• 자원환경지질
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• 제29권6호
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• pp.713-724
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• 1996

현장에서의 주요 운송 메카니즘을 연구하기 위하여 시간별 잔존수 농도분포곡선 자료를 이용하였다. 운송개념을 대표하는 모델로서 2개의 상반된 가설에 근기한 모델, 즉 CDE와 CLT모델을 사용하였으며 파라미터 추정을 위하여 깊이별 평균농도자료에 최적화기법을 적용하였으며 잔존수 농도의 도달시간을 나타내는 확율밀도함수를 이용하여 모멘트해석도 시행되었다. 모멘트 해석결과 잔존수농도의 1차 및 2차 시간 모멘트는 침출수농도의 것들보다 크게 나타났다. 또한 시간 모멘트를 이용하여 오염물질 운송시간의 변이도와 확산 파라미터도 도출되었다. 변이도 및 확산계수와 운송거리간의 상관관계는 침출수농도 및 잔존수농도에 대해서 동일하게 나타났다. 이러한 관계를 이용하여 2가지 모델을 검정하였으나 운송거리에 따른 운송파라미터의 불규칙한 변화로 확정적 결론을 얻을 수 없었다. 따라서 첫 번째 깊이에서 얻은 파라미터를 이용하여 다른 깊이에서의 오염물질 운송 방식을 예측하여 실측자료와 비교하여 각 모델을 검정하였다. 그 결과 CLT 모델이 CDE 모델보다 현장실측자료에 근접하였다. 이는 오염물질이 이동함에 따라 완전한 혼합이 발생하는 것이 아니라 상관흐름 즉, "오염물질이 각 층을 통과할 때 빠른 물질은 빠르게 느린 물질은 지속적으로 느리게 움직인다"는 사실을 뒷받침한다고 볼 수 있다. 특히 첨두농도에 대한 CDE 모델의 과대예측은 오염물질 확산의 과소평가에 기인하는 것으로 나타났다.

• 한국방사선학회논문지
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• 제15권1호
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• pp.55-61
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• 2021

방사선 촬영실은 감염원을 지닌 환자와 간접적인 접촉이 빈번하게 일어나 2차 감염에 노출될 위험성이 높다. 따라서 본 연구는 흉부 X선 촬영을 대상으로 방사선사와 환자가 빈번하게 접촉하는 부위를 4급 암모늄세정제 중 하나인 에니오설프(ANIOS, ANIOSURF Premium NPC)를 이용하여 소독 전, 후의 미생물을 채z취한 후 비교하였다. 2020년 9월 1일부터 9월 7일까지 대구광역시 P병원을 대상으로 X-ray tube handle, Chin rsgion, Chest region, Palm region을 수송배지(TransystemTM, Copan Diagnostics Inc., Murrieta, CA, USA) 내의 멸균면봉을 사용하여 10×10㎠ 크기로 채취한 후 비색법을 통해 소독 전, 후 동정결과를 획득하였다. 그 결과 X-ray tube handle의 경우 Proteus mirabilis, Staphylococcus epidermidis, Bacillus spp., Candida spp이 검출되었고, Chin region의 경우 Proteus mirabilis, Enterococcu faecium, Pseudomonas aeruginosa, NTM이 검출되었고, Chest region의 경우 Proteus mirabilis, Enterococcu faecium, Pseudomonas aeruginosa이 검출되었고, Palm region의 경우 NTM, Candida spp.이 검출되었으며 공통적으로 103 CFU(Colony Forming Unit) 이상이 측정되었다. 소독 후 Chest region, Palm region에서는 미생물이 검출되지 않았고 X-ray tube handle에서만 Bacillus spp.이 검출되었으며 102 CFU 이상이 측정되었다. 소독 전 검출된 미생물은 대부분 기회감염균의 일종으로 소독 후 이러한 미생물의 수가 줄어들거나 제거되는 것을 통해 에니오설프(0.25%)는 에탄올(ethanol, 70~90%)와 이소프로필 알코올(Isopropyl alcohol, 70~90%)과 비교하였을 때 우수한 경제성과 유사한 소독효율을 보였다. 하지만 소독 후 Bacillus spp.가 검출됨에 따라 아포균에 대한 심화된 연구가 필요하다고 생각된다. 본 연구는 방사선 검사실 내 감염관리의 중요성을 재고하였으며 병원 내 2차 감염을 예방하기 위한 유용한 기초자료로 사용될 것으로 사료된다.

• Journal of Advanced Marine Engineering and Technology
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• 제35권7호
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• pp.907-913
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• 2011

Swirling flows are related to the spiral motion in the tangential direction in addition to the axial and radial direction using several swirl generators. These type of flows are used in combustion chambers to improve flame stability, heat exchanger to enhance heat transfer coefficients, agricultural spraying machines and some vertical pipes to move slurries or transport of materials. However, only a few studies three dimensional velocity profiles in a vertical pipe have been reported. In this present paper, 3 dimension particle image velocimetry(PIV) technique was employed to measure the velocity profiles in water along a vertical circular pipe with Reynolds number from 6000 to 13,000. A tangential inlet condition was used as the swirl generator to produce the required flow. The velocities were measured with swirling flow in the water along the test section using the PIV technique.

• 대한기계학회논문집
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• 제6권4호
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• pp.331-340
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• 1982

Numerical analysis is made on the turbulent heat transfer with suspension of solid particles in circular tube with constant heat flux. The mean motion of suspending particles in mixture is treated as the secondary gas flow with virtual density and viscosity. Our modeling of turbulent transport phenomena of suspension flow is based on this assumption and conventional mixing length theory. This paper gives the evidence that the mixing length models can be extended to close the governing equations for two phase turbulent flow with solid boundary at a first order level. Results on Nusselt numbers obtained by analytical treatments are compared with available experimental data and discussed. They suggest that the most important parameters of two phase turbulent heat transfer phenomena are relative particle diameter to pipe diameter, gas-solid loading ratio, and specific heat of suspending material.

• 한국원자력학회:학술대회논문집
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• 한국원자력학회 1995년도 추계학술발표회논문집(1)
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• pp.429-436
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• 1995

This paper describes a methodology for determination of representative CANDU feeder geometry and the pressure drops between inlet/outlet header and fuel channel in the primary loop. A code, MEDOC, was developed based on this methodology and helps perform a calculation of equivalent feeder geometry for a selected channel group on the basis of feeder geometry data (fluid volume, mass flow rate, loss factor) and given property data pressure, quality, density) at inlet/outlet header. The equivalent feeder geometry calculated based on this methodology will be useful fur the transient thermohydraulic analysis of the primary heat transport system for the CANDU heavy water-cooled pressure tube reactor.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2002년도 하계학술대회 논문집
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• pp.248-251
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• 2002

We measured the electron drift velocity, W, in 0.5% $SF_{6}$-Ar mixture over the E/N range from 30 Td to 300 Td and gas pressure range from 0.1 to 8 Torr by the double shutter drift tube with a variable drift distance. This coefficient in the mixture was calculated over the same E/N and gas pressure range by using the two-term approximation of the Boltzmann equation. And the measured and calculated values at different gas number density at each E/N was appreciable dependence in the results on the gas number density,

• 천문학회지
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• 제29권spc1호
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• pp.201-204
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• 1996

Magnetic fields are thought to playa role in a wide variety of important astrophysical processes, from angular momentum transport and jet formation in accretion disks to corona formation in stars. Unfortunately, the dynamics of magnetic fields in astrophysical plasmas are extremely complicated, and the success of current theoretical models and computer simulations seems to be inversely correlated with the amount of observational detail available to us. Here I will discuss some of the more striking conflicts between numerical simulations and observations, and present an explanation for them based on an important dynamical process which is not adequately modeled in current numerical simulations. These processes will lead to the formation of flux tubes in stars and accretion disks, in accordance with observations. I will discuss some of the implications of flux tube formation for stellar and accretion disk dynamos.

• 대한기계학회논문집B
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• 제32권11호
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• pp.870-877
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• 2008

Numerical analysis is applied to model Pt-catalyzed reaction in a micro-scale combustor fueled by butane. The reaction constants of catalytic oxidation are determined from plug flow model with the experimental data. Orders of magnitude between the chemical reaction rate and the mass transfer rate are carefully compared to reveal which mechanism plays a dominant role in the total fuel conversion rate. For various conditions of fuel flow rate and surface temperature, the profiles of Sherwood number are investigated to study the characteristics of the mass transport phenomena in the micro-tube combustor.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2005년도 추계학술대회 논문집 전기물성,응용부문
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• pp.21-23
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• 2005

The electron transport coefficients, the electron drift velocity W, the longitudinal diffusion coefficient $ND_L$ in $C_{3}F_{8}-Ar$ mixture gases were measured by Double shutter drift tube and calculated by multi-term approximation of the Boltzmann equation over the wide E/N range from 0.03 to 100 Td. And an inelastic collision cross sections for $C_{3}F_{8}$ molecular gas were redetermined for quantitative characteristic analysis.

• 대한기계학회:학술대회논문집
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• 대한기계학회 2000년도 춘계학술대회논문집B
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• pp.7-12
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• 2000

The purpose of this study is to develop heat transfer analysis program of heat pipe elements and design a revolving heat pipe exchanger by the performance experiment of hot air production by means of middle-temperature waste heat. Experimental variables are the revolution per minute, normal velocity of inlet air and the temperature of waste heat. The revolving heat exchanger has designed as $2^{\circ}$ in inclination angle of heat pipe bundle and as 20% in working fluid quantity and as water in working fluid. Experimental value of the total heat transfer coefficient was $20w/m^2-^{\circ}C$