• 전력전자학회지
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• 제6권6호
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• pp.63-63
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• 2001

• 한국항공우주학회지
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• 제32권9호
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• pp.80-87
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• 2004

향후 인공위성의 정밀 자세지향 요구가 매우 높아짐에 따라 궤도상의 위성에서 발생하는 고주파 진동인 지터 (Jitter) 의 능동적인 재어가 중요한 문제로 대두되고 있다 . 지터는 탑재체의 성능을 저하시키는 주요 요인이다. 지난 10년간 수동식 및 능동식의 지터 제어 방법이 연구되어 왔다. 본 연구에서는 모텔 장치에 대한 능동식의 지터 분리에 대한 기법을 소개하기로 한다. 모델 장치는 피드백 제어의 원리를 기반으로 3 자유도의 운동을 통해 능동적인 제어가 가능하게 해준다. 이를 위해 시스템의 수학적 모델링을 수행하고 확보된 모델은 기본적인 제어기 설계에 이용된다. 설계된 제어법칙은 시뮬레이션을 통해 그 성능을 검증하도록 한다.

• 우주기술과 응용
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• 제3권2호
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• pp.165-198
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• 2023

2021년 국제 우주감시학회(AMOS)에 발표된 논문에 따르면, 저궤도 우주공간의 우주물체 간 충돌가능성은 작동중인 위성이 아니라 발사체 상단, 폐위성 등 우주 쓰레기에 의한 충돌확률이 높고, 우주교통관제(space traffic management)를 통해 그 충돌 가능성을 줄일 것을 제안하고 있다. 이러한 배경에 최근 우주공간에 위성 등 우주물체의 급속한 증가로 우주 쓰레기(debris) 문제가 국제적인 주요 도전과제로 부각되고 있고, 이에 지난 2022년 9월 뉴욕에서 열린 유엔총회에 한국을 포함한 유엔 회원국들이 수직발사식 위성요격미사일(anti-satellite, ASAT) 실험을 실시하지 않도록 하는 결의안 채택을 통해 전세계 8개국(23년 6월 기준 13개국)이 ASAT 실험을 실시하지 않기로 했다. 또한, 우주 쓰레기를 줄이기 위한 방안이 민간 분야에서 활발히 연구되고 있는데, 이러한 우주 쓰레기 상용서비스는 필요시 군사적으로도 사용이 가능할 것으로 판단된다. 이에 우주 쓰레기 제거기술 현황, 우주위협 평가 및 궤도 상 랑데부 및 근접기동작전 사례에 대해 알아보고, 우주 강국의 우주 쓰레기 제거기술을 활용한 우주무기 개발 개연성에 대해 고찰하겠다. 그리고 미래 우주전장을 대비하기 위한 우주기동전(space maneuver warfare) 이해를 통해 새로운 우주추진체계의 개발 필요성에 대해 제언하고자 한다.

• 통합자연과학논문집
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• 제3권3호
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• pp.143-147
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• 2010

Since it is of great importance to know how a ligand binds to a receptor, there have been a lot of efforts to improve the quality of prediction of docking poses. Earlier efforts were focused on improving search algorithm and scoring function in a docking program resulting in a partial improvement with a lot of variations. Although these are basically very important and essential, more tangible improvements came from the reduction of search space. In a normal docking study, the approximate active site is assumed to be known. After defining active site, scoring functions and search algorithms are used to locate the expected binding pose within this search space. A good search algorithm will sample wisely toward the correct binding pose. By careful study of receptor structure, it was possible to prioritize sub-space in the active site using "receptor-based pharmacophores" or "hot spots". In a sense, these techniques reduce the search space from the beginning. Further improvements were made when the bound ligand structure is available, i.e., the searching could be directed by molecular similarity using ligand information. This could be very helpful to increase the accuracy of binding pose. In addition, if the biological activity data is available, docking program could be improved to the level of being useful in affinity prediction for a series of congeneric ligands. Since the number of co-crystal structures is increasing in protein databank, "Ligand-Guided Docking" to reduce the search space would be more important to improve the accuracy of docking pose prediction and the efficiency of virtual screening. Further improvements in this area would be useful to produce more reliable docking programs.

• 천문학회보
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• 제35권1호
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• pp.34.1-34.1
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• 2010

Solar proton events, whose fluxes are larger than 10 particles cm-2 sec-1 ster-1 for >10 MeV protons, have been observed since 1976. NOAA proton event list from 1997 to 2006 shows that most of the events are related to both flares and CMEs but a few fraction of events (5/93) are only related with CMEs. In this study, we carefully identified the sources of these events. For this, we used LASCO CME catalog and SOHO MDI data. First, we examined the directions of CMEs related with the events and the CMEs are found to eject from the western hemisphere. Second, we searched a major active region in the front solar disk for several days before the proton events occurred by taking into account two facts: (1) The location of the active region is consistent with the position angle of a given CME and (2) there were several flares in the active region or the active region is the largest among several candidates. As a result, we were able to determine active regions which are likely to produce proton events without ambiguity as well as their longitudes at the time of proton events by considering solar rotation rate, $13.2^{\circ}$ per day. From this study, we found that the longitudes of five active regions are all between $90^{\circ}W$ and $120^{\circ}W$. When the flare peak time is assume to be the CME event time, we confirmed that the dependence of their rise times (proton peak time - flare peak time) on longitude are consistent with the previous empirical formula. These results imply that five events should be also associated with flares which were not observed because they occurred from back-side.

• International Journal of Aeronautical and Space Sciences
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• 제7권2호
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• pp.70-85
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• 2006

The supersonic flutter suppression of a cantilevered plate wing is studied with the finite element method and the quasi-steady aerodynamic theory. We suppress wing flutter by using piezoelectric materials and electric devices. Two approaches to flutter suppression using piezoelectric materials are presented; an energy-recycling semi-active approach and a negative capacitance approach. To assess their flutter suppression performances, we simulate flutter dynamics of the plate wing to which piezoelectric patches are attached. The critical dynamic pressure drastically increases with our flutter control using a negative capacitor.

• 전력전자학회:학술대회논문집
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• 전력전자학회 1998년도 Proceedings ICPE 98 1998 International Conference on Power Electronics
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• pp.615-619
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• 1998

Active power filter is a kind of device used for compensating instantaneous reactive and harmonic current in three-phase circuits. An essential technology that determines the behavior of an active power filter is the method of detecting the distorted current. Using three-dimensional space vectors, this paper describes a simple method for detecting the distorted current without any coordinate transformation. The effectiveness of the novel method is verified by the theoretical analysis and simulation.

• 한국방송∙미디어공학회:학술대회논문집
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• 한국방송공학회 2009년도 IWAIT
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• pp.714-718
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• 2009

3D reconstruction of a human face from an image sequence remains an important problem in computer vision. We propose a method, based on a factorization algorithm, that reconstructs a 3D face model from short image sequences exhibiting rotational motion. Factorization algorithms can recover structure and motion simultaneously from one image sequence, but they usually require that all feature points be well tracked. Under rotational motion, however, feature tracking often fails due to occlusion and frame out of features. Additionally, the paucity of images may make feature tracking more difficult or decrease reconstruction accuracy. The proposed 3D reconstruction approach can handle short image sequences exhibiting rotational motion wherein feature points are likely to be missing. We implement the proposal as a reconstruction method; it employs image sequence division and a feature tracking method that uses Active Appearance Models to avoid the failure of feature tracking. Experiments conducted on an image sequence of a human face demonstrate the effectiveness of the proposed method.

• Journal of Astronomy and Space Sciences
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• 제40권4호
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• pp.247-258
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• 2023

Studying the accretion phenomena provides a window into understanding most heavenly bodies, from the birth of stars to active galactic nuclei (AGN). We would adopt the effect of the radiation pressure, which reduces accretion rates (Ṁ), on the accretion phenomena. The Shakura-Sunyaev α-disk model of disk accretion is a good candidate theory of advection dominated accretion flow (ADAF). Reduction in the angular velocity leads to the suppression the disk luminosity and surface temperature, essentially indicating the transition of the standard accretion disk model from convection dominated accretion flow (CDAF) to ADAF.

• 천문학회보
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• 제34권2호
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• pp.27.2-27.2
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• 2009