on the change in chemical composition due to spallation reactions induced by high-energy particles. We establish or define more accurately how the energies of the incident positron, emitted ${\gamma}-quantum$ and recoiling nucleus correlate with the atomic number and weight of the target nucleus. For light elements, we provide detailed tables of all indicated parameters. A new criterion is proposed, based on the use of the ratio of the fluxes of ${\gamma}-quanta$ formed in one- and two-photon annihilation of positrons in a diffuse medium. It is concluded that, as is the case in young supernova remnants, the two-photon annihilation tends to occur in solid-state grains as a result of active loss of kinetic energy of positrons due to ionisation down to thermal energy of free electrons. The single-photon annihilation of positrons manifests itself in the gas component of active galactic nuclei. Such annihilation occurs as interaction between positrons and K-shell electrons; hence, it is suitable for identification of the chemical state of substances comprising the gas component of the investigated media. Specific physical media producing high fluxes of positrons are discussed; it allowed a significant reduction in the number of reaction channels generating positrons. We estimate the brightness distribution in the ${\gamma}-ray$ spectra of the gas-and-dust media through which positron fluxes travel with the energy range similar to that recorded by the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) research module. Based on the results of our calculations, we analyse the reasons for such a high power of positrons to penetrate through gas-and-dust aggregates. The energy loss of positrons by ionisation is compared to the production of secondary positrons by high-energy cosmic rays in order to determine the depth of their penetration into gas-and-dust aggregations clustered in active galactic nuclei. The relationship between the energy of ${\gamma}-quanta$ emitted upon the single-photon annihilation and the energy of incident electrons is established. The obtained cross sections for positron interactions with bound electrons of the diffuse component of the non-central, peripheral AGN regions allowed us to obtain new spectroscopic characteristics of the atoms involved in single-photon annihilation.

• 핵의학기술
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• 제18권1호
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• pp.33-42
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• 2014

I-131의 주 에너지는 364 keV이고 이차적으로 637과 723 keV의 감마선을 방출한다. 이런 이유로 I-131 핵종을 이용한 검사에서는 일반적으로 고 에너지 조준기를 사용하고 있다. 반면 중 에너지 조준기는 과도한 격벽 투과의 영향 때문에 사용이 권고되지 않지만 I-131의 낮은 선량에 대해 계수율의 민감도를 향상시키기 위해 중 에너지 조준기를 사용하기도 한다. 이에 본 연구에서는 I-131 SPECT/CT에서 고 에너지와 중 에너지 조준기를 사용하여 조준기 선택에 대한 영상의 영향을 평가하고자 한다. I-131 점 선원과 NEMA NU-2 IQ phantom을 이용하여 Siemens symbia T16 SPECT/CT 장비로 중 에너지 조준기와 고 에너지 조준기를 사용하였다. 영상획득은 단일 에너지 창과 삼중 에너지 창으로 각각 적용하여 영상을 획득하였고, 재구성방법은 반복재구성 기법인 Flash 3D를 이용하여 CTAC, Scatter correction 적용 유무와 Iteration과 subset의 횟수를 변경하여 획득된 영상을 재구성하였다. 획득된 영상을 분석하여 두 조준기의 민감도와 대조도 그리고 잡음을 비교 평가하였다. 민감도는 중 에너지 조준기가 고 에너지 조준기보다 높게 나타났다(중 에너지 조준기: 188.18 cps/MBq, 고 에너지 조준기: 46.31 cps/MBq). 대조도는 삼중 에너지 창과 고 에너지 조준기를 사용하고 CTAC를 적용하여 16 subset 8 iteration을 적용한 재구성영상에서 가장 높은 대조도를 나타냈고(TCQI=190.64), 동일한 조건에서 중 에너지 조준기를 사용하였을 경우는 고 에너지 조준기에 비해 낮은 대조도를 나타냈다(TCQI=66.05). 잡음평가에서는 고 에너지 조준기보다 중 에너지 조준기에서 높게 나타났다 (P<0.001). 적절한 조준기의 선택은 영상의 질에 있어 중요한 사항이다. 본 연구를 통해 고 에너지 감마선을 방출하는 I-131 검사에서는 일반적으로 사용되고 있는 고 에너지 조준기를 사용하는 것이 영상의 질에 있어 가장 권고되는 바이다. 하지만 에너지 창, 매트릭스 크기, 반복 재구성 조건(subset과 iteration 수) 그리고 CTAC 및 scatter correction 여부등과 같은 조건들을 적절히 적용한다면 낮은 선량의 낮은 민감도를 갖는 조건에서는 중 에너지 조준기를 사용할 수 있을 것으로 사료된다.