• 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.

• 대한전자공학회논문지SD
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• 제44권4호
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• pp.91-96
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• 2007

사파이어 기반의 GaN LED의 광추출 효율을 시뮬레이션을 이용하여 정량적으로 평가하였다. 각각의 LED는 ray-tracing 시뮬레이션을 이용하여 광추출 효율을 계산하였다. 본 연구에는 PSS(patterned sapphire substrate) LED와 flat LED의 비교 분석을 통하여, LED에서의 사파이어 기판의 패턴이 광추출에 미치는 영향을 설명하였다. 또한, 각각의 칩에서 반사막의 반사도가 광추출에 미치는 영향을 분석하고, 그 원인을 시뮬레이션을 이용하여 설명하였다. 한편, 사파이어 패턴에 의한 광추출효율의 변화 효과를 공기(air)와 실리콘(silicone) 분위기에서 시뮬레이션을 수행하였다. 이러한 시뮬레이션 기술을 통해 광추출 효율의 개선 정도를 정량적으로 평가할 수 있었으며, 이러한 연구가 향후 고효율 LED 개발에 도움을 줄 것으로 판단된다.

• 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.

• Geomechanics and Engineering
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• 제16권1호
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• pp.85-95
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• 2018

Water affects the mechanical properties of coal and stress wave propagation. To comprehensively investigate the effect of water content on the properties of coal, laboratory tests including X-Ray Diffraction (XRD) analysis, P-wave test, S-wave test, static and dynamic compression test with different water contents were conducted. The compressive strength, elastic modulus and failure strain and their mechanism of coal specimen under coupled static-dynamic load with the increased water content were observed. Meanwhile, energy transmission and dissipation characteristics of a stress wave in coal specimens with different water contents under dynamic load and its relation with the failure features, such as fragmentation and fractal dimension, of coal was analyzed. Furthermore, the dynamic interpretation of water infusion to prevent coal burst based on water infusion model of coal seam roadway was provided.

• Tuberculosis and Respiratory Diseases
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• 제70권1호
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• pp.10-20
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• 2011

Various diseases can diffusely involve central airways, including the trachea and main stem bronchi. Central airway abnormalities are frequently not apparent or are overlooked on chest radiographs, even though the patient may have significant symptoms. Recent advances in spiral and multi-detector computed tomography (CT) with multi-planar reconstruction and three-dimensional demonstration, including virtual bronchoscopy, allow for excellent display of central airway anatomy and abnormalities with visualization of accurate locations of lesions. Early detection and proper diagnosis of airway diseases based on various radiographic findings will help determine appropriate treatment, including surgical planning and evaluation of treatment response. Herein we describe and illustrate the imaging findings of a wide spectra of diffuse central airway diseases.

• 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.

• 천문학회지
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• 제37권5호
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• pp.361-369
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• 2004

Galaxy clusters as the densest and most prominent regions within the large-scale structure can be used as well characterizable laboratories to study astrophysical processes on the largest scales. X-ray observations provide currently the best way to determine the physical properties of galaxy clusters and the environmental parameters that describe them as laboratories. We illustrate this use of galaxy clusters and the precision of our understanding of them as laboratory environments with several examples. Their application to determine the matter composition of the Universe shows good agreement with results from other methods and is therefore a good test of our understanding. We test the reliability of mass measurements and illustrate the use of X-ray diagnostics to study the dynamical state of clusters. We discuss further studies on turbulence in the cluster ICM, the interaction of central AGN with the radiatively cooling plasma in cluster cooling cores and the lessons learned from the ICM enrichment by heavy elements.

• 천문학회보
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• 제44권1호
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• pp.74.1-74.1
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• 2019

We present an ongoing imaging survey of the host galaxies of hard X-ray-selected active galactic nuclei (AGNs) observed with the Hubble Space Telescope (HST). The snapshot images are taken with the Advanced Camera for Surveys through an HST gap-filler program. The sample, selected from the 70-month Swift-BAT X-ray source catalog, represents an unbiased and uniform AGN population, which will enable us to test the AGN unification model and explore the physical connection between host galaxies and central supermassive black holes. We also plan to investigate the AGN triggering mechanism by examining merger signatures and searching for dual nuclei. We present the pipeline for imaging analysis and the current status of the survey.

• Journal of Astronomy and Space Sciences
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• 제30권3호
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• pp.123-125
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• 2013

2FGL J1823.8+4312 and 2FGL J1304.1-2415 are two unidentified Fermi objects which are associated with cluster of galaxies. In order to exam the possibility of cluster of galaxies as gamma-ray emitters, we search for counterpart of these two unidentified Fermi objects in other wavebands. However, we find other candidate to be more likely the counterpart of the unidentified Fermi object for both sources. We compare their light curves and SEDs in order to identify their source types. However, data at millimeter and sub-millimeter wavebands, which is important for us to constrain the SED at synchrotron peak, is lacking of measurement. Therefore, we proposed to SMA observation for these two sources. We have got data and are doing further analysis.

• 한국정보디스플레이학회:학술대회논문집
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• 한국정보디스플레이학회 2008년도 International Meeting on Information Display
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• pp.330-332
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• 2008

Banana-shaped molecules were synthesized introducing ester linking group into mesogenic unit, varying the central unit with 1,6-, 2,3-naphthylenes, and introducing the hexyloxy group as the terminal flexible unit. The properties of the compounds were characterized by FT-IR, NMR spectroscopy, DSC, polarizing optical microscopy, and X-ray diffractometry.