• 전기학회논문지P
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• 제62권3호
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• pp.139-144
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• 2013

In Korea, where most of the sites are narrow in space and their earth resistivity is relatively high, the spaces between grounding conductors are likely to be designed narrow in order to lower ground resistance and dangerous voltage below to the permitted safety values. In addition, ground nets are in the shape of square or rectangle depending on the location and size of the facilities and ground contact area, and inner conductors are laid out in grids like the pattern of nets. Nevertheless, with the existing designs, the marginal voltage for safety gets higher as the area is extended further outside, in comparison with that of inner mesh grounding, thus causing much difficulty maintaining them equipotential, and there exist limits in the burial, grounding grid design considering the dangerous voltage of muti-layered model in the constrained sites, was studied.

• 천문학회보
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• 제37권2호
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• pp.88.2-88.2
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• 2012

We present kinematic properties of the narrow-line region in three type-2 QSOs at z~0.35, using 2-D spectra obtained with the VIMOS integral field unit spectrograph at the Very Large Telescope. One of the objects shows a line-of-sight velocity shift of the [OIII] and $H{\beta}$ lines up to 40km/s on a 15 kpc scale, which can be interpreted as either outflow or rotation. The outflow scenario is supported by the presence of blue wings and a radio structure showing lobes in the same direction. Another object features double-peaked emission lines which can be decomposed into two velocity components. Its Hubble Space Telescope image shows two nuclei separated by ~0.2"(~1kpc), implying this may be a binary AGN.

• 천문학회보
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• 제37권2호
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• pp.97.1-97.1
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• 2012

NIR Emission lines from singly-ionized Iron, in particular [Fe II] $1.64{\mu}m$, are good tracer of dense atomic gas in star-forming regions, around evolved stars, and in supernova remnants. We are imaging about 180 square degrees along the Galactic Plane ($6^{\circ}$ < l < $65^{\circ}$;$-1.5^{\circ}$ < b < $+1.5^{\circ}$) with the narrow band filter centered on the [Fe II] $1.64{\mu}m$ line using WFCAM at UKIRT. The observations will complement the UWISH2 survey, which have imaged the same area with the narrow band filter centered on the molecular hydrogen 1-0 S(1) emission line at $2.12{\mu}m$, and probe a dynamically active component of ISM. We present the goals and preliminary results of our survey.

• 천문학회보
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• 제44권2호
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• pp.75.2-75.2
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• 2019

This poster introduces the ongoing "Narrow-band Ca Photometry for Dwarf Spheroidal Galaxies" project and presents the latest results. The project aims to explain the formation and evolution of dwarf spheroidal galaxies by examining the structural properties of stellar populations as a function of metallicity. To overcome the lack of stars with known spectroscopic metallicities for dwarf spheroidal galaxies, we apply the hk index as a photometric metallicity indicator to three galaxies-Draco, Sextans, and Canes Venatici I. For all three galaxies, we found that metal-poor and metal-rich groups of red-giant-branch stars have distinct spatial distributions, in which metal-rich stars are centrally concentrated while metal-poor stars are relatively dispersed. In Sextans, we found an off-centered peak of metal-poor stars which is presumed to be a disrupting star cluster in this galaxy. We will discuss the implications of our results for the dwarf galaxy formation and possible directions on future work of this project.

• 한국가구학회지
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• 제24권3호
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• pp.247-256
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• 2013

A dormitory is the most important compound space to college students who have to live with others. Also, for the students living in the boarding area, the dorm space can be the space for learning, exchanges and cultural. These Housing environment is a public space, so this is based on Universal Design. However, the 1970s-built dormitory space for the current user is narrow and not right for furniture standard. In this study, in order to compensate for these problems, the design directions are based on the previous studies - Park, Young-Soon, 2008, 'A Proposal on Dormitory Furniture Design for University Students.' Based on the previous study, the type of variable design is designed for desks, bookcases, beds, wardrobes, and other cabinets as representative household types. Furthermore, these furnitures are assembled and transformed depend on the dormitory space for single, double and four students. The furniture assembly system and arrangement module are presented in the direction of three kinds of designs. Therefore, three meaning of this study are the development of design to be used each item, the realization of custom furniture for space and presenting variable design module.

• Journal of Astronomy and Space Sciences
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• 제40권4호
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• pp.237-245
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• 2023

Laser communication has been considered as a novel method for earth observation satellites with generation of high data volume. It offers faster data transmission speeds compared to conventional radio frequency (RF) communication due to the short wavelength and narrow beam divergence. However, laser beams are refracted due to atmospheric turbulence between the ground and the satellite. Refracted laser beams, upon reaching the receiver, result in angle-of-arrival (AoA) fluctuation, inducing image dancing and wavefront distortion. These phenomena hinder signal acquisition and lead to signal loss in the course of laser communication. So, precise alignment between the transmitter and receiver is essential to guarantee effective and reliable laser communication, which is achieved by pointing, acquisition, and tracking (PAT) system. In this study, we simulate the effectiveness of tip/tilt compensation for more efficient laser communication in the satellite-ground downlink. By compensating for low-order terms using tip/tilt mirror, we verify the alleviation of AoA fluctuations under both weak and strong atmospheric turbulence conditions. And the performance of tip/tilt correction is analyzed in terms of the AoA fluctuation and collected power on the detector.

• 한국인터넷방송통신학회논문지
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• 제15권2호
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• pp.137-143
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• 2015

과거 30년 동안 메모리 생산의 경제성 이유로 주 메모리 핵심 제품으로 사용된 DRAM의 단점을 극복할 수 있는 대체 기술로 PRAM 기술이 제안되어 왔다. 본 논문에서는 PRAM의 내로우 값을 이용하여 쓰기 동작을 줄임으로써 에너지 소모를 절감할 수 있는 기법을 제안한다. 이를 위해 내로우 값을 이용한 데이터 압축 방법을 기술하고, PRAM의 아키텍쳐 구조를 설정하고, Simplescalar 3.0e 시뮬레이터와 SPEC CPU2000 벤치마크를 사용하여 실험한다. 본 연구의 실험 결과에 의하면 제안된 기법을 사용할 경우 PRAM의 데이터 히트율은 39.4%에서 67.7%로 증가하였으며, 에너지 소모율은 9.2% 감소하였다. 제안된 기법을 사용하기 위해서는 공간 오버헤드가 워드 당 3.13% 발생하며 약간의 추가적인 하드웨어 모듈이 필요하다.

• 천문학회보
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• 제38권2호
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• pp.52.2-52.2
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• 2013

We explore the relative importance of the role of small-scale environment and large-scale environment in triggering nuclear activity of the local galaxies using a volume-limited sample with $M_r$ < -19.5 and 0.02 < z < 0.0685 selected from the Sloan Digital Sky Survey Data Release 7. The active galactic nuclei (AGN) host sample is composed of Type II AGNs identified with flux ratios of narrow emission lines with S/N > 6 and the central velocity dispersion of the sample galaxies is limited to have a narrow range between 130 < ${\sigma}$ < 200($km\;s^{-1}$), corresponding to 7.4 < $log(M_{BH}/M_{\odot})$ < 8.1 in order to fix the mass of the supermassive black hole at the center of its host galaxy. In this study, we find that the AGN fraction ($f_{AGN}$) of late-type galaxies are larger than of early-type galaxies and that for target galaxy with late-type nearest neighbor, $f_{AGN}$ starts to increase as the target galaxy approaches the virial radius of the nearest neighbor (about a few hundred kpc scale). The latter result may support the idea that the hydrodynamic interaction with the nearest neighbor as well as tidal interaction and merger also plays an important role in triggering the nuclear activity of galaxy. We also find that early-type cluster galaxies show decline of AGN activity compared to ones in lower density regions, whereas the direction of dependence of AGN activity for late-type galaxies is opposite.

• Composites Research
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• 제31권5호
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• pp.227-237
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• 2018

본 논문에서는 밀폐/협소의 공간에 적용을 위한 이동형 용접 로봇의 매니퓰레이터의 경량화 및 단열 성능 확보를 위한 설계 적용 연구 내용을 나타내었다. 선박 및 해양플랜트와 같이 구조가 복합하고 협소한 공간에 대한 용접 작업을 위하여 용접사를 작업 대상물 외부에서 용접로봇을 이용한 용접작업을 위하여 다양한 로봇 플랫폼이 개발되고 있다. 일반적인 로봇의 개발 과정은 적용 환경과 요구조건을 고려하여 기계 개발, 전자 장치 개발, 제어 알고리즘 개발 및 통합 검증으로 이루어 진다. 용접로봇의 완성도 높은 개발을 위하여 로봇 플랫폼의 기본 설계에서 환경 조건을 고려한 로봇 매니퓰레이터의 경량 설계를 수행하였다. 또한, 단열성능 및 냉각 성능 확보를 위한 소재 선정과 검증, 해석 및 시험의 과정을 거처 개발된 로봇과 연구 결과를 나타내었다.

• 천문학회보
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• 제46권1호
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• pp.60.1-60.1
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• 2021

The Balloon-borne Investigation of Temperature and Speed of Electrons in the corona (BITSE) is a technology demonstration mission launched in 2019 to observe the solar corona from ~3 Rs to 15 Rs at four wavelengths (393.5, 405.0, 398.7, and 423.4 nm). Preliminary analysis shows that BITSE imaged the solar minimum corona with the equatorial streamers on the east and west limbs. The narrow streamers observed by BITSE are in good agreement with the geometric properties obtained by the Solar and Heliospheric Observatory (SOHO) coronagraphs in the overlapping physical domain. In spite of the small signal-to-noise ratio we were able to obtain the temperature and flow speed of the western steamer. In the heliocentric distance range 4 - 7 Rs on the western streamer, we obtained a temperature of ~ 1.0 ± 0.3 MK and a flow speed of ~ 260 km s^-1 with a large uncertainty interval.