• Journal of The Korean Digital Architecture Interior Association
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• v.6 no.2
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• pp.25-30
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• 2006

The purpose of this study was to investigate how student felt the strengths and shortness of presentation methods for formation of interior spaces. For this study, the process of the interior architecture design class was divided into three stages: the programming. the design development, and the design completion. In the design development stage, students used presentation methods: hand sketch, scale model, computer modeling, and virtual realty. The strengths of hand sketch was that quick expression. Models provided three-dimensional feelings. Computer modelling provide realistic color and texture. Virtual reality provided three-dimensional immersion and real scale. It is effective that students collect brain storm images using quick hand sketch in the beginning of design development stage. After that, they compose interior spaces in study models with small scale. Watching the models, they design details of spaces by using hand sketch and computer modelling. Using virtual reality, they can check the scale and circulation. Finally, they complete computer modelling by texture mapping and check the final design in virtual reality.

• Bulletin of the Korean Space Science Society
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• 2011.04a
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• pp.21.1-21.1
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• 2011

우리는 분리형 쌍성 11개(원궤도 7개, 타원궤도 4개), 반분리형 쌍성 7개와 접촉형 쌍성 9개(근첩촉형 3개, 접촉형 2개, 초과 접촉형 4개)를 포함하는 27개의 다양한 종류의 표준식쌍성의 분석하여 절대량을 구하였다. 표준 식쌍성은 식쌍성의 광도곡선이 적어도 두 파장 영역 이상에서 그리고 모든 위상에서 골고루 관측되었고, 쌍성의 두 구성원 별에 대하여 시선속도 곡선이 발표된 식쌍성, 즉, 이중분광선 식쌍성 (Double line spectroscopic eclipsing binariy)으로 정의한다. 우리는 표준식쌍성의 370개의 후보에 대하여 문헌을 조사하여 관측 데이터를 확보 하였다. 이중에서 시선속도곡선과 광도곡선 자료가 동시에 존재하는 식쌍성은 80개이다. 이번 연구에서 우리는 표준식쌍성의 관측 질을 고려하여 27개의 식쌍성을 선택하여 절대량을 계산하였고, 이전 연구자들이 발표한 절대량과 비교 하였다. 이 논문에서 제시한 표준식쌍성의 유용성을 확인하기 위해 소마젤란은하에서 발견한 식쌍성의 광도곡선을 분석하여 측광학적인 해를 구하는 작업을 수행하였다. 이를 위하여 표준 식쌍성을 식쌍성의 종류별로 구분하고, 소마젤란은하에서 발견된 식쌍성 20여개를 선정하였다. 선정된 식쌍성을 표준식쌍성의 광도곡선과 형태를 비교하여 초기값을 결정하였고, 반복적인 차등보정법으로 측광학적인 해를 구하였다. 이 논문에서 제시한 표준식쌍성이 소마젤란은하에서 발견된 식쌍성들의 광도곡선의 형태를 대부분 포함하는 다양한 분포로 형성되어 있고, 이에 따른 측광학적인 해가 관측과 잘 일치함을 보여주고 있다.

• Journal of Astronomy and Space Sciences
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• v.23 no.4
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• pp.435-444
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• 2006

Since artificial space objects are observable only in a short period of time and the characteristics of their motion is not exactly predictable, it is difficult to obtain both photometric and spectroscopic data by a set of observations. We have, therefore, designed a mount to load multi-optical instruments on the Kyung Hee University (KHU) satellite tracking and observation system for both photometric and spectroscopic observations of artificial space objects. In this paper, we have calculated the deformation of the remodeled mount using structural analyses for the loading of the multi-optical instruments. We have also deduced pointing errors of the mount occurring at tracking and observing artificial space objects. we have derived tracking reliably artificial space objects in our field of view and confirmed structural safety test of mount utilizing equivalent (von-mises) stress distribution.

• Journal of Astronomy and Space Sciences
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• v.16 no.2
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• pp.241-254
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• 1999

Differential time-series observations of BL Camelopardalis classified as a double mode SX Phoenicis type variable were secured with a charge coupled device. The observed photometric data was reduced using the IRAF Package and the differential magnitudes were obtained through aperture photometry. The periods of BL Cam were analyzed with the Generalized Least-Square Method by Vanicek (1971) and the Fourier Decomposition Method. It was found that the first and second period of BL Cam were 0.0391 day respectively which lead the period ratio of P1/P0=0.81. This period ratio is much different from 0.78 determined by other investigators and also much more larger than that of other double-mode SX Phe type variables. In addition, this period ratio is much different from the value expected from the relation between the metallicity and period ratio. From these results, it can be confirmed that BL Cam is the most extreme case among all double-mode SX Phe type variables.

• The Bulletin of The Korean Astronomical Society
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• v.37 no.1
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• pp.70.1-70.1
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• 2012

CQUEAN (Camera for QUasars in EArly uNiverse)은 초기우주천체 연구단(Center for Exploration of Origin of the Universe) 사업에서 개발한 CCD 카메라로서 초기우주의 퀘이사 후보를 찾기 위한 목적으로 설계되었다. CCD를 구동할 때는 픽셀 다이오드의 PN 접합층에 공핍층(depletion layer)을 생성하기위해 역 바이어스 전압을 준다. 이 전압에 의해 CCD를 사용한 관측 시 광이온화와 열이온화 현상에 의해 생성된 전자의 전하값에 추가로 바이어스 값이 읽혀진다. 정확한 CCD 측광 결과를 얻어내기 위해서는 안정된 바이어스를 유지해야 한다. 본 연구에서는 향후 CQUEAN의 보다 정확한 관측 및 데이터 처리에 대비하여 CQUEAN의 바이어스 특성을 분석하여 이 값에 영향을 주는 요인을 찾고 해결책을 논의한다.

• The Bulletin of The Korean Astronomical Society
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• v.37 no.2
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• pp.94.1-94.1
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• 2012

국내의 교육기관에서는 망원경과 검출장비의 한계로 천체의 측광관측에 중점을 둔 실험교육을 하고 있으며 천체의 물리, 화학적 특성을 이해하는데 필수적인 천체분광 실험교육은 원활하지 못한 상황이다. 천체분광 실험 교육을 위하여 과학교육용 실험장비인 랩주니어(Lab-Junior)를 이용하여 소형망원경으로도 천체의 스펙트럼을 얻을 수 있는 어댑터를 개발하였다. 5인치 망원경에 랩주니어 장비를 장착하여 달과 행성의 태양반사 스펙트럼을 얻을 수 있었고 12인치 망원경에 장착하여 데네브(deneb) 같은 밝은 천체의 스펙트럼을 얻을 수 있었다. 이 발표에서는 랩주니어를 이용하여 관측된 스펙트럼 데이터를 분석해 보고 학교 현장에서 교육적 활용 방안을 소개하고자 한다. 개발된 장비를 활용한다면 고가의 분광장치가 없는 학교나 천문교육시설에서도 손쉽게 천체분광 실험 교육프로그램을 운영할 수 있을 것이다.

• Proceedings of the Korean Institute of IIIuminating and Electrical Installation Engineers Conference
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• 2004.05a
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• pp.217-222
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• 2004

사진 측광은 일시에 대량의 데이터를 얻을 수 있으므로 시간에 따라 빛이 변화하는 주광의 측정 수단으로 이용될 수 있다. 이를 위하여 자연광 아래에서 디지털 이미지와 휘도 측정치의 보정실험을 행하였으나 청공광과 백색시료를 제외한 나머지 시료에 대해서는 그리 만족스러운 결과를 가져오지 못하였다. 앞으로 Videophotometry를 실현하기 위해서는 피 계측면의 분광 반사특성에 의한 계측치의 오차를 제거하기 위한 CCD 소자의 시감도 보정, 시야를 정확하게 재현하기 위한 광학적 연구, 인간의 시각 특성에 부합하는 측정 휘도의 보정 등에 대한 연구가 이루어져야 할 것이다.

• Journal of Astronomy and Space Sciences
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• v.19 no.1
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• pp.67-74
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• 2002

Optical observations of Geostationary and Molynia orbit spin-stabilized satellites over the Korean peninsula have been carried out at the Kyung Hee University Observatory with a 30 inch telescope. We have observed 5 spin-stabilized satellites, and obtained 0spin periods, which can be used for deducing a design for each bus model. Verifications of spin periods of 3 known satellites from manufacturer, and observations of 2 unknown satellites were made. The difference between known spin periods and observed spin periods is 0.06sec on the average and the difference of those spin rates is 3.3rpm on the average. Those results indicate that spin periods and spin rates of observed geostationary spin-stabilized satellites are within operating limits. Spin rates of unknown satellites, Fengyun 2B and Molynia 1-87 are 89.3rpm, 78.4rpm earh. It is suggested that the research of spin stabilized satellites can be used for the determinations of standard light sources for short period celestial objects and helpful for the constructions of satellite databases with photometric and/or spectroscopic satellite observations.

• Journal of Astronomy and Space Sciences
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• v.22 no.3
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• pp.329-352
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• 2005

Long term observations of full-disk Lyman-o irradiance have been made by the instruments on various satellites. In addition, several sounding rockets dating back to the 1950s and up through the present have measured the $Lyman-{\alpha}$ irradiance. Previous full disk $Lyman-{\alpha}$ images of the sun have been very interesting and useful scientifically, but have been only five-minute 'snapshots' obtained on sounding rocket flights. All of these observations to date have been snapshots, with no time resolution to observe changes in the chromospheric structure as a result of the evolving magnetic field, and its effect on the Lyman-o intensity. The $Lyman-{\alpha}$ Imaging Solar Telescope(LIST) can provide a unique opportunity for the study of the sun in the $Lyman-{\alpha}$ region with the high time and spatial resolution for the first time. Up to the 2nd year development, the preliminary design of the optics, mechanical structure and electronics system has been completed. Also the mechanical structure analysis, thermal analysis were performed and the material for the structure was chosen as a result of these analyses. And the test plan and the verification matrix were decided. The operation systems, technical and scientific operation, were studied and finally decided. Those are the technical operation, mechanical working modes for the observation and safety, the scientific operation and the process of the acquired data. The basic techniques acquired through the development of satellite based solar telescope are essential for the construction of space environment forecast system in the future. The techniques which we developed through this study, like mechanical, optical and data processing techniques, could be applied extensively not only to the process of the future production of flight models of this kind, but also to the related industries. Also, we can utilize the scientific achievements which are obtained throughout the project And these can be utilized to build a high resolution photometric detectors for military and commercial purposes. It is also believed that we will be able to apply several acquired techniques for the development of the Korean satellite projects in the future.