• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2008년도 한국우주과학회보 제17권2호
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• pp.22.3-22.3
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• 2008

We present the results of the investigations of high dispersion spectra of two stars. These are the eclipsing binary RR Lyn, and $\rho$ Pup - the prototype of the group of pulsating variables. The spectra were obtained at 1.8 m Bohyuunsan observatory telescope, and 8.2 m VLT. We found the chemical composition. The both components of RR Lyn are Am stars (metallic line stars), but the abundance patterns of the components are not similar - the iron abundance and the abundances of other elements are surely different. For few elements the differences exceeds 1 dex. We found the abundances of 56 chemical elements in the atmosphere of $\rho$ Pup. This is one of the best stellar abundance patterns. It permits to investigate the role of the charge-exchange reactions in stellar atmospheres. These reactions can produce the abundance anomalies in the atmospheres of B-F type stars. These reactions can be one of the sources of galactic cosmic rays, and the reason of the braked rotation of A-F type chemically peculiar stars.

• 응용통계연구
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• 제18권2호
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• pp.411-420
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• 2005

본 논문에서는 불균형 일원랜덤효과모형에서 분산성분에 대한 MIVQUE 추정량들의 효율에 대하여 연구하였다. MIVQUE 추정량에 대한 초기 추정치로 3가지 추정치가 사용되었으며 이들을 이용하여 얻어지는 MIVQUE 추정량의 효율성을 척도화된 추정량의 경험적 분위수를 이용하는 EQDGs 플롯을 이용하여 비교하였다. 모의실험 결과 집단간 분산의 초기치를 0으로 하고 집단내 분산의 초기치를 1로 사용한 MIVQUE 추정량의 효율이 추정량의 안정성 관점에서 다른 초기치를 사용한 MIVQUE 추정량에 비하여 약간 효율적인 것으로 나타났다.

• 한국지반공학회:학술대회논문집
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• 한국지반공학회 2010년도 춘계 학술발표회
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• pp.1294-1301
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• 2010

This study is an experimental research for the dispersion behavior and impact characteristics of debris flow according to change of slope. Large scale experimental setup for the debris flow was established to simulate the artificial rainfall and control the ground slope. Parameters such as materials of debris flow, slope, and length of slope were used for the experiments. After the experiments, it was found that the speed of ground material components was increased about 28~47%. It was found that speed can be increased by increasing the particle size. Furthermore, maximum/final loads for ground material components were increased 89% for the coarse aggregate and 68% for the fine aggregate comparing with sand.

• Wind and Structures
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• 제19권5호
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• pp.541-563
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• 2014

This paper investigates the topographic effects on wind characteristics over hilly terrain, based on wind data recorded at a number of meteorological stations in or near complex terrain. The multiply data sources allow a more detailed investigation of the flow field than is normally possible. Vertical profiles of mean and turbulent wind components from a Sodar profiler were presented and then modeled as functions of height and wind speed. The correlations between longitudinal and vertical wind components were discussed. The phenomena of flow separation and generation of vortices were observed. The distance-dependence of the topographic effects on gust factors was revealed subsequently. Furthermore, the canyon effect was identified and discussed based on the observations of wind at a saddle point between two mountain peaks. This study aims to further understanding of the characteristics of surface wind over rugged terrain. The presented results are expected to be useful for structural design, prevention of pollutant dispersion, and validation of CFD (computational fluid dynamics) models or techniques over complex terrains.

• Journal of the Korean Data and Information Science Society
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• 제22권4호
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• pp.803-809
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• 2011

Properties of multivariate Shewhart and CUSUM charts for monitoring variance-covariance matrix, specially focused on correlation coefficient components, are investigated. The performances of the proposed charts based on control statistic Lawley-Hotelling $V_i$ and likelihood ratio test (LRT) statistic $TV_i$ are evaluated in terms of average run length (ARL). For monitoring correlation coe cient components of dispersion matrix, we found that CUSUM chart based on $TV_i$ gives relatively better performances and is more preferable, and the charts based on $V_i$ perform badly and are not recommended.

• 천문학회보
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• 제45권1호
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• pp.61.1-61.1
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• 2020

We examine the HI gas kinematics and distribution of galaxy pairs in group or cluster environment from high-resolution Australian Square Kilometre Array Pathfinder (ASKAP) WALLABY pilot observations. We use 22 well-resolved galaxies in the Hydra cluster of which 4 galaxies are visually identified as pairs and others are isolated ones. We perform profile decomposition of HI velocity profiles of the galaxies using a new tool, BAYGAUD which enables us to separate a line-of-sight velocity profile into an optimal number of Gaussian components based on Bayesian MCMC techniques. All the HI velocity profiles of the galaxies are decomposed into kinematically cold or warm gas components with their velocity dispersion, 4~8 km/s or > 8 km/s, respectively. We derive the mass fraction of the kinematically cold gas with respect to the total HI gas mass, f = log10(M_cold / M_HI), of the galaxies and correlate them with their dynamical mass. The cold gas reservoir of the paired galaxies in the Hydra cluster is found to be relatively higher than that of the isolated ones which show a negative correlation with the dynamical mass in general.

• 한국세라믹학회지
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• 제44권5호
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• pp.179-183
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• 2007

BCB $Resin-BaNd_2Ti_4O_{12}$(BNT) composites with BNT contents were prepared by tape casting method and epoxy resin-BNT composites were prepared by using heating press. Their dielectric properties and microstructures were investigated. The dielectric properties such as dielectric constant and dielectric loss at 1 MHz for epoxy resin-BNT composites and BCB resin-BNT composites are improved with an increase of BNT volume fraction. The dielectric constant of the Epoxy-BNT composite increased from 5.9 to 7.8 as the volume fraction of BNT increased from 15 to 25. The dielectric constant of the BCB-BNT composite increased from 9.1 to 15.5 as the volume fraction of BNT increased from 30 to 50. The dielectric behavior of BCB-BNT system can be explained by Lichtenecker's equation. The dielectric constant of epoxy resin-BNT composite is smaller than that of BCB resin-BNT composite. These results are considered to be related with the dispersion of BNT filler in polymer matrix from the result of SEM photograph.

• 천문학회보
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• 제40권2호
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• pp.32.3-33
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• 2015

There exist scaling relations that link the mass of supermassive black holes with both the velocity dispersion and the mass of the central stellar cusp of their host galaxies. This implies that these two components grow in tandem. Feedback from actively accreting supermassive black holes (AGN), in the form of multi-phase gas outflows, has been argued to be the agent of this co-evolution. Here we employ the powerful GMOS integral field spectroscopy unit on the 8.2m Gemini-North telescope to investigate ionized gas outflows of luminous Type 2 AGN in the local Universe (z<0.1). Our sample of 6 galaxies is drawn from the Sloan Digital Sky Survey (SDSS) and was selected based on their [OIII] dust-corrected luminosity (>1042 erg/s) and signatures of outflows in the [OIII] line profile of their spatially integrated SDSS spectra. These are arguably the best candidates to explore AGN feedback in action since they are < 1% of a large local type 2 AGN SDSS sample selected based on their [OIII] kinematics. We combine a careful spectral decomposition of the [OIII] and $H{\alpha}$ line profiles with spatial information on ~0.5kpc scales to understand the outflow kinematics and energetics in these objects. We find clear evidence for strong outflows in [OIII] and occasionally $H{\alpha}$ that are clearly driven by the ionizing radiation of the AGN. We kinematically and spatially decompose outflowing and rotating ionized gas components. We find [OIII] to be a better tracer of AGN outflows, while $H{\alpha}$ appears to be strongly affected by both stellar rotation and outflows induced by ongoing star formation. The observed kinematics and spatial distribution of the ionized gas imply a large opening angle for the outflow. Finally, we find the projected outflow velocity to decrease as a function of distance, while its dispersion shows a more complex structure with a potentially initially increasing trend (out to 0.5-1kpc distances).

• Nuclear Engineering and Technology
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• 제24권1호
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• pp.40-51
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• 1992

연구용 원자로의 분산형 핵연료에 대한 노내 조사 거동의 주요 특성중의 하나는 핵연료심 팽윤에 기인된 핵연료봉 직경 증가이다. 본 논문에서는 분산형 우라늄실리사이드 핵연료에 대한 노내 조사거 동과 실험 증거들을 분석함으로써 그 핵연료의 팽윤에 대한 물리적 해석 모형인, DFSWELL 전산 모형을 개발하였다. 문헌에 보고된 실험 증거들로부터 노내에서 U$_3$Si-Al 핵연료심의 부피변화는 온도와 핵분열율에 따라 크게 영향을 받는 것으로 나타났다. 분산형 우라늄 실리사이드 핵연료에 대한 정량적 팽윤량은 주어진 온도, 핵분열율, 핵분열고체생성물 측적 및 핵분열기체 기포거동을 고려함으로써 평가될 수 있다. 연구로의 분산형 우라늄실리사이드 핵연료의 팽윤 현상은 다음과 같은 세 가지 현상으로 귀결된다. i ) 핵분열기체생성물 기포 생성/축적에 치한 부피변화 ii ) 고체 핵분열생성물의 축적 및 상 변화에 의한 부피변화 iii ) 핵연료 입자와 기지 사이의 공유층에 대한 부피변화 상기 세 가지의 물리 적 현상을 고려하는 본 DFSWELL 전산 모형의 출력이력 조건에 따른 절대 예측치들은 실행 결과와 비교할 때 분산형 우라윰실리 사이드 핵연료의 조사추 팽윤 실측치와 잘 일치한다.

• 대한전자공학회논문지SP
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• 제40권1호
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• pp.20-27
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• 2003

본 논문에서는 사용자가 질의를 원하는 물체 영역을 선택하면 유사 물체를 영상 데이터베이스 내에서 검색할 수 있는 내용기반 영상검색 시스템을 구현하였다. 질의영상은 색상성분과 그레이성분으로 나누어져 웨블릿 변환되고 색상성분에서는 컬러 오토코릴로그램과 분산으로 색상특성을 추출한다. 그리고 그레이성분에서는 오토코릴로그램과 GLCM을 통해 질감특성을 추출한다. 이렇게 구한 2개 성분에서의 특성들을 이용하여 데이터베이스내의 영상들과 각각 유사도를 비교하여 검색하게 된다. 이때 각 유사도에 가중치를 적용하였다. 한 가지 성분보다 두 가지 성분에서 특성을 구하여 각각의 단점을 보완하였고 실험 결과에서도 소환성(recall) 및 정확성(precision)이 향상됨을 볼 수 있었다 또한 가중치를 적용함으로써 검색 효율이 개선되었다. 그리고 데이터베이스내 영상들의 여러 특성을 특성 라이브러리내에 자동 색인화 시킴으로써 고속의 영상 검색이 가능하였다.