• 태양에너지
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• 제17권3호
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• pp.35-41
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• 1997

정방형 발열체를 갖는 수직채널내부의 공기유동을 고찰하고자 레이저를 광원으로하는 가시화 실험을 행하였다. 영상처리시스템은 퍼스널컴퓨터의 내부에 장착할 수 있는 범용의 이미지보오드로 구성하였고 광원으로서는 아르곤-이온레이저와 원통형렌즈를 이용하여 시이트라이트를 만들어 이를 대상 유동장에 조사하고 유동장의 영상을 기록하였다. 전유동장의 순시속도벡터는 2차원 PIV시스템에 의하여 구하였고 채택된 동일입자추적기법은 계조치상호상관법이다. 발열체의 발열량은 5W로 균일하며 유입유속은 0.3m/sec으로 일정하게 하였다. 가시화를 통한 PIV계측 결과는 운동에너지와 난류운동에너지의 분포 등에서 유동패턴을 잘 나타내었다.

• 한국태양에너지학회 논문집
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• 제31권3호
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• pp.80-88
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• 2011

Heliostat in the tower type solar thermal power plant is a sun tracking mirror system to reflect the solar energy to the receiver and the optical performance of it affects to the efficiency of whole power plant most significantly. Thus a solid understanding of heliostat's energy concentration characteristics is the most important step in designing of the heliostat field and the whole power plant. The work presented here is the analysis of energy concentration characteristics of heliostat used in 200kW solar thermal power plant, where the receiver located at 43m high in tower has $2{\times}2$m rectangular shape. The heliostat reflective surface is formed by 4 of $1{\times}1$m flat plate mirror facet and the mirror facet is mounted on the spherical frame. The direct normal incident radiation models in vernal equinox, summer solstice, autumnal equinox and winter solstice are first derived from the actually measured data. Then the intercept ratio, heat flux distribution and total energy collected at the receiver for the heliostats located in the various places of the heliostat field are investigated. Finally the effect of mirror facet installation error on the optical performance of the heliostat is analyzed.

• 한국태양에너지학회 논문집
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• 제34권5호
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• pp.33-41
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• 2014

Heliostat field in a tower type solar thermal power plant is the sun tracking mirror system which affects the overall efficiency of solar thermal power plant most significantly while consumes a large amount of energy to operate it. Thus optimal operation of it is very crucial for maximizing the energy collection and, at the same time, for minimizing the operating cost. Heliostat field operational algorithm is the logics to control the heliostat field efficiently so as to optimize the heliostat field optical efficiency and to protect the system from damage as well as to reduce the energy consumption required to operate the field. This work presents the heliostat field operational algorithm developed for the heliostat field of 200kW solar thermal power plant built in Daegu, Korea. We first review the structure of heliostat field control system proposed in the previous work to provide the conceptual framework of how the algorithm developed in this work could be implemented. Then the methodologies to operate the heliostat field properly and efficiently, by defining and explaining the various operation modes, are discussed. A simulation, showing the heat flux distribution collected by the heliostat field at the receiver, is used to show the usefulness of proposed heliostat field operational algorithm.

• 한국태양에너지학회 논문집
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• 제31권4호
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• pp.57-65
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• 2011

This study proposes a Passive Solar Chamber System (PSCS) as a passive method for reduction of building energy consumption. Through numerical analysis, the study quantitatively analyzes system performance and aims to provide foundational data for system design. For this purpose, the study configures different system operation modes seasonally and also computes thermal and ventilation performance of the system in accordance with design factors(solar radiation, air channel height and distance). System and ventilation efficiency increases along with increase in solar radiation and air channel distance; however, as the air channel height increases, the efficiencies showed a tendency to decrease. Upon installation of PSCS, an average of $98.23W/m^2$ of heat flux was introduced in the daytime for the month of January in comparison to walls with no PSCS installed. For the month of August, natural ventilation of $56.68m^3/h$ was shown to be supplied to the room.

• 한국수산과학회지
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• 제29권1호
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• pp.84-91
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• 1996

각종 해${\cdot}$기상 자료와 위성관측에 의한 운량 자료를 이용하여 벌크법에 의해 동지나해에 있어서 대기와 해양간의 열속을 추정하였으며, 그 결과를 요약하면 다음과 같다. 1) 태양복사량은 5월에 $255Wm^{-2}$로 최대, 12월에 $111Wm^{-2}$로 최소이며, 그 분포는 동절기에는 남쪽으로 갈수록 증가하고, 하절기에는 장마전선의 영향으로 북쪽으로 갈수록 증가하는 경향이 있었다. 장파복사량의 경우, 공간적 분포의 차이는 작으나 계절에 따른 차이는 커서 최대인 2월의 값은 (약 $70Wm^{-2}$) 최소인 7월의 2배에 이른다. 2) 현열과 잠열의 공간적 분포양상은 조사해역내의 해류 분포와 비슷하였다. 겨울철에 이 두 요소에 의한 해양의 열손실량은 대단히 커서 $830Wm^{-2}$ 이상이고, 이것은 같은 기간중 순폭사량의 5배에 이른다. 3) 연평균 순열플럭스의 분포는 전역에서 부 값을 보였으며, 최대 열손실 해역은 큐슈 남단으로 1월에 $400Wm^{-2}$ 이상이었다. 4) 조사해역의 태양복사량, 장파복사량, 현열 및 잠열의 연평균치는 각각 187, -52, -30, $-137Wm^{-2}$이고, 결과적으로 연간 약 $32Wm^{-2}(2.48\times10^{13}\;W)$의 에너지를 손실하고 있는 것으로 추정되었다. 5) Fig. 1에 표시되어 있는 A 해역 (황해)은 대기와의 열교환을 통하여 오히려 연간 $10Wm^{-2}(0.4\times10^{13}\;W)$의 에너지를 얻고, B 해역 (동지나해)은 $48Wm^{-2}(2.1\times10^{13}\;W)$,그리고 C 해역 (쿠로시오역)은 $39Wm^{-2}(1.7\times10^{13}\;W)$의 열을 손실하고 있는 것으로 추정되었다.

• 태양에너지
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• 제5권2호
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• pp.11-19
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• 1985

In this paper, the interface stability not to occur mixing and entrainment between the adjacent layers has been studied in the case of the selective withdrawal of a stratum and the injection in stratified fluid formed by the density difference in a small solar pond. There are stability parameter, Richardson number, Rayleigh number and Froude number as the parameters governing stability in order to measure the interface stability on the stratified fluid. The model which could measure the interface stability on the stratified fluid was the small solar pond composed by 1 meters wide, 2 meters high, and 5 meters long. In order to measure the interface stability on the stratified fluid at the inlet port, the middle section and the outlet port, Richardson number, Rayleigh number, and Froude number involved in the parameters governing the stability were calculated by means of the data resulted from the test of the study on hydrodynamic stability between the convective and nonconvective layers in that solar pond. Richardson number written by the ratio of inertia force to buoyancy force can be used in order to measure the stability on the stratified fluid related to the buoyancy force generated from the injection of fluid. Rayleigh number written by the product of Grashof number by Prandtl number can be used in order to measure the stability of the fluid related to the heat flux and diffusivity of viscosity. Froude number written by the ratio of gravity force to inertia force can be used in order to measure the stability of the nonhomogeneous fluid related to the density difference. As the result of calculating the parameters governing stability, the interface stability on the stratified fluid couldn't be identified below the 70cm height from the bottom of the solar pond, but it could be identified above the 70cm height from it at the inlet port, the middle section and the outlet port. When compared with such the three parameters as Richardson number, Rayleigh number, Froude number, the calculated result was in accord with them at inlet port, the middle section and the outlet port. Henceforth, it is learned that even though any of the three parameters is used for the purpose of measuring the interface stability on the stratified fluid, the result will be the same with them. It is concluded that all the use of Richardson number, Rayleigh number, and Froude number, is desirable and infallible to measure the interface stability on the stratified fluid in the case of considering the exist of the fluid flow and the heat flux like the model of the solar pond.

• 한국환경과학회지
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• 제7권5호
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• pp.639-645
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• 1998

A Jump model was evaluated for the calculation of hourly mixing height and mean potential temperature within the height. The Sump model was modified for estimation of downward heat fluxes by mechanical convections and surface heat fluxes. The surface heat fluxes were estimated from routine weather data such as solar radiation and air temperature. Total of 8 upper-air data observed at 0000UTC and 0600UTC in Osan station during April 23 to 26, 1996 were analyzed, and compared to the model results in detail. The calculated mixing heights and potential temperatures within the height were comparable to the observations, but some differences were showed. The calculated mixing heights were generally higher than observations. And, when variations of wind directions were large, the large difference of potential temperature was occurred. From the results, it was important to note that vortical motions and advections of air masses would affect to the growth of the mixing height.

• 한국태양에너지학회 논문집
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• 제22권1호
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• pp.23-30
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• 2002

본 연구는 축방향 내부 핀을 가진 열사이폰의 작동유체의 체적변화에 대한 응축 및 비등열전달 성능에 관한 연구이다. 열사이폰 내부의 작동유체는 증류수를 사용하였다. 열사이폰의 총체적에 대한 작동유체의 양을 변화시키면서 실험데이터를 산출하였다. 열사이폰의 응축부에 대한 열유속과 응축열전달계수를 구하였으며, 실험결과를 이론모델과 비교분석하였다. 실험결과로부터 열사이폰의 열전달 성능은 작동유체의 체적변화에 크게 의존하였다. 축방향내부 핀을 가진 열사이폰의 열전달 성능은 평튜브로 제작한 열 사이폰보다 크게 향상되었다. 이와 같은 열사이폰을 태양열 분야의 열교환기에 응용할 경우, 고성능화와 소형화할 수 있다. 그리고 산업현장에서 실제적으로 적용하기 위해 총열전달계수를 산출하였다.

• 한국신재생에너지학회:학술대회논문집
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• 한국신재생에너지학회 2008년도 춘계학술대회 논문집
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• pp.178-181
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• 2008

Cylindrical stainless-steel/sodium heat pipe for a high-temperature application was manufactured and tested for transient and steady-state operations. The container material was made of stainless-steel 316, and the working fluid was sodium. Stainless-steel 316 mesh screen was inserted as a capillary structure. The working fluid fill charge ratio was approximately 64 $\sim$ 181% based on the pore space of the wick. The outer diameter of the heat pipe was 12.7 mm and the total length was 250 mm. The evaporator part was 150 mm and the condenser 80 mm. The performance test of the heat pipe has been conducted in the furnace with up to 800 W. The variation of the average heat transfer coefficient was investigated as a function of heat flux and vapor temperature. As input thermal load increased, it was showed that difference of temperatures in evaporator and condenser decreased and that operating section and heat transfer characteristics at the heat pipe increased.

• Journal of Advanced Marine Engineering and Technology
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• 제37권4호
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• pp.316-323
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• 2013

평판형 태양열 집열기의 성능을 향상시키기 위하여 다양한 형태의 형상과 크기의 인공 거칠기가 가장 일반적이고 효과적으로 사용된다. 본 연구에서는 다양한 형상의 립을 삽입한 사각 채널에서의 열전달 특성 및 압력강하에 대하여 수치해석을 수행하였다. 사각 채널의 윗 평판에 일정한 열유속을 가하였다. 삽입된 립의 형상은 rib $90^{\circ}$, groove $90^{\circ}$, groove $60^{\circ}$, baffle $90^{\circ}$, baffle $60^{\circ}$, wave $90^{\circ}$, wave $60^{\circ}$ 모델이다. 작동유체는 공기이며 Reynolds 수는 3200~17800의 범위이다. 다양한 형태의 립 형상에 따른 시스템의 성능을 예측하기 위하여 Nusselt 수와 마찰인자를 고찰하였다. 모든 형태의 립에서 속도가 증가할수록 Nusselt 수와 압력강하는 증가하였다. 열전달 향상과 압력강하가 가장 높은 모델은 baffle $90^{\circ}$ 모델이지만, 열전달 특성과 압력강하를 고려하여 나타낸 성능계수에서는 groove $60^{\circ}$ 모델이 가장 크게 나왔다. 따라서 평판형 태양열 집열기에서는 열전달 향상과 압력강하를 항상 동시에 고려한 설계가 필요하다.