• 한국산림과학회지
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• 제99권4호
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• pp.633-637
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• 2010

본 연구는 낙엽송의 4가지 배발생조직(LL-L, LL-K, LL-P 및 LL-N)으로 체세포배 유도에 영향하는 배지종류, 엡시식산(abscisic acid, ABA)의 농도, 삼투압제의 종류 및 농도의 효과를 평가하기 위해 수행되었다. 배지종류 비교에서 1/2LM 배지에 배양한 LL-P 조직라인(134.9개/90 mg조직)에서 가장 높은 자엽단계의 체세포배가 유도되었으나 BLG 배지의 경우 LL-P라인(32.9개)을 제외하고는 체세포배가 전혀 유도되지 않았다. 2가지 ABA농도(60 혹은 100 ${\mu}M$)에 대한 4가지 배발생조직의 체세포배 유도 효과를 비교 한 바 최대 체세포배는 60 ${\mu}M$ ABA농도(142.9개)에서 나타났으나 LL-N 라인을 제외하고는 체세포배 발생에 ABA영향은 그리 크지 않은 것으로 나타났다. 삼투압제 종류 및 농도 비교에서 최고의 체세포배 발생은 LL-K 조직라인을 0.2 M maltose 첨가배지(540.5개)에 배양하였을 때 나타났다. 결론적으로 체세포배 발생 효과는 배지의 종류, 혹은 배지에 첨가된 ABA 및 삼투압제 농도보다는 배발생 조직 라인에 따라 크게 좌우되었다.

• Journal of Power Electronics
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• 제6권1호
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• pp.18-28
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• 2006

The Electric Power Subsystem (EPS) is one of the most critical systems on any satellite because nearly every subsystem requires power. This makes the choice of power systems the most important task facing satellite designers. The main purpose of the Satellite EPS is to provide continuous, regulated and conditioned power to all the satellite subsystems. It has to withstand radiation, thermal cycling and vacuums in hostile space environments, as well as subsystem degradation over time. The EPS power characteristics are determined by both the parameters of the system itself and by the satellite orbit. After satellite separation from the launch vehicle (LV) to its orbit, in almost all situations, the satellite subsystems (attitude determination and control, communication and onboard computer and data handling (OBC&DH)), take their needed power from a storage battery (SB) and solar arrays (SA) besides the consumed power in the EPS management device. At this point (separation point, detumbling mode), the satellite's angular motion is high and the orientation of the solar arrays, with respect to the Sun, will change in a non-uniform way, so the amount of power generated by the solar arrays will be affected. The objective of this research is to select satellite EPS component types, to estimate solar array illumination parameters and to determine the efficiency of solar arrays during both detumbling and normal operation modes.

• Journal of Power Electronics
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• 제6권2호
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• pp.104-113
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• 2006

Satellites have provided the impetus for the orderly development of reliability engineering research and analysis because they tend to have complex systems and hence acute problems. They were instrumental in developing mathematical models for reliability, as well as design techniques to permit quantitative specification, prediction and measurement of reliability. Reliability engineering is based on implementing measures which insure an item will perform its mission successfully. The discipline of reliability engineering consists of two fundamental aspects; $(1^{st})$ paying attention to details, and $(2^{nd})$ handling uncertainties. This paper uses some of the basic concepts, formulas and examples of reliability theory in application. This paper emphasizes the practical reliability analysis of a Low Earth Orbit (LEO) Micro-satellite power subsystem. Approaches for specifying and allocating the reliability of each element of the power system so as to meet the overall power system reliability requirements, as well as to give detailed modeling and predicting of equipment/system reliability are introduced. The results are handled and analyzed to form the final reliability results for the satellite power system. The results show that the Electric Power Subsystem (EPS) reliability meets the requirements with quad microcontrollers (MC), two boards working as main and cold redundant while each board contains two MCs in a hot redundant.

• 천문학회보
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• 제35권1호
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• pp.48.1-48.1
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• 2010

Four of nine exoplanets found by microlensing were detected by the resonant caustic, which represents the merging of the planetary and central caustics at the position when the projected separation of a host star and a bounded planet is s~1. One of the resonant caustic lensing events, OGLE-2005-BLG-169, was a caustic-crossing high-magnification event with A_max ~800 and the source star was much smaller than the caustic, nevertheless the perturbation was not obviously apparent on the light curve of the event. In this paper, we investigate the perturbation pattern of the resonant caustic to understand why the perturbations induced by the caustic do not leave strong traces on the light curves of high-magnification events despite a small source/caustic size ratio. From this study, we find that the regions with small magnification excess around the center of the resonant caustic are rather widely formed, and the event passing the small-excess region produces a high-magnification event with a weak perturbation that is small relative to the amplification caused by the star and thus does not noticeably appear on the light curve of the event. We also find that the positive excess of the inside edge of the resonant caustic and the negative excess inside the caustic become stronger and wider as q increases, and thus the resonant caustic-crossing high-magnification events with the weak perturbation occur in the range of q $\leq$ 10-4. We determine the probability of the occurrence of events with the small excess $|\varepsilon|{\leq}3%$ in high-magnification events induced by a resonant caustic. As a result, we find that for the Earth-mass planets with a separation of ~2.5 AU the resonant caustic high-magnification events with the weak perturbation can occur with a significant frequen.

• 한국재료학회지
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• 제7권2호
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• pp.129-135
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• 1997

용탕단조법에 의해 제조된 Mg-6AI-xZn(x=0,1,2)합금의 기계적 성질에 미치는 시효열처리의 영향을 조사하였다. 주조상태에서의 미세조직은 초정 Mg고용체, 과포화된 상태의 Mg상, 응고과정에서 형성된 $\beta(Mg_{17}AI_{12}$)화합물 등 3개의 상으로 구성되어 있었다. 용체화처리 수 $200^{\circ}C$및 $240^{\circ}C$에서 시효열처리한 결과 Mg-6AI-xZn(x=0,1,2)합금은 $\beta$ 석출물에 의한 피크 경도값이 나타났으며, 석출물의 형태는 $200^{\circ}C$에서는 lamella 형태의 불연속 석출물이, $240^{\circ}C$에서는 미세분산분포된 연속석출물의 형태를 보였다. 용탕단조방법에 의해 제조된Mg-6AI-xZn합금의 기계적 성질은 사형주조법에 비해 인장강도 및 연신율에서 우수한 특성을 보였으며 Zn의 첨가량이 증가함에 따라 Zn의 고용강화 효과에 따라 강도값이 증가되었다.

• 자원환경지질
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• 제40권5호
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• pp.551-561
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• 2007

본 연구는 토양오염의 공간적 확산 및 거동을 이해하기 위한 측정방법을 고찰하고, 토양공극수 채취와 해석에 관한 사례연구이다. 이를 위해서 석유계 탄화수소로 오염된 대표적인 국내 유류오염부지 토양내 PAH류(Polycyclic aromatic hydrocarbons)의 오염 확산과 거동을 정량하기 위한 심도별 토양공극수의 추출장치를 구성하고, 불포화층과 포화층의 토양수를 분석하여 오염물질의 거동을 해석하였다. 토양공극수 추출장치는 공극수 추출용 압력펌프와 토양공극수 추출부로 구성되고, 토양수분장력과 추출압력을 동시에 측정하며 심도별로 토양공극수를 채취하도록 구성하였다. PAH류 오염물질은 추출압력과 시간에 따른 주변 토양공극수의 유입에 의한 희석에 의해서 농도가 낮아졌다. 특히, 추출 심도에 따라 토양의 산화환원전위의 영향에 의해 불포화층의 산화환경에서 포화층의 환원환경보다 자연저감정도가 높았다. 따라서 토양수분장력의 세기에 따라 강한 토양수분장력의 모세관수와 약한 장력의 중력수에 해당하는 토양공극수를 추출함으로써 토양공극수의 평형과 비평형정도를 해석할 수 있다.