• 한국항행학회논문지
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• 제12권5호
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• pp.437-443
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• 2008

본 논문에서는 다중사용자 환경의 상향링크 가상적 MIMO-OFDM 시스템 기반 하에서 정보 이론적인 관점에서의 합 전송률을 최대화 할 수 있는 최적의 사용자 수에 대하여 분석하였다. 다중 안테나 기반의 기지국과 단일 안테나용 단말기를 기반으로 하고 있으며 주파수 비선택적 블록 페이딩 및 시변 페이딩 채널 하의 파일럿 기반의 채널 추정 방식을 가정하였다. 이론적 분석을 통하여 낮은 SNR 영역에서 다중화 이득과 파일럿 오버헤드 간의 트레이드오프가 있음을 증명하였고 동일한 파일럿 및 신호 전력이 주어질 때, 주파수 비선택적 블록 채널에서의 시스템 성능을 최대화 하는 최적의 사용자 수는 min ($N_r$,LT/2)으로 결정되는 반면, 페이딩 채널에서는 min($N_r$, ${\lfloor}{\sqrt{LT+1}}-1{\rfloor}$)으로 접근함을 보여 준다.

• 한국수산과학회지
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• 제46권2호
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• pp.186-194
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• 2013

We compiled and analyzed long-term time-series data collected in Korea to evaluate changes in oceanographic conditions and marine ecosystems near Jeju Island ($33^{\circ}00^{\prime}-34^{\circ}00^{\prime}\;N$, $125^{\circ}30^{\prime}-127^{\circ}30^{\prime}\;E$) from 1981 to 2010. Environmental data included depth-specific time series of temperature and salinity that have been measured bimonthly since 1961 in water columns at 175 fixed stations along 22 oceanographic lines in Korean waters by the National Fisheries Research & Development Institute, and time series of estimated volume transport of the Tsushima Warm Current (TWC) and Korea Strait Bottom Cold Water (KSBCW) for the period from 1961 to 2008. We analyzed the species composition in terms of biomass of fish species caught by Korean fishing vessels in the waters near Jeju Island (1981-2010). Data were summarized and related to environmental changes using canonical correspondence analysis (CCA). The CCA detected major shifts in fish community structure between 1982 and 1983 and between 1990 and 1992; the dominant species were a filefish during 1981-1992 and chub mackerel from 1992 to 2007. CCA suggested that water temperature and salinity in the mixed layer and the volume transport of the TWC and the KSBCW were significantly related to the long-term changes in the fish community in the waters off Jeju Island. Fish community shifts seemed to be related to the well-established 1989 regime shift in the North Pacific. Further studies are required to elucidate the mechanisms driving climate change effects on the thermal windows and habitat ranges of commercial species to develop fisheries management plans based on reliable projections of long-term changes in the oceanographic conditions in waters off Jeju Island.

• 한국태양에너지학회 논문집
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• 제29권5호
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• pp.35-44
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• 2009

In this study, boiling heat transfer coefficients(HTCs) and critical heat flux(CHF) are measured on a smooth square flat copper heater in a pool of pure water with and without carbon nano tubes(CNTs) dispersed at $60^{\circ}C$. Tested aqueous nanofluids are prepared using multi-walled CNTs whose volume concentrations are 0.0001, 0.001, 0.01, and 0.05%. For dispersion of CNTs, polyvinyl pyrrolidone(PVP) is used in distilled water. Pool boiling HTCs are taken from $10kW/m^2$ to critical heat flux for all nanofluids. Test results show that the pool boiling HTCs of the nanofluids are lower than those of pure water in entire nucleate boiling regime. On the other hand, critical heat flux is enhanced greatly showing up to 200% increase at volume concentration of 0.001% CNTs as compared to that of pure water. This is related to the change of surface characteristics by the deposition of CNTs. This deposition makes a thin CNT layer on the surface and the active nucleation sites of heat transfer surface are decreased due to this layer. The thin layer acts as the thermal resistance and also decreases the bubble generation rate resulting in a decrease in pool boiling HTCs. The same layer, however, maintains the nucleate boiling even at very high heat fluxes and reduces the formation of large vapor canopy at near CHF resulting in a significant increase in CHF.

• 한국전산유체공학회지
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• 제17권3호
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• pp.68-74
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• 2012

Near-wall effect on wakes behind particles is one of the important factors in precise tracking of particles in turbulent flows. However, most aerodynamic force models for particles did not fully consider the wall effect. In the present study, we focused on changes of hydrodynamic forces acting on a particle depending on wall proximity. To this end, we developed an immersed boundary method with multi-direct forcing incorporated to a fully implicit decoupling procedure for incompressible flows. We validate the present immersed boundary method through two-dimensional simulations of flow over a circular cylinder. Comprehensive parametric studies on the effect of the wall proximity on the drag and lift forces acting on an immersed circular cylinder in a channel flow are performed in order to investigate general flow patterns behind the circular cylinder for a wide range of Reynolds number (0.01 ${\leq}$ Re ${\leq}$ 200). As the cylinder is closer to the wall, the drag coefficient decreases while the lift coefficient increases with a local maximum. Maximum drag and lift coefficients for different wall proximities decrease with increment of Reynolds number. Normalized drag and lift coefficients by their maximum values show universal correlations between the coefficients and wall proximity in a low Reynolds number regime (Re ${\leq}$ 1).

• 천문학회보
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• 제36권2호
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• pp.65-65
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• 2011

Early-type galaxies represent the end point of galaxy evolution and, despite pervasive residual star formation, are generally considered "red and dead", that is composed exclusively of old stars with no star formation. Here, their molecular gas content is constrained and discussed in relation to their evolution, supporting the continuing importance of minor mergers and/or cold gas accretion. First, as part of the Atlas3D survey, the first complete, large, volume-limited survey of CO in normal early-type galaxies is presented. At least of 23% of local early-types possess a substantial amount of molecular gas, the necessary ingredient for star formation, independent of mass and environment but dependent on the specific stellar angular momentum. Second, using CO synthesis imaging, the extent of the molecular gas is constrained and a variety of morphologies is revealed. The kinematics of the molecular gas and stars are often misaligned, implying an external gas origin in over a third of all systems, more than half in the field, while external gas accretion must be shot down in clusters. Third, many objects appear to be in the process of forming regular kpc-size decoupled disks, and a star formation sequence can be sketched by piecing together multi-wavelength information on the molecular gas, current star formation, and young stars. Fourth, early-type galaxies do not seem to systematically obey all our usual prejudices regarding star formation (e.g. Schmidt-Kennicutt law, far infrared-radio continuum correlation), suggesting a greater diversity in star formation processes than observed in disk galaxies and the possibility of "morphological quenching". Lastly, a first step toward constraining the physical properties of the molecular gas is taken, by modeling the line ratios of density- and opacity-sensitive molecules in a few objects. Taken together, these observations argue for the continuing importance of (minor) mergers and cold gas accretion in local early-types, and they provide a much greater understanding of the gas cycle in the galaxies harbouring most of the stellar mass. In the future, better dust masses and dust-to-gas mass ratios from Herschel should allow to place entirely independent constraints on the gas supply, while spatially-resolved high-density molecular gas tracers observed with ALMA will probe the interstellar medium and star formation laws locally in a regime entirely different from that normally probed in spiral galaxies.

• 한국경제지리학회지
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• 제16권4호
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• pp.551-566
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• 2013

이 논문은 지난 10여 년간 우리나라가 채택한 산업클러스터 정책의 평가에 기초하여, 이 정책이 창조경제 실현을 목표로 하는 시대에서도 유효한 정책이 될 수 있을 것인지를 검토하고 향후 정책방향을 제시하기 위한 목적으로 작성되었다. 그동안의 산업클러스터 정책은 산 학 연 네트워킹의 개선과 혁신기반의 강화로 생산성 증가에 기여했지만, 정부 주도의 인위적 클러스터 만들기 정책으로 인해 개방적이고 유연한 클러스터의 발전이 이루어지지 못한 문제가 있었다. 산업클러스터는 창의성에 의한 혁신 유발과 가치창출이라는 창조경제의 선순환에 기여할 것으로 보았다. 그 효과를 극대화하기 위한 향후 정책방향으로서 지리적 집중과 상호 연계라는 클러스터의 본질에 충실할 것, 창조성이 보장되는 클러스터를 만들 것, 국지적-세계적 전략을 결합한 다중 스케일의 산업클러스터를 지향할 것, 지역정책과 산업정책 부문 간의 정합성을 확보할 것 등이 제안된다.

• Wind and Structures
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• 제32권2호
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• pp.127-142
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• 2021

Wind load acting on a standalone structure is different from that acting on a similar structure which is surrounded by other structures in close proximity. The presence of other structures in the surrounding can change the wind flow regime around the principal structure and thus causing variation in wind loads compared to a standalone case. This variation on wind loads termed as interference effect depends on several factors like terrain category, geometry of the structure, orientation, wind incident angle, interfering distances etc., In the present study, a three building configuration is considered and the mean pressure coefficients on each face of principle building are determined in presence of two interfering buildings. Generally, wind loads on interfering buildings are determined from wind tunnel experiments. Computational fluid dynamic studies are being increasingly used to determine the wind loads recently. Whereas, wind tunnel tests are very expensive, the CFD simulation requires high computational cost and time. In this scenario, Artificial Neural Network (ANN) technique and Support Vector Regression (SVR) can be explored as alternative tools to study wind loads on structures. The present study uses these data-driven approaches to predict mean pressure coefficients on each face of principle building. Three typical arrangements of three building configuration viz. L shape, V shape and mirror of L shape arrangement are considered with varying interfering distances and wind incidence angles. Mean pressure coefficients (Cp mean) are predicted for 45 degrees wind incidence angle through ANN and SVR. Further, the critical faces of principal building, critical interfering distances and building arrangement which are more prone to wind loads are identified through this study. Among three types of building arrangements considered, a maximum of 3.9 times reduction in Cp mean values are noticed under Case B (V shape) building arrangement with 2.5B interfering distance. Effect of interfering distance and building arrangement on suction pressure on building faces has also been studied. Accordingly, Case C (mirror of L shape) building arrangement at a wind angle of 45º shows less suction pressure. Through this study, it was also observed that the increase of interfering distance may increase the suction pressure for all the cases of building configurations considered.

• 동남아시아연구
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• 제27권2호
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• pp.119-153
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• 2017

본고는 인도네시아 신질서(Orde Baru; 1966-1998) 체제하에서 진행된 여성다움의 제도화된 이미지를 고찰해보고, 다르마 와니따(Dharma Wanita), 뻬까까(PKK), 교과서 및 인도네시아 국영방송에 표상화되어 있는 제도화된 여성다움을 검토한다. 본고는 인도네시아 신질서 기간 동안, 여성다움을 가내적 공간에 국한시키는 국가 이데올로기인 '이부이즘(ibuism)'의 테두리 안에서 특정한 여성다움의 이미지가 제도화되었음을 밝히고, 이 제도화된 여성다움이 다르마 와니따(Dharma Wanita), 뻬까까(PKK), 교과서 및 인도네시아 국영방송 등을 통해서 전파되었음을 피력한다. 결론을 맺으며 본고는 또한 특히 1990년대 중반이후, 여성다움의 불특정하고 다각적인 현대적 이미지가 대중매체를 매개로 전파되어 왔고, 이러한 현대적 현상으로 인해 신질서체제 이후인 2000년경 인도네시아 여성다움의 이미지는 다소 경합적이었음을 지적한다. 본고는 기존의 연구물들이 심도있게 다루지 않은 여성다움에 대한 국가 이데올로기의 '수단'과 '내용'에 대한 상세한 논의를 진행하며, 이를 통해서 인도네시아 신질서 체제하에서 진행된 여성다움의 제도화된 이미지를 이해하는데 소중한 자료가 되어줄 것으로 기대된다.

• 천문학회지
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• 제56권1호
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• pp.59-73
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• 2023

The second generation of stars in the globular clusters (GCs) of the Milky Way (MW) exhibit unusually high N, Na, or Al, compared to typical Galactic halo stars at similar metallicities. The halo field stars enhanced with such elements are believed to have originated in disrupted GCs or escaped from existing GCs. We identify such stars in the metallicity range -3.0 < [Fe/H] < 0.0 from a sample of ~36,800 giant stars observed in the Sloan Digital Sky Survey and Large Sky Area Multi-Object Fiber Spectroscopic Telescope survey, and present their dynamical properties. The N-rich population (NRP) and N-normal population (NNP) among our giant sample do not exhibit similarities in either in their metallicity distribution function (MDF) or dynamical properties. We find that, even though the MDF of the NRP looks similar to that of the MW's GCs in the range of [Fe/H] < -1.0, our analysis of the dynamical properties does not indicate similarities between them in the same metallicity range, implying that the escaped members from existing GCs may account for a small fraction of our N-rich stars, or the orbits of the present GCs have been altered by the dynamical friction of the MW. We also find a significant increase in the fraction of N-rich stars in the halo field in the very metal-poor (VMP; [Fe/H] < -2.0) regime, comprising up to ~20% of the fraction of the N-rich stars below [Fe/H] = -2.5, hinting that partially or fully destroyed VMP GCs may have in some degree contributed to the Galactic halo. A more detailed dynamical analysis of the NRP reveals that our sample of N-rich stars do not share a single common origin. Although a substantial fraction of the N-rich stars seem to originate from the GCs formed in situ, more than 60% of them are not associated with those of typical Galactic populations, but probably have extragalactic origins associated with Gaia Sausage/Enceladus, Sequoia, and Sagittarius dwarf galaxies, as well as with presently unrecognized progenitors.

• 한국가스학회지
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• 제20권4호
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• pp.65-77
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• 2016

Fischer-Tropsch 반응기 내 복잡한 반응과 흐름을 상세히 모델링하는 것은 CFD 분야에 있어 도전적 과제이다. Fischer-Tropsch 반응은 여러 가지 탄소수를 가진 탄화수소들을 만들어내는데, 탄화수소에는 무수히 많은 이성질체가 존재하는 이유로 모든 화학종에 대해서 각각의 반응속도식을 도출해 적용하는 것은 어렵다. 이의 극복을 위해 기존 연구들에서 사용된 반응속도식 모델링 방법론들을 분석한 뒤, 화학종별 상세한 반응속도식 적용을 위해 non-Anderson-Schulz-Flory 방법론을 선정하여 상세 모델링을 진행하였다. 또한 반응 특성상 다상 흐름 형태를 띠는데, 다상 흐름 모델링의 경우 상간의 간섭이나 분산상의 분포 및 유동 형태 등에 따라 적합한 모델링 방법론이 다르다. 그러나 기존 연구들에서는 타당성에 대한 논의나 근거 제시 없이 각양각색의 내부 흐름 모델링 방법론이 사용되고 있다. 실험을 통해 내부 흐름 형태를 관찰한 뒤 유동 형태에 따른 모델링을 진행하는 것이 최선이나, 자원 여건상 어려움이 있어, 본 연구에서는 전통적인 유체역학 이론에 근거해 내부 흐름 형태를 먼저 추론하고 Mixture 모델 방법론을 선정하여 체계적인 CFD 모델링을 진행함으로써, 사용된 방법론에 대한 근거를 마련하고자 하였다. 10가지 실험조건에서 진행한 실험 결과와 본 연구의 시뮬레이션 결과를 비교하였으며, 이를 통해 본 연구가 제안하는 체계적 모델링 방법론의 타당성을 입증하였다.