• 천문학회보
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• 제21권
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• pp.20.2-20.2
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• 1996

• 천문학회보
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• 제31권2호
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• pp.60.1-60.1
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• 2006

• 지구물리와물리탐사
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• 제18권3호
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• pp.133-142
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• 2015

지구대기압력이 지각에 변위를 일으키는 현상은 오래 전부터 인식되었으며, 근래의 측지-측량, 특히 우주측지에서 이의 정확한 산정이 필요하게 되었다. 육지에서의 대기 하중에 의한 변형은 주어진 대기압 분포와 하중함수로부터 바로 계산할 수 있으며, 해양에 근접한 지역에서는 근사적인 모델이 사용되고 있다. 지구 대기대순환의 변화와 계절별 지구 양반구에서의 대기압의 분포의 변화들이 각각 지구자전속도 변화와 극운동의 가장 큰 요인으로 알려져 있으며, 바람과 대기압의 변화는 여러 주기영역에서 지구상의 지점들의 좌표의 섭동 및 지구자전상태의 큰 변화 요인이 되고 있다. 본 연구에서는 이와 같은 현상들을 기술하며 관련된 이론과 모델들을 요약하고, 또한 한반도를 지나가는 가상적인 태풍에 의한 효과를 예시하였다. 마지막으로 관련된 몇몇 문제점들과 향후 연구방향을 논의하였다.

• 천문학회보
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• 제28권2호
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• pp.30-30
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• 2003

• 천문학회보
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• 제36권2호
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• pp.93.2-93.2
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• 2011

Japan Aerospace Exploration Agency (JAXA) has measured space environment and its effects on spacecraft and astronaut since 1987. At present, we have operated space environment monitors onboard one GEO spacecraft, one QZO spacecraft, and two LEO spacecrafts. The obtained space environment data has been gathered into the Space Environment and Effects System database (SEES, http://sees.tksc.jaxa.jp/). In this presentation, measurement result of space environment in low earth orbit obtained by the Daichi satellite from 2006 through 2011 is reported as well as recent activities in space environment engineerings in JAXA. The Technical Data Acquisition Equipment (TEDA) on board the Daichi satellite (Advanced Land Observing Satellite: ALOS) had been operated in low earth orbit at 700 km altitude with 98 degree inclination from February 2006 until April 2011. The TEDA consists of the Light Particle Telescope and the Heavy Ion Telescope. The operation period of the Daichi satellite was through the solar-activity minimum period. The space radiation environment around the Daichi satellite had been almost stable. However, large solar flares followed by CMEs sometimes disturbed the space radiation environment in the orbit of the Daichi satellite. In addition, high speed solar wind often flowed and modulated the electron flux in the horn region. On the other hand, a little variation was seen in the SAA region.

• 한국지구과학회지
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• 제31권3호
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• pp.267-275
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• 2010

본 연구의 목적은 9학년 학생의 공간능력 차이에 따른 지구자전 개념을 알아보는 것이다. 광역시 소재 9학년 학생 83명중 천체의 공간운동 개념 평가(김기정, 1997)에서 개념 획득 정도가 비슷하면서 공간능력에 차이가 있는 남학생 2명과 여학생 2명을 각각 표집하여 질적 분석의 대상으로 삼았다. 연구 결과, 공간능력이 높은 학생일수록 개념이 올바르고 개념들을 입체적 공간으로 재구성하여 이해하였다. 공간능력이 낮을수록 개념이 불완전하고 단편적인 개념들을 암기하고 있었다. 성별에 따라서는 공간능력이 높은 남학생은 개념들을 간단 명료하게 표현하였고, 낮은 학생은 자전에 대한 방향을 일주운동과 연관시켜 해석하지 못했다. 반면에 여학생은 공간능력이 높을 때 개념들을 구체적으로 표현하였으며, 낮을수록 개념들을 입체적으로 표현하지 못하였다. 따라서 공간능력이 높은 학생은 문제 상황을 제시하여 스스로 해결할 수 있도록 하고, 낮은 학생은 현상들을 직접 관찰하여 쉽게 이해 할 수 있도록 학습 자료를 개발하여야겠다. 여학생은 공간을 입체적으로 조작해 볼 수 있도록 하고 남학생은 사물을 여러 관점으로 생각해 볼 수 있도록 교수 전략 및 학습 자료 등을 개발 한다면 천문단원의 공간능력이 향상되고, 개념 획득이 잘 될 수 있을 것이라 기대한다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2008년도 한국우주과학회보 제17권2호
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• pp.28.2-28.2
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• 2008

Recently, star sensors have been successfully used as main attitude sensors for attitude control in many satellites. This research presents the star visibility analysis for star trackers and the goal of this analysis is to make sure that the star tracker implementation is suitable to the mission profile and scenario and satisfies the requirement of attitude orbit control system. As a main optical attitude sensor imaging stars, accomodations of a star tracker should be optimized in order to improve the probability of the usage by avoiding the blinding (the unavailability) by the Sun and the Earth. For the analysis, a statistical approach and a time simulation approach are used. The statistical approach is based on the generation of numerous cases, to derive relevant statistics about Earth and Sun proximity probabilites for different lines of sight. The time simulation approach is performed for one orbit to check the statistical result and to refine the statistical result and accomodations of star trackers. In order to perform simulations first of all, an orbit and specific mission profiles of a satellite are set, next the earth proximity probability and the sun proximity probability are calculated by considering the attitude maneuvers and the geometry of the orbit, and then finally the unavailability positions are estimated. As a result, the optimized accomodations of two star trackers are suggested for the low earth orbit satellite.

• 천문학회지
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• 제56권2호
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• pp.263-275
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• 2023

The Sun-Earth Lagrange point L4 is considered as one of the unique places where the solar activity and heliospheric environment can be observed in a continuous and comprehensive manner. The L4 mission affords a clear and wide-angle view of the Sun-Earth line for the study of the Sun-Earth and Sun-Moon connections from he perspective of remote-sensing observations. In-situ measurements of the solar radiation, solar wind, and heliospheric magnetic field are critical components necessary for monitoring and forecasting the radiation environment as it relates to the issue of safe human exploration of the Moon and Mars. A dust detector on the ram side of the spacecraft allows for an unprecedented detection of local dust and its interactions with the heliosphere. The purpose of the present paper is to emphasize the importance of L4 observations as well as to outline a strategy for the planned L4 mission with remote and in-situ payloads onboard a Korean spacecraft. It is expected that the Korean L4 mission can significantly contribute to improving the space weather forecasting capability by enhancing the understanding of heliosphere through comprehensive and coordinated observations of the heliosphere at multi-points with other existing or planned L1 and L5 missions.

• 한국지반공학회:학술대회논문집
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• 한국지반공학회 1999년도 가을 학술발표회 논문집
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• pp.457-464
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• 1999

The active earth pressure on the retaining wall is reduced by 3-Dimensional effects of the ground. Therefore, the test was focused on reducing the earth pressure on the retaining wall by inserting the vertical reinforcement in the backfill ground to develope the 3-Dimensional effects. Model tests in sand were peformed to measure the 3-Dimensional effects of the vertical reinforcement on the active earth pressure and its distribution and results were compared with the theories. The size of the vertical reinforcement, the geometry of the backfill space, and the wall friction of vertical reinforcement were varied. It was observed that the active earth pressure and its distribution on the underground structure were affected by the size of the vertical reforcements and wall friction.

• Geomechanics and Engineering
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• 제16권3호
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• pp.321-329
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• 2018

Classic braced walls use struts and wales to minimize ground movements induced by deep excavation. However, the installation of struts and wales is a time-consuming process and confines the work space. To secure a work space around the retaining structure, an anchoring system works in conjunction with a braced wall. However, anchoring cannot perform well when the shear strength of soil is low. In such a case, innovative retaining systems are required in excavation. This study proposes an innovative earth-retaining wall that uses in situ soil confined in dual sheet piles as a structural component. A numerical study was conducted to evaluate the stability of the proposed structure in cohesionless dry soil and establish a design chart. The displacement and factor of safety of the structural member were monitored and evaluated. According to the results, an increase in the clearance distance increases the depth of safe excavation. For a conservative design to secure the stability of the earth-retaining structure in cohesionless dry soil, the clearance distance should exceed 2 m, and the embedded depth should exceed 40% of the wall height. The results suggest that the proposed method can be used for 14 m of excavation without any internal support structure. The design chart can be used for the preliminary design of an earth-retaining structure using in situ soil with dual steel sheet piles in cohesionless dry soil.