• 한국습지학회지
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• 제16권1호
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• pp.41-50
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• 2014

본 연구는 오염된 유수지 수질개선을 위한 고속 선회류 침전 장치(HRSC)의 이용 가능성을 평가하는데 목적을 두었다. 이를 위해 실험실 규모 및 파일럿 규모의 실험을 수행하였다. 또 전산유체역학(CFD) 프로그램 중 하나인 Fluent를 이용하여 유입속도 및 유입직경, 몸체길이($L_B$) 및 하부콘길이(Lc), 역경사콘 기울기 및 간격, 하부유출홀 설치 여부가 HRSC 장치내부의 유체흐름 패턴에 미치는 영향을 분석하였다. 유동 분석 결과와 실험실 규모의 실험 결과를 토대로 파일럿 장치를 제작하고 유수지 시료를 대상으로 현장 적용 가능성을 평가하였다. 장치 내부의 유동 조사 결과, 유입 유량과 직경 보다 유입 속도가 선회류 형성에 더 큰 영향을 나타내었으며, $L_B$ $1.2{\sim}1.6D_B$(몸체 직경), Lc $0.35{\sim}0.5L_B$ 범위에서는 큰 차이가 없었으나 $L_B/D_B$ 2.0, $Lc/L_B$ 0.75로 비가 큰 경우 선회류는 감소되었다. 역경사콘 기울기가 커질수록 역경사콘 내부 속도는 낮아지고 매우 균일하게 분포되었으며, 역경사콘 간격은 난류를 방지하기 위해 10cm가 20cm 보다 좋은 조건이었다. 하부 유출홀은 설치하지 않는 것이 배출수의 고른 유량 분배와 편류 방지를 위해 보다 좋은 것으로 판단되었다. 파일럿 규모의 현장 실험 결과 수중의 입자성 물질이 효과적으로 제거되어 본 장치가 유수지와 같은 대용량 수체의 수질개선을 위한 한 가지 방안으로 활용될 수 있을 것으로 기대되었다.

• 천문학회보
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• 제41권2호
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• pp.54.1-54.1
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• 2016

Stellar wind and radiation pressure from massive stars can trigger the formation of new generation of stars. The sequential age distribution of stars, the morphology of cometary globules, and bright-rimmed clouds have been accepted as evidence of triggered star formation. However, these characteristics do not necessarily suggest that new generation of stars are formed by the feedback of massive stars. In order to search for any physical connection between star forming events, we have initiated a study of gas and stellar kinematics in NGC 1893, where two prominent cometary nebulae are facing toward O-type stars. The spectra of gas and stars in optical and near-infrared (NIR) wavelength are obtained with Hectochelle on the 6.5m MMT and Immersion GRating INfrared Spectrograph on the 2.7m Harlan J. Smith Telescope at McDonald observatory. In this study, the radial velocity field of gas across the cluster is investigated using $H{\alpha}$ and [N II] ${\lambda}$ 6584 emission lines, and that of the cometary nebula Sim 130 is also probed using 1-0 S(1) transition line of $H_2$. We report a distinctive velocity field of the cometary nebulae and many ro-vibrational transitions of $H_2$ even at high energy levels in the NIR spectra. These properties indicate the interaction between the cometary nebulae and O-type stars, and this fact can be a clue to triggered star formation in NGC 1893.

• 한국해양학회지
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• 제16권1호
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• pp.31-37
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• 1981

우리나라 남동부의 광범한 유역을 따라 흐르는 낙동강은 국내에서 가장 긴 하천의 하나로서 영남지역을 굽이쳐 흐르다가 부산 앞바다를 통하여 대한해협에 유입한다. 이 강의 하구는 유역주민의 생활 및 산업용수원으로서 중요할 뿐만 아니라 최근에는 산업입지 및 자연환경 보전문제로서 논의의 대상이 되고 있다. 낙동강은 하구로부터 약 40km상류까지 상향류를 보이며, 약 60km상류까지 조석의 영향을 받는 감조하천으로서 (유 장 1979), 하구역에는 해수, 하천의 담수 및 양자의 혼합수가 조석의 간만등 여러 가지 요인에 따라 유출되기도 하고 유입되기도 한다.

• 한국화재소방학회논문지
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• 제25권3호
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• pp.85-90
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• 2011

본 연구는 국내 고층건물 특별피난계단의 부속실에 설치되는 급기가압 제연시스템에서 화재 발생 시 피난을 위하여 출입문이 개방되었을 경우 형성되는 방연풍속의 특성을 FDS를 이용하여 해석하였고, 해석 결과를 분산분석으로 기류의 특성에 따른 측정 방안을 분석하고자 한다. 부속실과 같은 구획공간의 설계 조건에서 급기댐퍼에서 토출되는 보충량은 심한 와류를 형성하고 형성된 와류의 범위 안에 출입문이 존재할 경우 비정상적인 기체의 유동이 출입문지점에 발생한다는 것을 선행연구를 통하여 확인할 수 있었다. 국가화재안전기준 NFSC 501A에서 방연풍속을 측정할 때에는 출입문의 개방에 따른 개구부를 대칭적으로 균등 분할하는 10 이상의 지점에서 측정하는 풍속의 평균치로 할 것으로 정하고 있으나 이러한 조건에서는 출입구 상부 지점에 기류의 유입 현상을 파악하기 어렵고 풍속의 편차가 심하기 때문에 측정점을 공기조화설비의 시험조정 평가 기술기준에서 제시하는 64점 이상으로 세분화하여 측정하여야 할 것이다.

• 천문학회보
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• 제38권1호
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• pp.51.1-51.1
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• 2013

We present molecular line observations of a small group of Young Stellar Objects (YSOs), L1251C. Observations by Spitzer Space Telescope legacy program "From Molecular Cores to Planet Forming Disks"(c2d; Evans et al. 2003) revealed that there are three YSOs within ~15" in L1251C: IRS1 (Class I), IRS2 (Class II), and IRS3 (Class II). In order to understand the molecular environment around these YSOs, we carried out the KVN single-dish observations in $HCO^+$ J=1-0, $H^{13}CO^+$ J=1-0, $N_2H^+$ J=1-0 and HCN J=1-0. CO J=1-0 was also mapped in L1251C with the TRAO 14m telescope. Integrated intensity maps of high density tracers such as $H^{13}CO^+$ J=1-0, $N_2H^+$ J=1-0 and HCN J=1-0 show similar emission distributions, whose peaks are off from the positions of YSOs. However, $HCO^+$ J=1-0, which is believed to trace both infall and outflow, presents its emission distribution different from those of other molecular transitions. The line profile of $HCO^+$ J=1-0 is superimposed by two velocity (narrow and broad) components. The $HCO^+$ outflow map reveals multiple structures while the CO outflow map elongates mainly along the EW direction. With the KVN single dish, the 22 GHz $H_2O$ maser emission has been also monitored toward L1251C to find variations of the systemic velocity and intensity with time.

• Smart Structures and Systems
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• 제32권5호
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• pp.281-295
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• 2023

The purpose of this study is to demonstrate and verify the application of phase-control absolute-acceleration-feedback active tuned mass dampers (PCA-ATMD) to multiple-degree-of-freedom (MDOF) building structures. In addition, servo speed control technique has been developed as a replacement for force control in order to mitigate the negative effects caused by friction and inertia. The essence of the proposed PCA-ATMD is to achieve a 90° phase lag for a structure by implementing the desired control force so that the PCA-ATMD can receive the maximum power flow with which to effectively mitigate the structural vibration. An MDOF building structure with a PCA-ATMD and a real-time filter forming a complete system is modeled using a state-space representation and is presented in detail. The feedback measurement for the phase control algorithm of the MDOF structure is compact, with only the absolute acceleration of one structural floor and ATMD's velocity relative to the structure required. A discrete-time direct output-feedback optimization method is introduced to the PCA-ATMD to ensure that the control system is optimized and stable. Numerical simulation and shaking table experiments are conducted on a three-story steel shear building structure to verify the performance of the PCA-ATMD. The results indicate that the absolute acceleration of the structure is well suppressed whether considering peak or root-mean-square responses. The experiment also demonstrates that the control of the PCA-ATMD can be decentralized, so that it is convenient to apply and maintain to real high-rise building structures.

• 한국재료학회지
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• 제12권2호
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• pp.129-134
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• 2002

The optimum condition for fabricating cordierite disc type filter element was deduced. Cordierite monolith was used as starting material for filter element because it has many advantages such as high thermal shock resistance and good catalytic activity compared with $TiO_2$and SiC. The contents of organic additives and foaming agent were optimized to control the porosity and mechanical strength of cordierite filter. Among the required properties to be adopted as filter elements, the pressure drop and NOx removal efficiency were investigated depending on processing variables. It was found that pressure drop depends on particle size distribution of cordierite monolith and organic additives added as forming agent. The pressure drop at 5cm/sec of face velocity was in the range of 15~655mm$H_2O$ at room temperature. The NOx removal efficiency of catalytic filter with $V_2O_5$ as catalyst was over 85% at $450^{\circ}C$.

• 천문학회보
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• 제37권1호
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• pp.48.2-48.2
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• 2012

We present preliminary results of a statistical study on the nuclear activity of compact group galaxies. What triggers Active Galactic Nuclei (AGN) is still a puzzling problem. One of the suggested AGN triggering mechanisms is galaxy-galaxy interaction. Many simulations have shown that gas can be supplied to the center of galaxies during galaxy encounters. In this regard, compact groups of galaxies are an ideal laboratory for studying the connection between galaxy interaction and nuclear activity because of their high densities and low velocity dispersions. We study the environmental dependence of the activity in galactic nuclei using 59 compact groups in the SDSS DR6. Using the emission line data, we classify galaxies in the compact groups. We find that 19% of the compact group galaxies are pure star-forming nuclei, 10% as transition objects, and only 7% of the galaxies in compact groups show the nuclear activity. The AGN fraction of compact group is higher than galaxy clusters, but lower than field environment. Implications of this result will be discussed.

• 한국정밀공학회지
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• 제32권6호
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• pp.577-585
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• 2015

We fabricated multi-scale such as macro-, micro-, and multi-scale wrinkles by using repetitive volume dividing (RVD) method and thermal curing process. Also wrinkle surface was modified with coating of a self-assembled monolayer (SAM). We measured the contact angle of each wrinkled surface, and observed the behavior of droplets on sloping surface. Through experimental study, we found out that the contact angle was much higher in case of multi-scale and SAM coated wrinkles. And micro-scale wrinkle showed a high contact angle comparing with that of macro-scale wrinkle. Dynamic behaviors of a water droplet like sliding velocity on diverse wrinkled surfaces were dependent on their static contact angles. These results showed that hydro-dynamic characteristics were changed depending on the wrinkle structure and the material forming the wrinkle. These dynamic characteristics can be utilized in bio-chip, microfluidics, and many others in order to control easily chemical reactivity.

• 천문학회지
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• 제27권2호
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• pp.147-158
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• 1994

We have obtained high angular resolution maps toward a molecular cloud associated with an HII region S287 and studied mainly kinematics of the cloud. The mapped region is 1.5 square degrees of the cloud in the transitions of $^{12}CO\;and\;^{13}CO\;J=1-0$. We have obtained a large range of mass, $1.3\times10^4M_\bigodot$, to $7.2{\times}10^4M_{\bigodot}$ using three different techniques. The S287 molecular cloud shows a very disturbed feature: velocity field of the cloud is very complicated, and shows several arcs. It is likely that the southern part of cloud is being disrupted by the residing HII region S287 as well as external perturbing sources. In addition to an HII region, five bipolar outflows are also disturbing the molecular gas significantly. The large virial mass and the very disturbed morphology may reflect the fact that the cloud is not gravitationally bound system, as in the case of nearby giant molecular cloud (GMC) G216-2.5. The several arc structure and the filamentary features are possibly driven by external strong stellar winds, and these external perturbing sources may be driving the second generation of star-forming activities on the edges of the S287 molecular cloud.