• 설비공학논문집
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• 제7권1호
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• pp.42-51
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• 1995

In order to establish a theoretical basis for the analyses of transient behaviors in stratified thermal storage tanks, analytical approaches to an improved one-dimensional model are made. In the present model the storage tank is treated as a finite region with an adiabatic tank exit, whereas it has been considered as a simple semi-infinite region previously. Application of the Laplace transformation and the Inversion theorem to the governing equations makes it possible to obtain an exact infinite-series solution, which is convergent only at sufficiently large time. Accordingly a complementary solution which is available for short times, i.e., the time range of this study is sought by an approximate method. The approximate solution which is rigorously validated through the examination of neglected terms in the solution procedure agrees quite well with the exact one. Moreover, it is simpler to use and more convenient to interpret the physical meaning of the solution. Comparison of the present solution with the previous ones shows relatively large difference near the tank bottom, which results from the more realistic boundary condition adopted in the present model. Some representative results by the approximate solution including effects of the Peclet number on temperature distrbutions are illustrated to show the utility of this study. In consequence, it is expected that the present results based on the improved model replace the foregoing ones as a new theoretical reference for studies of thermal stratification fields.

• Computers and Concrete
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• 제19권6호
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• pp.659-666
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• 2017

Based on the Arrhenius equations, several hydration exothermic models that precisely calculate the influence of concrete's self-temperature duration on its hydration exothermic rate have been presented. However, the models' convergence is difficult to achieve when applied to engineering projects, especially when the activation energy of the Arrhenius equation is precisely considered. Thus, the models' convergence performance should be improved. To solve this problem and apply the model to engineering projects, the relationship between fast iteration and proper expression forms of the adiabatic temperature rise, the coupling relationship between the pipe-cooling and hydration exothermic models, and the influence of concrete's self-temperature duration on its mechanical properties were studied. Based on these results, the rapid convergence of the hydration exothermic model and its coupling with pipe-cooling models were achieved. The calculation results for a particular engineering project show that the improved concrete hydration exothermic model and the corresponding mechanical model can be suitably applied to engineering projects.

• 한국전산유체공학회지
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• 제2권2호
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• pp.59-72
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• 1997

A numerical model is constructed to simulate the interactions of oblique shock wave / turbulent boundary layer on a strongly heated wall. The heated wall temperature is two times higher than the adiabatic wall temperature and the shock wave is strong enough to induce boundary layer separation. The numerical diffusion in the finite volume method is reduced by the use of a higher order convection scheme(UMIST scheme) which is a TVD version of QUICK scheme. The turbulence model is Chen-Kim two time scale model. The comparison of the wall pressure distribution with the experimental data ensures the validity of this numerical model. The effect of strong wall heating enlarges the separation region upstream and downstream. In order to eliminate the separation, wall suction is applied at the shock foot position. The bleeding slot width is about same as the upstream boundary layer thickness and suction mass flow is 10% of the flow rate in the upstream boundary layer. The final configuration of the shock reflection pattern and the wall pressure distribution approach to the non-viscous value when wall suction is applied.

• 콘크리트학회논문집
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• 제22권3호
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• pp.389-397
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• 2010

콘크리트는 역학적 성능, 내구성능, 경제성이 우수한 재료이지만 장경간 교량에 적용하기는 쉽지 않은데, 이는 콘크리트의 중량 대비 강도가 낮기 때문이다. 초고성능 콘크리트는 높은 압축강도를 가지며 굵은 골재를 사용하지 않으므로 단면의 크기를 줄일 수 있어, 장경간 교량 바닥판으로 활용이 기대된다. 그러나 초고성능 콘크리트는 재료 특성상 단위결합재량이 많으므로 바닥판 양생과정에서 수화열에 의한 균열이 발생할 수 있다. 이 연구에서는 UHPC 바닥판의 초기재령 균열 위험성을 평가하기 위한 기초 작업을 수행하였다. 먼저 단열온도 상승시험 결과를 바탕으로 2변수 모델과 S자형 함수의 중첩으로 단열온도 상승곡선을 모델링하고, 등가재령의 개념을 도입하여 UHPC의 아레니우스 상수를 결정하였다. 이상의 결과를 실물크기 시험체에 대한 수화발열 측정시험으로 검증하였다. 다음으로 초음파 속도 측정 결과와 하중 재하에 의하여 탄성계수, 인장강도, 압축강도와 같은 UHPC의 역학적 특성을 구하였다.

• 콘크리트학회논문집
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• 제14권1호
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• pp.118-125
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• 2002

콘크리트는 수화과정을 통하여 재료가 성숙되고, 경화된다. 수화의 진행은 엄밀한 의미에서 재령에 의하지 않고 수화도에 의해 제어되므로, 경화가 진행되는 콘크리트의 모든 재료특성과 미세구조 형성과정은 수화도에 의해 정식화되는 것이 바람직하다. 기존 연구는 주로 양생온도가 수화발열속도에 미치는 영향을 고려한 반응함수 개념을 주로 사용하였고, 또한 내부 수분상태의 영향을 습도함수의 형태로 고려한 연구결과는 실제 수화기구를 반영하지 못하고 단지 각 연구자의 실험조건과 배합조건에만 부합하는 결과를 보인다. 따라서 본 연구는 기존 제안식의 단점을 보완하기 위하여 수화기구와 미세구조 형성 과정에 기초하여 반응속도함수를 모델링하였다. 수화반응속도는 온도 및 수분상태에 따라 변화하므로, 본 연구에서는 수화발열 속도에 영향을 미치는 인자로, 시멘트 종류, 물-시멘트비 등의 배합특성과 양생온도 빛 세공조직의 내부수분상태를 고려하였다. 똔 연구에서 제시한 콘크리트의 수화도 예측모델은 기존의 온도영향만을 주로 고려하는 반응속도함수를 콘크리트내부의 수분분포 상태를 고려하여 모델을 개선하였으며, 이는 실제 측정한 수화도에 매우 근접하여 그 유용성을 검증하였다. 또한 수화도의 정의와 제시한 모델을 이용하여 콘크리트 요소내의 온도, 습도 덴 수화도를 수치적으로 결정하여 단열온도상승곡선을 정확히 모사 할 수 있었다. 제안된 모델은 수화가 진행되는 콘크리트의 여러 역학적 특성 및 미세구조 형성과정을 적절히 표현하고, 수화과정이 온도 및 습도상태를 결정하는 초기재령 콘크리트의 단면 내 온 습도상태를 추정하여 궁극적으로 초기재령 콘크리트의 균열 위험성을 평가하는데 유용하게 이용될 수 있을 것으로 사료된다.

• 설비공학논문집
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• 제19권1호
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• pp.19-27
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• 2007

Analytical investigation on the performance of a two stage twin rotary compressor for $CO_2$ heat pump water heater system has been carried out. A computer simulation program was made based on analytical models for gas compression in control volumes, leakages among neighboring volumes, and dynamics of moving elements of the compressor. Calculated cooling capacity, compressor input, and COP were well compared to those of experiments over the compressor speeds tested. For the operating condition of suction pressure of 3 MPa, and discharge pressure of 9 MPa, and compressor inlet temperature of $35^{\circ}C$, the compressor efficiency was calculated to be 80.2%: volumetric, adiabatic, and mechanical efficiencies were 88.3%, 93.2%, and 92.7%, respectively. For the present compressor model, volumetric and adiabatic efficiencies of the second stage cylinder were lower by about $6{\sim}7%$ than those of the first stage mainly due to the smaller discharge port at the second stage. Parametric study on the discharge port size showed that the compressor performance could be improved by 3.5% just by increasing the discharge port diameter by 20%.

• 한국건설순환자원학회논문집
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• 제9권4호
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• pp.650-657
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• 2021

광물질 혼화재를 자극하는 알칼리 활성화제는 고가의 소재이지만, 고 알칼리 성분의 산업부산물 대체하기 위해서는 제품성과 경제성을 모두 만족하여야 한다. 본 연구에서는 50MPa 이상의 고강도 콘크리트에 GGBFS의 알칼리 활성 반응을 위한 목적으로 LCD 제조 공정에서 발생하는 알칼리 산업부산물(LW)을 사용하였다. LW을 혼입한 콘크리트는 작업성이 다소 저하되었으나, 압축강도가 증진되는 특징이 있었다. ACI 209.2R-08 압축강도 모델식을 이용하여 분석하여 LW 혼입에 따른 강도계수의 변화를 비교하였다. 콘크리트의 내구성능 시험에서도 염화물 침투 저항성 및 탄산화 저항성에서 우수한 성능을 나타내었다. 단열온도 상승시험 결과에서는 LW를 혼입하면 초기 수화열이 빨라지는 효과가 있으나, 최종 단열온도상승량은 LW의 혼입 유, 무에 큰 영향을 받지 않았다.

• 대기
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• 제31권2호
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• pp.199-214
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• 2021

A record-breaking high surface air temperature of 41.0℃ was observed on 1 August 2018 at Hongcheon, South Korea. In this study, to quantitatively determine the formation mechanism of this extremely high surface air temperature, particularly considering the contributions of the foehn and the foehnlike wind, observational data from Korea Meteorological Administration (KMA) and the Weather Research and Forecasting (WRF) model were utilized. In the backward trajectory analysis, trajectories of 100 air parcels were released from the surface over Hongcheon at 1600 LST on 1 August 2018. Among them, the 47 trajectories (38 trajectories) are tracked back above (below) heights of 1.4 km above mean sea level at 0900 LST 31 July 2018 and are defined as upper (lower) routes. Lagrangian energy budget analysis shows that for the upper routes, adiabatic heating (11.886 × 10³ J kg^-1) accounts for about 77% of the increase in the thermal energy transfer to the air parcels, while the rest (23%) is diabatic heating (3.650 × 10³ J kg^-1). On the other hand, for the lower routes, adiabatic heating (6.111 × 10³ J kg^-1) accounts for about 49% of the increase, the rest (51%) being diabatic heating (6.295 × 10³ J kg^-1). Even though the contribution of the diabatic heating to the increase in the air temperature rather varies according to the routes, the contribution of the diabatic heating should be considered. The diabatic heating is caused by direct heating associated with surface sensible heat flux and heating associated with the turbulent mixing. This mechanism is the Type 4 foehn described in Takane and Kusaka (2011). It is concluded that Type 4 foehn wind occurs and plays an important role in the extreme event on 1 August 2018.

• 대한기계학회논문집B
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• 제26권6호
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• pp.883-892
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• 2002

A numerical study has been carried out to investigate the flow and heat transfer from an aluminum foam heat sink in a confined channel. A uniform heat flux is given at the bottom of the aluminum foam heat sink, which is horizontally placed on the heated surface. The channel walls are assumed to be adiabatic. Cold air is supplied from the top opening of the channel and exhausted to the channel outlet. Comprehensive numerical solutions are acquired to the governing Wavier-Stokes and energy equations, using the Brinkman-Forchheimer extended Darcy model and the local thermal non-equilibrium model f3r the region of porous media. Details of flow and thermal fields are examined over wide ranges of the principal parameters; i.e., the Reynolds number Re, the height of heat sink h/H, porosity $\varepsilon$and pore diameter ratio $R_{H}$.

• 천문학회지
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• 제34권4호
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• pp.313-315
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• 2001

Some authors have concluded that spiral structures and shocks do not develop if an adiabatic index $\gamma$ > 1.16 is adopted in accretion disc modelling, whilst others have claimed that they obtained well defined spirals and shocks adopting a $\gamma$ = 1.2 and a $M_2/ M_1$ = 1 stellar mass ratio. In our opinion, it should be possible to develop spiral structures for low compressibility gas accretion discs if the primary component is a black hole. We considered a primary black hole of 8M0 and a small secondary component of 0.5M$\bigodot$ to favour spiral structures formations and possible spiral shocks via gas compression due to a strong gravitational attraction. We performed two 3D SPH simulations and two 2D SPH simulations and characterized a low compressibility model and a high compressibility model for each couple of simulations. 2D models reveal spiral structures existence. Moreover, spiral shocks are also evident in high compressibility 2D model at the outer disc edge. We believe that we could develop even well defined spiral shocks considering a more massive primary component.