• 대한방사선치료학회지
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• 제3권1호
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• pp.63-67
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• 1989

The central beam characteristics of 6 MV X-ray from a Mevatron KD linear Accelerator are examin-depths The PDD (Percent Depth Dose) values and the TMR (Tissue Maximum Ratio) values are evaluated from measurement as a function of the depths and the field sizes. The calculated TMR values from the PDD are compared to those from measurement. The average differences between calculated TMR and measured one are within $1\%$ and we have concluded that calculated TMR values are acceptable for practical use.

• 천문학논총
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• 제30권2호
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• pp.417-421
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• 2015

We analyzed 0.5-45 keV data of NGC 3227 observed by Suzaku six times between 2008 October 28 and December 2. The count-count plot between the 0.5-3 keV and 3-10 keV bands exhibits a clear break, separating the data into bright and faint phases. Applying the difference spectrum method and time-averaged spectral fits to the phase data, we found the presence of two kinds of variable primary X-rays, (1) a hard primary component with ${\Gamma}{\sim}1.7$ dominating in the faint phase and (2) a soft primary continuum with ${\Gamma}{\sim}2.4$ appearing in the bright phase, both affected by partial absorption. Considering their timing and spectral characteristics, component (1) is presumably identical to a Compton continuum in the low/hard state, while component (2) may correspond to the hard tail emission in the high/soft state, or compact-jet emission. In that case, an accretion ow onto the central super massive black hole in NGC 3227 can be interpreted to include the two different states.

• 한국방사선학회논문지
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• 제12권7호
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• pp.919-927
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• 2018

본 연구에서는 일반 X선 검사를 대상으로 시뮬레이션 교육 모델을 제시하고 실습 시 발생하는 오류를 분석하고자 하였다. 2012년부터 2018년까지 총 183명 (남자 77명, 여자 106명)의 학생이 참가하였다. 시뮬레이션 X선 시스템은 컴퓨터방사선영상(computed radiography, CR) 시스템을 이용하였다. 환자 보호, X선 검사의 정확성, 영상의 안정성 등의 검사 프로세스에 발생하는 오류 빈도수를 분석하였다. 그 결과 환자 자세 설정 오류, X선 중심선의 정확성 오류, 영상검출판의 크기 및 위치 설정 오류, 그리드 사용의 오류, 마킹의 오류, X선 조사조건 설정 오류, 조사야 설정의 오류, X선 입사각도의 오류, X선 조사거리의 오류 순으로 분석되었다. 이러한 오류를 중심으로 개선된 방사선사 실습 교육이 필요할 것이며 그로 인하여 정밀한 검사와 고품질의 의료서비스를 제공하여 국민들의 보건의료에 조금이나마 기여할 수 있기를 기대한다.

• 한국안전학회지
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• 제21권4호
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• pp.60-65
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• 2006

It is a well known fact that LCD is a central part of the IT industry which is important in the present and the future. But the biggest problem of LCD manufacturing is maintaining a cleaning room environment and administration. Therefore the purpose of this study is to first, prevent the yield depreciation and damage of products, and second, protect the worker ftom accidental electrostatic discharge during LCD manufacture. The soft x-ray ionizer is a type of electrostatic reducer device. It protects against electrostatic discharge in the cleaning room environment and is a necessary environmental factor during LCD production. The positive aspects of the soft x-ray are its shorter time and wider angle of exposure. But the negative aspect of the soft x-ray is its need for several shielding of protection from the harmful x-ray exposure. On this study, the development of the Air Nozzle-type ionizer to amend and refine some problems. For example, examined the electrostatic reduce device of a soft x-ray type and discovered the ion did not go inside well. also workers to be free from danger. An Air Nozzle-type ionizer is comprised of soft x-ray radiation and ionized air production. Air is injected through the nozzle after being ionized from radiation. It supplies air keeping the same pressure into the end foundation of ion production. The soft x-ray is the structure which radiates ionized air through the nozzle (21 holes) having micro holes of the ionizable radiation after ionizing the inside air by the ion production. A worker does not need a cover to protect against x-rays and the Air Nozzle-type ionizer is easy to set up and is more effective at eliminating electrostatic.

• 천문학회보
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• 제45권1호
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• pp.30.2-31
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• 2020

We present the properties of circumnuclear gas associated with the AGN located in the center of Abell 1644-South. A1644-S is the main cluster in a merging system, which is also known for gas sloshing in its core as seen in X-ray. The X-ray emission of A1644-S shows a rapidly declining profile, indicating the presence of cooling gas flow. This flow of cool gas may fuel the supermassive black hole embedded in the brightest cluster galaxy, leading to the activation of the central AGN. Indeed, we find a parsec-scale bipolar jet feature in the center of A1644-S in our recent KaVA observation, which implies that its central AGN is likely to have been (re)powered quite recently. In order to verify the hypothesis that cooling gas flow in the cluster core can (re)activate the central AGN, we probe the cold gas properties of the central 1 kpc region of A1644-S using the archival VLA and ALMA data. Based on the spatially resolved morphology and kinematics of HI and CO gas, we challenge to identify inflow/outflow gas streams and clumps. We study the role of circumnuclear cool gas in fueling the centrally located cluster AGN in the cool-core environment. We also discuss how the feedback due to the (re)powered AGN affects the surrounding medium.

• 한국방사선학회논문지
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• 제10권7호
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• pp.539-543
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• 2016

본 연구는 진단용 X선 발생장치에서 조사야 외부의 산란선량을 감소시켜 환자의 피폭 선량을 감소시키기 위한 방법이다. 자체 제작한 $150{\times}190mm^2$ 납판을 콜리메이터 하단에 부착함으로써 조사야 이외의 부위에 도달하는 산란선량을 감소시키고자 하였다. 납판을 추가로 삽입 후 X선 관축방향인 X-축의 산란선량을 측정한 결과 26 ~ 36% 감소하는 것으로 나타났으며, 관축의 수직 방향인 Y-축 방향에서는 납판의 사용 유무에 따른 산란선량은 큰 변화를 나타내지 않았다. 이러한 결과는 콜리메이터 Shutter에 의해서 발생하는 산란선 보다는 초점 근방에서 발생하는 초점외 X선에 의한 산란선 영향이 크다는 것을 의미한다. 따라서 기존의 콜리메이터 하단에 추가로 납판을 설치하는 것이 조사야 외부의 X-축 산란선량을 감소시키는 방법으로 판단되어진다.

• 천문학회지
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• 제37권5호
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• pp.575-578
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• 2004

High resolution observations of cluster of galaxies by Chandra have revealed the existence of an X-ray emitting comet-like galaxy C153 in the core of cluster of galaxies A2125. The galaxy C153 moving fast in the cluster core has a distinct X-ray tail on one side, obviously due to ram pressure stripping, since the galaxy C153 crossed the central region of A2125. The X-ray emitting plasma in the tail is substantially cooler than the ambient plasma. We present results of two-dimensional magnetohydrodynamic simulations of the time evolution of a sub clump like C153 moving in magnetized intergalactic matter. Anisotropic heat conduction is included. We found that the magnetic fields are essential for the existence of the cool X-ray tail, because in non-magnetized plasma the cooler sub clump tail is heated up by isotropic heat conduction from the hot ambient plasma and does not form such a comet-like tail.

• 천문학회지
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• 제37권5호
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• pp.375-379
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• 2004

In this paper I give an overview of the detection of emission from the warm-hot intergalactic medium (WHIM) in the outer parts of clusters of galaxies. The evidence for the presence of soft excess X-ray emission in 7 out of 21 clusters is summarized, and it is demonstrated that several of these clusters show the signatures of thermal emission in the outer parts. A strong signature is the presence of redshifted O VII emission at 0.57 keV. In the central parts, several clusters show also a soft excess, but m this case the observations cannot well discriminate between a thermal or non-thermal origin of the soft X-ray excess.

• Bulletin of the Korean Chemical Society
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• 제22권12호
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• pp.1316-1322
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• 2001

Transition metal complexes of novel mono- and di-ferrocene-substituted porphyrins have been synthesized and characterized by structural and electrochemical methods. The X-ray structures of Mn(FPTTP)Cl and Mn(DFTTP)Cl showed the distorted square pyramidal coordination geometry with syn configuration of chloride and ferrocenyl substituents. The electrochemistry of ferrocene-substituted porphyrins and their metal complexes has been determined to elucidate the ${\pi}-conjugation$ effect of the porphyrin ring. The ferrocenyl group of H2FPTTP underwent a reversible one-electron transfer process at 0.30 V, indicating the good electron donating effect of the phorphyrin ring to the ferrocene substituent. The redox potential of the ferrocenyl subunit and porphyrin ring was affected by the central metal ions of the metalloporphyrins, that is, Zn(II) and Ni(II) made the oxidation of ferrocene much easier and Mn(III) made it harder. The ferrocene subunits of H2DFTTP interacted electrochemically with each other with peak splitting of 0.21 V. The strength of the electrochemical interactions between the two ferrocenyl substituents can be controlled by central metal ions of metalloporphyrins.

• 한국방사선학회논문지
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• 제5권5호
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• pp.223-229
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• 2011

X선은 X선관 내 음극측 전자(electron)를 빠른 속도로 가속시킨 다음 진행하는 전자의 흐름을 저지극(target)에서 차단시킬 때 에너지의 변환을 일으켜 발생한다. 가속된 고속의 전자가 저지면에 충돌하는 실제면적을 실초점(actual focal spot)이라 하고, 실초점의 크기를 X선이 나오는 방향인 중심선(central ray)측에서 관측할 경우 축소되어 작게 보이는데 이때의 초점을 실효초점(effective focal spot)이라고 한다. X선관 방사각에 따라 음극 측의 강도가 양극 측 보다 높게 나타나 X선 강도가 균등하지 않다. 이러한 효과를 경사각 효과(heel effect)라고 하며, 경사각 효과로 인하여 환자가 받는 피폭의 정도는 양극의 각도, 즉 실효초점의 크기에 따라 달라지게 된다. 본 논문에서는 실효초점의 크기와 그에 따른 환자 피폭선량의 상관관계를 알아보고 실효초점의 크기에 따른 균질선량 분포를 위한 효과적인 조사야를 제시하고자 한다. 결론적으로 초점크기에 따라서 평균적으로 -8cm ~ 0cm 범위에서 효과적인 조사야 범위를 찾을 수 있었고, 평균 선량률은 0.019 R/min이 나왔다. 이 범위를 이용하면 환자에게는 적은 피폭선량으로 균등한 흑화도 및 해상력을 가진 영상을 얻을 수 있을 것이다.