• 지구물리와물리탐사
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• 제10권4호
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• pp.241-251
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• 2007

본격적인 지진관측 이래 최대 규모의 내륙 지진으로 기록된 오대산지진의 관측 스펙트럼을 이용하여, 점지진원 스펙트럼 모델의 지진원 크기 및 오차의 공간적인 특성을 평가하였다. 먼저 지진원 스펙트럼을 추정하기 위해, 최근까지 국내에 축적된 지진자료를 기반으로 비교적 상세하게 추정된 추계학적 지진동모델(Boore, 2003)의 지진파 전달, 부지특성(연관희, 2007)을 이용하여 관측 자료를 보정하였다. 추정된 오대산지진의 지진원 스펙트럼을 $1-f_c$(1개의 코너주파수) Brune의 ${\omega}^2$ 지진원모델에 적합한 결과, 기존에 제시된 지진규모-응력강하량 대표모델(연관희 등, 2006)에 의해 잘 예측되었으며, 오대산지진의 지진원 스펙트럼은 최근까지 한반도 인근에서 발생한 중규모 이상의 지진원 스펙트럼으로부터 추정된 $2-f_c$(2개의 코너주파수)의 경험적인 지진원모델에 보다 잘 부합되었다. 또한 일반적으로 무작위 잡음으로 취급되는 점지진원 지진파 스펙트럼 모델링 오차에 대해 방위각에 따른 방향성과 지역별 전달특성을 평가한 결과, 오차가 완전한 무작위 특성이 아님을 확인할 수 있었다. 이러한 모델링 오차의 방향성은 이론적으로 추정된 방사패턴과도 매우 유사한 관측된 방사패턴을 나타내었으며, 지역별로는 지질학적인 경계 혹은 지진파전달의 불연속적 특성과 밀접한 관계가 있는 것으로 판단되는 주파수별로 상이한 공간적인 분포 특성을 보여주었다.

• Journal of Radiation Protection and Research
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• 제40권1호
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• pp.55-64
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• 2015

방사선치료계획장치의 핵심기술인 선량분포 계산은 빠르고 정확함을 요구한다. 기존 상용화된 치료계획장치의 선량 계산 방법은 빠르지만 정확성이 부족하고, 몬테칼로 방법은 시뮬레이션 시간과다 문제가 있다. 관심영역의 일부만 몬테칼로 방법이 계산하고 나머지 영역은 비선형함수사상 능력이 뛰어난 신경회로망이 계산하는 시스템은 상대적으로 빠르고 정확한 선량분포를 계산해낼 수 있다. 비균질 매질의 선량분포에 나타나는 불연속점과 변곡점의 특성을 신경회로망이 학습가능 하다는 것을 사전 작업을 통해 확인하였다. 이때 사용된 신경회로망은 Feedforward Multi-Layer Perceptron에 Scaled Conjugated Gradient 알고리즘과 Levenberg-Marquardt 알고리즘으로 각각 학습하여 성능비교를 하였고, 은닉층의 뉴런 개수에 따른 성능비교도 하였다. 마지막으로 균질매질의 팬텀에 대해 상용 치료계획장치의 선량계산 알고리즘으로 계산한 선량분포를 사전작업을 통해 확인된 신경회로망에 학습하여 깊이선량율의 평균제곱오차가 0.00214인 결과를 보여주었다. 균질 및 비균질 매질의 팬텀에 대한 3차원 선량분포를 계산하는 신경회로망 모델 개발 연구가 추가로 진행될 것이다.

• 한국의학물리학회:학술대회논문집
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• 한국의학물리학회 2002년도 Proceedings
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• pp.53-60
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• 2002

Motion of lung tumors from respiration has been reported in the literature to be as large as of 1-2 cm. This motion requires an additional margin between the Clinical Target Volume (CTV) and the Planning Target Volume (PTV). While such a margin is necessary, it may not be sufficient to ensure proper delivery of Intensity Modulated Radiotherapy (IMRT) to the CTV during the simultaneous movement of the DMLC. Gated treatment has been proposed to improve normal tissues sparing as well as to ensure accurate dose coverage of the tumor volume. The following questions have not been addressed in the literature: a) what is the dose error to a target volume without gated IMRT treatment\ulcorner b) what is an acceptable gating window for such treatment. In this study, we address these questions by proposing a novel technique for calculating the 3D dose error that would result if a lung IMRT plan were delivered without gating. The method is also generalized for gated treatment with an arbitrary triggering window. IMRT plans for three patients with lung tumor were studied. The treatment plans were generated with HELIOS for delivery with 6 MV on a CL2100 Varian linear accelerator with a 26 pair MLC. A CTV to PTV margin of 1 cm was used. An IMRT planning system searches for an optimized fluence map ${\Phi}$ (x,y) for each port, which is then converted into a dynamic MLC file (DMLC). The DMLC file contains information about MLC subfield shapes and the fractional Monitor Units (MUs) to be delivered for each subfield. With a lung tumor, a CTV that executes a quasi periodic motion z(t) does not receive ${\Phi}$ (x,y), but rather an Effective Incident Fluence EIF(x,y). We numerically evaluate the EIF(x,y) from a given DMLC file by a coordinate transformation to the Target's Eye View (TEV). In the TEV coordinate system, the CTV itself is stationary, and the MLC is seen to execute a motion -z(t) that is superimposed on the DMLC motion. The resulting EIF(x,y)is inputted back into the dose calculation engine to estimate the 3D dose to a moving CTV. In this study, we model respiratory motion as a sinusoidal function with an amplitude of 10 mm in the superior-inferior direction, a period of 5 seconds, and an initial phase of zero.

• 한국응용약물학회:학술대회논문집
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• 한국응용약물학회 2007년도 Proceedings of The Convention
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• pp.153-158
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• 2007

Background: Naturally occurring antioxidants were used to regulate the skin damage caused by ultraviolet (UV) radiation because several antioxidants have demonstrated that they can inhibit wrinkle formation through prevention of matrix metalloproteinases (MMPs) and/or increase of collagen synthesis. We examined the effect of oral administration of the antioxidant mixture ("L-Skin Care") on UVB-induced wrinkle formation. In addition, we investigated the possible molecular mechanisms of photoprotection against UVB through inhibition of collagen-degrading MMP activity or through enhancing of pro collagen synthesis in mouse dorsal skin. Methods: Female SKH-l hairless mice were orally administrated "L-Skin Care" (test group) or vehicle (control group) for 10 weeks with UVB irradiation by three times a week. The intensity of irradiation was gradually increased from 30 to $180mJ/cm^2$. Microtopographic and histological assessments of the dorsal skins were carried out at the end of 10 weeks to evaluate wrinkle formation. Western blot analysis and EMSA were also carried out to investigate the changes in the balance of collagen synthesis and collagen degradation. Results: Our "L-Skin Care" significantly reduced UVB-induced wrinkle formation, accompanied by significant reduction of epidermal thickness, and UVB-induced hyperplasia, acanthosis and hyperkeratosis. Oral administration of "L-Skin Care" significantly prevented UVB-induced expressions of MMPs, mitogen-activated protein (MAP) kinases and activation of activator protein (AP)-1 transcriptional factor in addition to enhanced type I procollagen and transforming growth factor-$\beta$ (TGF-$\beta$) expression. Conclusion: Oral administration of "L-Skin Care" significantly inhibited wrinkle formation caused by chronic UVB irradiation through significant inhibition of UVB-induced MMP activity accompanied with enhancement of collagen synthesis.

• 천문학논총
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• 제27권4호
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• pp.117-122
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• 2012

The interstellar dust grains are formed and supplied to interstellar space from asymptotic giant branch (AGB) stars or supernova remnants, and become constituents of the star- and planet-formation processes that lead to the next generation of stars. Both a qualitative, and a compositional study of this cycle are essential to understanding the origin of the pre-solar grains, the missing sources of the interstellar material, and the chemical evolution of our Galaxy. The AKARI/MIR all-sky survey was performed with two mid-infrared photometric bands centered at 9 and $18{\mu}m$. These data have advantages in detecting carbonaceous and silicate circumstellar dust of AGB stars, and the interstellar polycyclic aromatic hydrocarbons separately from large grains of amorphous silicate. By using the AKARI/MIR All-Sky point source catalogue, we surveyed C-rich and O-rich AGB stars in our Galaxy, which are the dominant suppliers of carbonaceous and silicate grains, respectively. The C-rich stars are uniformly distributed across the Galactic disk, whereas O-rich stars are concentrated toward the Galactic center, following the metallicity gradient of the interstellar medium, and are presumably affected by the environment of their birth place. We will compare the distributions of the dust suppliers with the distributions of the interstellar grains themselves by using the AKARI/MIR All-Sky diffuse maps. To enable discussions on the faint diffuse interstellar radiation, we are developing an accurate AKARI/MIR All-Sky diffuse map by correcting artifacts such as the ionising radiation effects, scattered light from the moon, and stray light from bright sources.

• 한국지구과학회지
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• 제32권2호
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• pp.190-199
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• 2011

지형 효과가 포함된 태양복사 모델(GWNU)을 이용한 한반도의 태양광 자원지도를 개발하였다. 태양복사 모델의 입력 자료는 위성 관측 자료(MODIS, OMI, MTSAT-1R)와 수치 모델(RDAPS) 자료를 사용하였으며 특히 고해상도 지형 자료를 이용하여 지형 효과에 따른 한반도의 지표면 태양광 변화를 계산하였다. 계산 결과를 월 및 연 누적하여 분석하였을 때 여름철은 태양 고도각이 높아 지형 효과에 영향이 10% 이하로 적은 반면 겨울철은 20% 이상의 큰 차이가 나타났다. 또한 4 km 해상도의 지표면 태양광의 경우보다 1 km 해상도의 경우 지형 효과 포함에 따른 태양광 차이가 약 2배 정도 크게 나타났다. 즉 지표면에 도달하는 태양광을 정확히 모델링하기 위해서는 입력 자료뿐만 아니라 정확하고 고해상도의 지형 자료가 필연적이며 지형효과는 더욱 뚜렷이 나타나 실제와 유사할 것이다.

• International Journal of Concrete Structures and Materials
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• 제7권2호
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• pp.95-110
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• 2013

We report various synchrotron radiation laboratory based techniques used to characterize cement based materials in nanometer scale. High resolution X-ray transmission imaging combined with a rotational axis allows for rendering of samples in three dimensions revealing volumetric details. Scanning transmission X-ray microscope combines high spatial resolution imaging with high spectral resolution of the incident beam to reveal X-ray absorption near edge structure variations in the material nanostructure. Microdiffraction scans the surface of a sample to map its high order reflection or crystallographic variations with a micron-sized incident beam. High pressure X-ray diffraction measures compressibility of pure phase materials. Unique results of studies using the above tools are discussed-a study of pores, connectivity, and morphology of a 2,000 year old concrete using nanotomography; detection of localized and varying silicate chain depolymerization in Al-substituted tobermorite, and quantification of monosulfate distribution in tricalcium aluminate hydration using scanning transmission X-ray microscopy; detection and mapping of hydration products in high volume fly ash paste using microdiffraction; and determination of mechanical properties of various AFm phases using high pressure X-ray diffraction.

• 핵의학기술
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• 제18권2호
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• pp.3-7
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• 2014

CT를 기반으로 감쇠보정이 시행되는 SPECT/CT 검사에서는 금속 삽입물에 의한 선속경화현상으로 인접한 부위의 과대평가를 유발하며, 영상의 질을 저하시킨다. 이에 대해, 본 연구에서는 인공고관절이 삽입된 팬텀을 이용하여 감쇠보정지도의 매개변수 변화에 따른 금속 인공물이 SPECT/CT 영상에 미치는 영향을 알아보고자 한다. SPECT/CT 장비는 Siemens사의 Symbia T16을 사용하였다. SPECT/PET 팬텀에 인공고관절을 삽입하고, CT영상에서 Bright Streak 영역에 직경 17 mm의 구를 배후방사능 대비 8배가 되도록 Tc-99m을 채웠다. 이후 감쇠보정지도에서 Wide Beam Coefficient[수동모드(0.1~0.9), 자동모드]변화에 따른 열소와 배후방사능의 계수를 측정하였고, 고관절의 유무에 따라 Metal과 Non-Metal의 병소 대 배후방사능 비(Region to Background Ratio, RBR)를 산출 및 비교 분석하였다. 수동모드의 값이 증가할수록 Metal과 Non-Metal의 열소 계수는 증가하는 경향을 나타냈으며, 수동모드 0.4와 0.5에서 두 군과의 열소 계수비가 가장 일치하게 나타났다(수동모드 0.4=1.001, 0.5=0.999). 또한 $RBR^{Metal}$과 $RBR^{Non-Metal}$의 비는 자동모드에서 1.135이였고, 수동모드 0.4와 0.5에서 통계적으로 유의한 차이를 보이지 않았다(0.4=0.999, 0.5=1.028, p=0.78). 감쇠보정지도에서 Wide Beam Coefficient의 자동모드는 13.52% 과 보정 되는 것을 알 수 있었으며, 수동모드 중 0.4와 0.5에서 인공물에 의한 과 보정을 최소화 할 수 있었다. 이를 활용하여 환자에게 적용하기 위해서는 추가적인 연구가 이루어져야 할 것이며, 고관절전치환술 환자의 인공고관절 주변에서 금속 인공물에 의한 과 보정을 감소시켜 진단능을 향상시킬 수 있을 것으로 사료된다.

• 천문학회보
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• 제42권2호
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• pp.42.2-42.2
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• 2017

The Large Magellanic Cloud (LMC) is a unique target to study the detail structures of molecular clouds and star-forming regions, due to its proximity and face-on orientation from us. Most part of the astrophysical subjects for the LMC have been investigated, but the magnetic field is still veiling despite its role in the evolution of the interstellar medium (ISM) and in the main force to influence the star formation process. Measuring polarization of the background stars behind interstellar medium allows us to describe the existence of magnetic fields through the polarization vector map. In this presentation, I introduce the near-infrared polarimetric results for the $39^{\prime}{\times}69^{\prime}$ field of the northeastern region of the LMC and the N159/N160 star-forming complex therein. The polarimetric observations were conducted at IRSF/SIRPOL 1.4 m telescope. These results allow us to examine both the global geometry of the large-scale magnetic field in the northeastern region and the close structure of the magnetic field in the complex. Prominent patterns of polarization vectors mainly follow dust emission features in the mid-infrared bands, which imply that the large-scale magnetic fields are highly involved in the structure of the dust cloud in the LMC. In addition, local magnetic field structures in the N159/N160 star-forming complex are investigated with the comparison between polarization vectors and molecular cloud emissions, suggesting that the magnetic fields are resulted from the sequential formation history of this complex. I propose that ionizing radiation from massive stellar clusters and the expanding bubble of the ionized gas and dust in this complex probably affect the nascent magnetic field structure.

• 한국발생생물학회:학술대회논문집
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• 한국발생생물학회 1998년도 제4차 학술발표대회 및 정기총회
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• pp.50-51
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• 1998

guanidinoacetate methyltransferase (GAMT) catalyzes the last step of creatine biosynthesis in mammals. Creatine plays an important role in cellular energy metabolism in variety of tissues including brain and male reproductive tract. Congenital deficiency of the enzyme leads to a neurologic disorder in humans. We used an interspecific backcross DNA panel to map Gamt to the central region of mouse Chromosome (Chr) 10 near the locus of hesitant mutation affecting male fertility. We assigned the human GAMT gene to Chr 19 by PCR analysis of a human/rodent somatic hybrid cell line DNA panel, and further localized the human gene to Chr 19 at band p13.3 by PCR analysis of a human radiation hybrid DNA panel. Human chr 19p13.3 is homologous to the central part of mouse Chr 10 where mouse Gamt is located. Furthermore, this part of mouse Chr 10 contains mutant loci the phenotype of which is similar to the GAMT deficiency in human.