• 한국산학기술학회논문지
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• 제16권3호
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• pp.2301-2307
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• 2015

본 연구에서는 산업용수의 처리 및 운용 과정에서 중요한 문제점으로 지목되고 있는 탄산칼슘에 의한 스케일 형성을 제어하기 위해 고전압 임펄스 (High Voltage Impulse, HVI) 기술의 활용 가능성을 평가하고자 하였다. 전원부, 고전압발생부, 축전기, 스위치 및 임펄스발생기로 구성된 HVI를 제작하여 17kV의 고전압 펄스를 생성시켰다. 반응조에 $Ca^{2+}$을 포함하고 있는 인공 시료를 투입한 후 HVI를 인가하였다. HVI 접촉시간 5분 후에는 $Ca^{2+}$ 초기값의 3.0% 가량만 감소하였으나, 접촉시간 60분 후에는 약 13.7% 가량 감소하였다. HVI 인가로 인해 용액의 온도와 pH는 증가하였고 전기전도도는 탄산칼슘 석출로 인해 감소하는 것을 확인하였다. 칼슘 이온의 감소가 충분하지는 않았지만 전계의 세기 및 접촉시간에 따른 제거율에 간한 구체적인 정보가 얻어진다면, HVI 기술을 적용하여 $Ca^{2+}$ 이온을 탄산칼슘으로 미리 석출시켜 제거하는 연수화 (softening) 공정이나 탈염 기술로 활용할 수 있는 가능성을 확인하였다.

• 천문학회보
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• 제37권2호
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• pp.110.2-110.2
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• 2012

We investigate a cool loop and a dark lane over a limb active region on 2007 March 14 by the Hinode/EUV Imaging Spectrometer (EIS). The cool loop is clearly seen in the EIS spectral lines formed at the transition region temperature (log T = 5.8). The dark lane is characterized by an elongated faint structure in coronal spectral lines (log T = 5.8 - 6.1) and rooted on a bright point. We examine their electron densities, Doppler velocities, and non-thermal velocities as a function of distance from the limb using the spectral lines formed at different temperatures (log T = 5.4 - 6.4). The electron densities of the cool loop and the dark lane are derived from the density sensitive line pairs of Mg VII, Fe XII, and Fe XIV spectra. Under the hydrostatic equilibrium and isothermal assumption, we determine their temperatures from the density scale height. Comparing the scale height temperatures to the peak formation temperatures of the spectral lines, we note that the scale height temperature of the cool loop is consistent with a peak formation temperature of the Mg VII (log T = 5.8) and the scale height temperature of the dark lane is close to a peak formation temperature of the Fe XII and Fe XIII (log T = 6.1 - 6.2). It is interesting to note that the structures of the cool loop and the dark lane are most visible in these temperature lines. While the non-thermal velocity in the cool loop slightly decreases (less than 7 km $s^{-1}$) along the loop, that in the dark lane sharply falls off with height. The variation of non-thermal velocity with height in the cool loop and the dark lane is contrast to that in off-limb polar coronal holes which are considered as source of the fast solar wind. Such a decrease in the non-thermal velocity may be explained by wave damping near the solar surface or turbulence due to magnetic reconnection near the bright point.

• 한국전산유체공학회:학술대회논문집
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• 한국전산유체공학회 2008년도 학술대회
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• pp.97-103
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• 2008

Unsteady three-dimensional flowfields generated by transverse fuel injection into a supersonic mainstream are simulated with a DES turbulence model. Comparisons are made with experimental results in term of the temporal eddy position and eddy formation frequency. The vorticity field around the jet exit is also analyzed to understand the formation mechanism of the jet vortical structures. Results indicate that the DES model correctly predicts the convection characteristics of the large scale eddies. However, it is also observed that the numerical results slightly overpredict the eddy formation frequency. The jet vortical structures are developed from the competing vortices in the recirculation region of upstream boundary.

• 한국전산유체공학회:학술대회논문집
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• 한국전산유체공학회 2008년 추계학술대회논문집
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• pp.97-103
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• 2008

Unsteady three-dimensional flowfields generated by transverse fuel injection into a supersonic mainstream are simulated with a DES turbulence model. Comparisons are made with experimental results in term of the temporal eddy position and eddy formation frequency. The vorticity field around the jet exit is also analyzed to understand the formation mechanism of the jet vortical structures. Results indicate that the DES model correctly predicts the convection characteristics of the large scale eddies. However, it is also observed that the numerical results slightly overpredict the eddy formation frequency. The jet vortical structures are developed from the competing vortices in the recirculation region of upstream boundary.

• 천문학회보
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• 제41권1호
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• pp.39.2-39.2
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• 2016

The central regions of barred-spiral galaxies contain interesting gaseous structures such as dust lanes located at the leading side of the bar and nuclear rings that are sites of intense star formation. Our previous studies showed how gas structures form under the influence of a non-axisymmetric bar potential and temporal/spatial behavior of the star formation in nuclear rings. However, previous works were limited to 2-dimensional infinitesimally-thin, unmagnetized and isothermal disks. To study effects of cooling/heating, vertical motions of gas structures and magnetic field, we use Mesh-Free magneto-hydrodynamic simulation code GIZMO. We find that temporal variations of the star formation rates in the nuclear ring in the three-dimensional model are overall similar those in the previous two-dimensional results, although the former shows more violent small-scale fluctuations near the early primary peak. We will present our recent results about evolution of gaseous structures and star formation rate compare with results of previous studies.

• 대한기계학회논문집B
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• 제23권11호
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• pp.1363-1370
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• 1999

A study of scaling and heat transfer has been carried out for a vertical tube evaporator in which $CaSO_4$ saturated water flows upward. Experimental apparatus including vacuum chambers and heaters has been designed and manufactured to study scaling phenomena for three different pressures(1atm, 0.27atm and 0.16atm). Overall heat transfer coefficients have been measured and shown to decrease with time as scaling proceeds. After the end of experiments, the vertical tube has been cut to measure the thickness of scale at different heights. Below the height where the bulk fluid temperature does not reach saturated temperature, the thickness of scale increases, however, beyond that height occurring saturated condition, the thickness does not vary much or even decreases a little. The measured fouling resistances also support these variations of scale thickness.

• 한국진공학회:학술대회논문집
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• 한국진공학회 1998년도 제14회 학술발표회 논문개요집
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• pp.135-136
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• 1998

By the ion bombardment the original discrete layered structure is damaged and a uniformly mixed layer is formed by the intermixing of the films. Immediately after this dynamic cascade mixing a structure of this mixed layer is likely to be a mixture of randomly distributed atoms. Subsequently the mixed layered structure becomes a non-equilibrium structure such as the metastable pphase because the kinetic energies of the incident ions rappidly dissippate and host atoms within the collision cascade region are quenched from a highly energetic state. The formation of the metastable transition metal alloys using ion-beam-mixing has been extensively studied for many years because of their sppecific ppropperties that differ from those of bulk materials. in ion-beam-mixing the alloy or comppound is formed due to the atomic interaction between different sppecies during ion bombardment. in this study the metastable pphase formed by ion-beam-mixing pprocess is comppared with equilibrium one by arc-melting method by GXRD and XAS. Therfore we studied the fundamental characteristics of charge redistribution uppon alloying and formation of intermetallic comppounds. The multi-layer films were depposited on a wet-oxidized Si(100) substrate by sequential electron beam evapporation at a ppressure of less than 5$\times$10-7 Torr during depposition. These compprise 4 ppairs of Co and ppt layers where thicknesses of each layer were varied in order to change the alloy compposition.

• 한국신재생에너지학회:학술대회논문집
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• 한국신재생에너지학회 2007년도 춘계학술대회
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• pp.511-514
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• 2007

Gas hydrate has a unique property that can store a large volume of gas in water as a solid form. Even though investigations for natural gas storage technology have been carried out for several decades, there are still a lot of unsolved problems due to complex formation process, low formation speed, high energy consumption and so on. So, lots of experiments were conducted to overcome these weaknesses and to develop artificial NGH formation technology applicable to industrial-scale storage and commercial transport. In this study, some series of experiments were performed to analyze both stirred and unstirred system especially about the influences of several gas hydrate formation factors such as agitation speed, system temperature, SDS concentration, etc. As a result, optimum range of SDS concentration and temperature that could enhance the storage capacity and shorten the formation time were found. And it is obviously presented that SDS such a kind of surfactant promotes gas hydrate formation dramatically and the quantity of stored gas are proportional to agitation speed in stirred system.

• 한국주거학회:학술대회논문집
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• 한국주거학회 2005년도 추계학술대회 논문집
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• pp.229-234
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• 2005

The purpose of this study is to analyze a Characteristics of block formation and commercialization of residential books commercial area along urban arteries on Teheran-ro in Seoul. 'Teheran-ro' is selected as a case site to analyze the characteristics of residential blocks commercial area along urban arteries. The study analyzes the characteristics of the street network and block formation in commercial area along arteries and rear residential blocks, and commercialization of residential blocks commercial area along urban arteries according to the characteristics of street network and block formation. The analysis about block formation progress about i ) a street network and block formation, ii ) the scale of blocks, iii) division of lots, iv) lots system. The analysis about commercialization of residential blocks commercial area progress about i) a street network and block formation, ii) a density of building, iii) a use of building

• 대한화학회지
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• 제52권3호
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• pp.303-314
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• 2008

이 연구의 목적은 고등학교 과학 교과서에 제시된 앙금 생성 반응을 이용한 화학반응속도 측정 실 험으로 small-scale chemistry (SSC)를 적용한 실험을 개발하고자 하는 것이다. 연구를 위해서 고등학교 10종 과 학 교과서에 제시된 화학반응속도에 미치는 농도와 온도의 영향에 대한 실험 방법을 반응 생성물 확인 방법 에 따라 분류하고, 과학 교과서에 가장 많이 제시되어 있는 앙금 생성 반응을 이용한 화학반응속도 측정 실험 을 교과서 실험 방법에 따라 수행하였다. 그리고 실험 과정에서 나타나는 문제점들을 분석해서 앙금 생성 반 응을 이용한 화학반응속도 측정 실험에 SSC를 적용한 실험을 개발하였다. 연구 결과에 의하면, 과학 교과서 에 제시된 앙금 생성 반응을 이용한 화학반응속도 측정 실험에는 반응 용액들의 혼합 방법에 대한 번거로움, X자가 보이지 않는 시점의 애매모호함, 실험 결과 수집의 시간 지연, 유독한 이산화황 기체의 발생, 물중탕 장 치 조작의 불편함, 그리고 반응 온도 통제의 어려움 등의 문제점들이 있었다. 또한, 실험 결과들의 재현성이 부 족하였다. 이러한 문제점들은 앙금 생성 반응을 이용한 화학반응속도 측정 실험에 SSC를 적용하여 개발한 실 험으로 해결할 수 있었다. SSC를 적용한 실험에서는 A4 용지 반응판에 실험의 순서를 명시하여 실험 방법을 명확하게 할 수 있었으며, 홈판과 스템 피펫을 사용하여 반응시간을 단축하여 실험 결과들을 연속적으로 얻을 수 있었다. 또한, 유독한 이산화황 기체의 발생량을 1/7 정도로 줄일 수 있었으며, X자가 보이지 않는 시점도 뚜렷하게 관찰할 수 있었다. 그리고 30분 내에 화학반응속도에 미치는 농도와 온도의 영향에 대한 두 실험을 간편하고 재현성 있게 수행할 수 있었다. 또한, 수업시간 중 실험 결과들을 해석하고 토의할 수 있는 시간을 확보할 수 있어, 고등학생들이 화학반응속도에 미치는 농도와 온도의 영향에 대한 과학적인 개념을 형성하는 데 도움을 줄 것으로 기대된다.