• 디자인학연구
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• 제19권4호
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• pp.91-100
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• 2006

현대 상업공간의 패션 리테일 샵은 변화하는 패션경향에 따라 소비자의 라이프 스타일을 고려한 기능적, 감성적 공간으로 다양화되고 있다. 최근 패션 리테일 샵은 형태로부터의 표면의 변화와 표현특성이 상징화되고 있는데, 이는 공간이 이미지화되고 감성화 되고 있는 표피의 중요성을 재인식하게 되었다. 따라서 본 논문에서는 표피의 특성을 시대적 배경으로 구분하고, 2000년부터 2003년까지의 브랜드 아이덴티티 개념이 도입되고 표피의 표현이 두드러진 패션 리테일 샵의 패션 선두매장 (Flagship store) 4개 브랜드를 중심으로 형태적 측면과 공간적 측면으로 각각 범주화하여 패션 리테일 샵에 나타난 표현경향과 표피의 상관성을 분석 고찰하고자 한다.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2005년도 추계학술대회논문집
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• pp.306-309
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• 2005

This parer describes the tracking control simulation of 6-DOF shaking table with a bell crank structure, which converts the direction of reciprocating movements. For the Joint coordinate-based control which uses lengths of each actuator, the trajectory conversion process inverse kinematics is performed. Applying the Newton-Euler approach, the dynamic equation of the shaking table is derived. To cope with nonlinear problems, time-delay control(TDC) is considered, which has been noted for its exceptional robustness to parameter uncertainties and disturbance, in addition to steady-state accuracy and computational efficiency. If the nominal model is equal to the real system, joint coordinate-based control can be very efficient. However, manufacturing tolerances installation errors and link offsets contaminate the nominal values of the kinematic parameters used in the kinematic model of the shaking table. To compensate differences between the nominal model and the real system. the joint coordinate-based control using acceleration feedback in the Cartesian coordinate space is proposed.

• 한국전자파학회논문지
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• 제21권4호
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• pp.433-442
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• 2010

본 논문에서는 멀티베이스라인 인터페로미터 방향 탐지 시스템에서 진폭 및 위상 부정합 오차를 보정할 수 있는 공분산행렬 기반 자체 교정 알고리즘을 제안한다. 제안된 기법은 비용함수를 정의한 후 제한 조건을 갖는 비선형 최소화 방법으로서, 공간 섹터를 이용하여 부정합 오차를 획기적으로 교정하는 알고리즘이다. 다만 공간 섹터를 선정하기 위하여 초기 추정각을 요구하는 단점이 있으나, 이는 일반적인 비선형 최소화 문제의 공통적인 단점이다. 적절한 공간 섹터 간격을 선정하여 시뮬레이션한 결과, 제안된 방법이 기존 인터페로미터 방식보다 표본바이어스, 표본표준편차, 평균제곱오차면에서 획기적으로 우수한 통계적 성능을 보여주었다. 더구나 섹터 간격이 도래각과 $5^{\circ}$ 이내일 경우에, 30 dB의 진폭 부정합 및 $50^{\circ}$ 이상 큰 값의 위상 부정합이 발생하는 경우에도 획기적인 보정 능력을 보여주었으며, 신호대 잡음비에도 덜 민감한 특징을 나타내었다.

• 천문학회보
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• 제39권1호
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• pp.74.1-74.1
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• 2014

We have investigated a supra-arcade structure associated with an M1.6 flare, which occurred on the south-east limb in the 4th of November 2010. It is ob- served in extreme ultraviolet (EUV) with the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO), microwaves at 17 and 34 GHz with the Nobeyama Radioheliograph (NoRH), and soft X-rays of 8-20 keV with the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI). Interestingly, we found exceptional properties of the supra-arcade thermal plasma from the AIA 131 A and the NoRH: 1) plasma upflows along large coronal loops and 2) enhancing microwave emission. RHESSI detected two soft X-ray sources, a broad one in the middle of supra-arcade structure and a bright one just above the flare-arcade. We estimated the number density and thermal energy for these two source regions during the decay phase of the flare. In the supra-arcade source, we found that there were increases of the thermal energy and the density at the early and the last stages, respectively. On the contrary, the density and thermal energy of the source on the top of the flare-arcade decreases throughout. The observed upflows imply that there is continuous energy supply into the supra- arcade structure from below during the decay phase of the flare. It is hard to be explained by the standard flare model in which the energy release site is located high in corona. Thus, we suggest that the potential candidate as the energy source for the hot supra-arcade structure is the flare-arcade which has exhibited a predominant emission throughout.

• Journal of Astronomy and Space Sciences
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• 제39권2호
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• pp.67-77
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• 2022

The elements that impact the dynamics and collaborations of waves and particles in the magnetosphere of planets have been considered here. Saturn's internal magnetosphere is determined by substantiated instabilities and discovered to be an exceptional zone of wave activity. Interchanged instability is found to be one of the responsible events in view of temperature anisotropy and energization processes of magnetospheric species. The generated active ions alongside electrons that constitute the populations of highly magnetized planets like Saturn's ring electron current are taken into consideration in the current framework. The previous and similar method of characteristics and the perturbed distribution function have been used to derive dispersion relation. In incorporating this investigation, the characteristics of electromagnetic ion cyclotron wave (EMIC) waves are determined by the composition of ions in plasmas through which the waves propagate. The effect of ring distribution illustrates non-monotonous description on growth rate (GR) depending upon plasma parameters picked out. Observations made by Cassini found appropriate for modern study, have been applied to the Kronian magnetosphere. Using Maxwellian ring distribution function of ions and detailed mathematical formulation, an expression for dispersion relation as well as GR and real frequency (RF) are evaluated. Analysis of plasma parameters shows that, proliferating EMIC waves are not developed much when propagation is parallelly aligned with magnetosphere as compared to waves propagating in oblique direction. GR for the oblique case, is influenced by temperature anisotropy as well as by alternating current (AC) frequency, whereas it is much affected only by AC frequency for parallel propagating waves.

• 의료ㆍ복지 건축 : 한국의료복지건축학회 논문집
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• 제22권4호
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• pp.7-17
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• 2016

Purpose: As our population ages and becomes an elderly society the number of elderly care hospitals is rapidly increasing. Because physical functions and spatial perception in the elderly decrease with age, these hospitals require more systematic and intelligent space designs. The design of these spaces are even more complex because they must accommodate medical programs to treat various different diseases and ailments and also because there are many first time patients and irregular short term patients that seek out outpatient treatment services. Also by analyzing the spatial configuration systems and systematic relationships between each of the functional spaces of the outpatient treatment service departments for hospitals specialized in care for the elderly by focusing on the hallway and corridor systems of these hospitals, the according characteristics and trends were examined. Methods: Based on preceding research, the types of hallway and corridor systems of these hospitals were categorized into five types, including gallery corridors, middle corridors, hall-type, mixed type and cyclic type corridors, and into six types according to function including by medical diagnosis, patient registration, examination, administration and convenience and shared common space to derive any interconnecting relationships between the corridor systems. Also by comprehensively examining the types and combined utilization of the corridor types and the integration and the intelligibility of the space syntax, any trends within the corridor system were derived. The elderly care hospitals examined in this research study were twelve hospitals that opened after the year 2000 in Korea with more that 150 sick beds with areas larger than $1000m^2$ and with all outpatient medical service related rooms located entirely on a single floor of the hospital. Results: The following results could be confirmed based on this research study. 1) The spaces where medical diagnosis and examination occurred were adjacent, and the movement lines for first time patients and re-visiting patients were taken into consideration by separating the treatment space. 2) This research study confirmed that the larger the size of the hospital was, there were more detailed categorizations of treatment services and that there was a tendency for treatment areas to be separated and independent from examination areas. 3) There was a tendency for integration and intelligibility to decrease the more complex and diverse the combination of hall types designed into the corridor systems of these hospitals was. cyclic type corridors dramatically decreased the intelligibility of the corridor systems of these hospitals. 4) The priority rank of these spaces were confirmed to be highest in the order of registration, diagnosis, examination, treatment, administration and shared common spaces. However it was confirmed for the local integration that the diagnosis scope had the highest priority rank. Implications: There were exceptional cases confirmed where the number of unit spaces did not have an absolute effect on integration and intelligibility. These results can be interpreted to mean that this can be overcome through efficient architectural planning.

• 한국지리정보학회지
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• 제18권3호
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• pp.89-101
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• 2015

본 연구는 질병역학의 관점에서 2014년 발생한 HPAI(H5N8)의 시간적 분포와 공간적 분포 그리고 시 공간을 동시에 고려한 분포를 지리정보시스템과 연계하여 분석함으로써 2014년 발생한 HPAI의 전파 및 확산 특징을 알아보고자 한다. 분석 결과 2014년 HPAI는 시간적으로는 모두 3 번의 파동을 형성하였으며, 공간적으로는 경기도 충청북도 충청남도가 인접하는 지역, 전라북도의 곰소만 일대, 전라남도의 영암과 나주 등 영산강과 인접한 지역에서 높은 밀도를 보였다. 시 공간적으로도 공간 밀도가 높은 충청북도 음성지역, 전라북도 부안 고창지역, 나주지역에서 군집이 형성되었다. 다만, 충청북도 음성 진천, 충청남도 천안, 경기도 안성 이천 지역과 전라남도 영암 지역에서는 공간적인 밀도는 높음에도 불구하고 시간적인 범위가 넓음으로써 시 공간 군집이 형성되지 못하였다. 이는 이들 지역의 방역에 문제가 있음을 의미한다. 반면에 곰소만과 인접하고 있는 전라북도 부안 고창 장수 지역은 시 공간 군집이 형성됨으로써, 상대적으로 효과적인 방역이 수행되었다고 볼 수 있다.

• 한국정보전자통신기술학회논문지
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• 제9권5호
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• pp.465-471
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• 2016

IPTV의 실시간 멀티미디어 컨텐츠 공유를 위해서는 안정적인 네트워크망과 멀티미디어 사용자 단말이 필요하다. 따라서 FC-AL과 IPTV STB를 이용하여 실시간 고화질 IPTV 컨텐츠 공유 아키텍처를 구성할 수 있지만, 프로토콜의 제한성으로 일정수 이상의 크기를 가진 커뮤니티 네트워크를 구성하기에는 어려움이 있다. 따라서 본 논문에서는 FC Switch를 활용하는 확장가능한 FC-AL 다중루프 기반의 IPTV 컨텐츠 공유 아키텍처를 제안한다. 제안된 아키텍처는 15 msec이하의 우수한 시작지연 시간을 보여주며, 루프수를 증가함에 따라 선형증가하는 공유 IPTV 프로그램수를 보여준다. 또한, 실험을 통하여 다중루프에서의 우수한 시간이동 서비스를 지원함을 보여준다.

• Asian Journal of Atmospheric Environment
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• 제11권2호
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• pp.122-130
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• 2017

The main purpose of the study was to clarify the properties of individual particles collected at each behavior space of a factory worker. The samplings of size-segregated ($PM_{2.1-1.1}$ and $PM_{4.7-3.3}$) indoor particles were conducted at three different behavior spaces of a factory worker who is engaged in an auto parts manufacturing plant (i.e., his home, his work place in factory, and his favorite restaurant). Elemental specification (i.e., relative elemental content and distribution in and/or on individual particles) was performed by a micro-PIXE system. Every element detected from the coarse particulate matters of home was classified into three groups, i.e., a group of high net-counts (Na, Al, and Si), a group of intermediate net-counts (Mg, S, Cl, K, and Ca), and a group of minor trace elements (P, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, and Pb). The results of EF for $PM_{4.7-3.3}$ in home indicated that several heavy metals were generated from the sources within the house itself. An exceptional feature shown in the individual particles in workplace is that Cr, Mn, and Co were clearly detected in both fine and coarse particles. Cluster analysis suggested that the individual coarse particles ($PM_{4.7-3.3}$) collected at the indoor of factory were chemically heterogeneous and they modified with sea-salt, mineral, and artificially derived elements. The principal components in individual coarse particles collected at restaurant were sea-salt and mineral without mixing with harmful trace elements like chromium and manganese. Compared to the indoor fine particles of home and restaurant, many elements, especially, Cl, Na, Cr, Mn, Pb, and Zn showed overwhelmingly high net-counts in those of factory.

• 천문학회보
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• 제42권2호
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• pp.48.3-49
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• 2017

Interplanetary space of the solar system contains a large number of dust particles, referred to as Interplanetary Dust Particles (IDPs) cloud complex. They are observable through meteors and zodiacal lights. The relative contribution of possible sources to the IDPs cloud complex was an controversial topic, however, recent research (Yang & Ishiguro, 2015 and references therein) suggested a dominance of cometary origin. In this study, we numerically investigated the orbital evolution of cometary dust particles, with special concerns on different evolutionary tracks and its consequences according to initial orbits, size and particle shape. The effect of dust particle density and initial size-frequency distribution (SFD) were not decisive in total cloud complex mass and mass supply rate, when these physical quantities are confined by observed zodiacal light brightness and dust particle SFD at 1 au. We noticed that, if we assume the existence of fluffy aggregates discovered in the Earth's stratosphere and the coma of 67P/Churyumov-Gerasimenko, the required mass supply rate decreases significantly. We also found out that close encounters with planets (mostly Jupiter) are the dominating factor of the orbital evolution of dust particles, as the result, the lifetime of cometary dust particles are shorter than Poynting-Robertson lifetime (around 250 thousand years). As another consequence of severe close encounters, only a small fraction of cometary dust particles can be transferred into the orbit < 1 au. This effect is significant for large size particles of ${\beta}$ < 0.01. The exceptional cases are dust particles ejected from 2P/Encke and active asteroids. Because they rarely encounter with Jupiter, most dust particles ejected from those objects are governed by Poynting-Robertson effect and well transferred into the orbits of small semimajor axis. In consideration of the above effects, we directly estimated probability of mutual collisions between dust particles and concluded that mutual collisions in the IDPs cloud complex is mostly ignorable, except for the case of large sized particles from active asteroids.