• 콘크리트학회지
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• 제28권1호
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• pp.51-54
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• 2016

• 한국도로학회:학술대회논문집
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• 한국도로학회 2001년도 학술발표회 논문집
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• pp.87-91
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• 2001

• 한국도로학회:학술대회논문집
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• 한국도로학회 2005년도 학술발표회 논문집
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• pp.233-238
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• 2005

• 한국도로학회논문집
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• 제11권2호
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• pp.185-194
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• 2009

초속경 라텍스개질 콘크리트(VES-LMC)를 포함한 고성능 콘크리트는 낮은 물-시멘트비, 높은 결합재량 및 고성능감수제의 사용 등으로 인해 자기수축(Autogenous Shrinkage)이 1종 콘크리트(OPC)보다 크게 나타난다. 초속경 라텍스개질 콘크리트의 배합특성은 낮은 물-시멘트비(0.38), 높은 단위시멘트량($390kg/m^3$) 및 라텍스첨가(단위시멘트량 대비 15%)로 구성되므로, 자기수축이 크게 발생할 수 있고, 또한 콘크리트 타설 후 3시간 이내에 발생하는 급격한 수분소산(Water Dissipation)과 수분증발은 자기수축을 증가시킬 수 있다. 본 논문의 목적은 현장에서 작업시간 확보를 목적으로 사용되는 지연제 첨가량 변화에 따른 초기수축, 온도변형 및 자기수축을 평가하는 것이다. 실험결과 지연제의 첨가는 콘크리트의 최대 수화열에 영향을 미치지 않는 것으로 나타났으며, 초속경 라텍스개질 콘크리트의 초기 팽창은 일부 자기팽창의 영향이 있기는 하지만 대부분이 열팽창에 기인하는 것으로 나타났다. 지연제 첨가량이 증가함에 따라 자기수축이 감소하는 것으로 나타났지만, 지연제의 과도한 사용은 과도한 초기 팽창을 일으킬 수 있으므로 현장조건을 고려하여 신중하게 결정되어야 한다.

• 한국산학기술학회논문지
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• 제11권3호
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• pp.1040-1046
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• 2010

급속경화 콘크리트의 가장 큰 단점은 단시간 내에 발생하는 급격한 수화발열 반응으로 인해 초기팽창이나 수축이 매우 크게 일어나 균열이 발생할 가능성이 높다는 것이다. 그러나 플라이 애시가 사용되면 콘크리트의 수화열을 낮출 수 있으므로 초기팽창과 수축을 현저히 줄일 수 있어 균열발생 억제에 효과적일 수 있다. 초속경 라텍스개질 콘크리트(VES-LMC)는 우수한 재료특성에도 불구하고, 재료 자체의 높은 수화열로 인해 균열이 발생하는 사례가 보고되고 있다. 따라서 본 논문에서는 플라이 애시를 VES-LMC에 적용할 수 있는 방법을 고안하여, 균열에 대한 안정성을 확보하기 위한 연구를 수행하였다. 울트라파인 플라이 애시(Ultra-Fine Fly Ash ; UFFA)를 사용하여 조기강도 저하의 단점이 극복된 조건에서, 초기 수화열을 낮추고 수축을 저감하여 균열안정성을 확보할 수 있도록 하였다. 실험결과 조기 압축강도는 UFFA 혼입률이 증가함에 따라 다소 감소하지만, 재령 28일 강도는 통계학적으로 유사한 것으로 나타났다. 초기수축 실험결과 UFFA가 단위시멘트량대비 15%에서 20%까지 치환되면 최대수축을 43~47%까지 줄일 수 있어 초기수축 억제에 매우 효과적이므로 균열에 대한 안정성을 확보할 수 있는 것으로 나타났다.

• 산업기술연구
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• 제21권B호
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• pp.307-315
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• 2001

The purpose of this study was to provide the evaluation and prediction of strengths of SB latex modified concrete(LMC) using a statistical method and factorial experimental design method. The main experimental variables were as follows ; W/C ( 4 levels ; 31, 33, 35, 42%), S/a( 2 levels ; 55, 58%) and L/C(2 levels ; 5, 15%). The compressive strength and flexural strength of LMC were selected as a factor of response. The statistical method was carried out to analyze the results, together with factorial experimental design method and response surface method. The analysis showed that if L/C had been 15%, W/C appeared to be around 33% to achieve the design strength of $350kgf/cm^2$. In this case, the flexural strength and the slump came to around $68kgf/cm^2$ and 18cm, respectively. Eventhough the L/C varied, the design strength and W/C could be predictable together with slump value and flexural strength. As a result of series of experiments in this study, W/C and L/C were proved to be the main factors influencing on the compressive and flexural strength of LMC. Both of strength and slump values could be predictable from the mixing proportion of LMC.

• 산업기술연구
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• 제24권A호
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• pp.165-171
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• 2004

Latex modification of concrete provides the material with higher flexural strength, as well as high bond strength and reduced water permeability. However, If the thermal expansion properties of overlay concrete (latex-modified concretes) are big different from that of substrate (ordinary portland cement concrete), these would cause a big interfacial stresses and result in premature failure. Therefore, the purposes of this study were to investigate thermal expansion characteristics of latex-modified concrete with cement types. The result of thermal expansion showed the coefficient of thermal expansion of concretes increased with latex inclusion. The coefficient of thermal expansion of RSLMC was a little smaller than that of LMC, which might be due to the finer cement grain, compacter internal, and stiffer properties of concrete. However, the coefficients of LMC and RSLMC were quite similar to that of ordinary cement concrete. Thus, this would not cause an interfacial stresses and will enable to ensure long-term performance of concrete bridge deck overlays.

• 천문학회보
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• 제37권1호
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• pp.56.2-56.2
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• 2012

We present a study of the asymptotic giant branch (AGB) contribution to the total Ks band luminosity of star clusters in the Large Magellanic Cloud (LMC) as a function of age. AGB stars, a representative intermediate-age population, are a strong source of NIR to MIR emission so that they are a critical component for understanding the near-to-mid infrared observation of galaxies. Current calibration of IR emission in evolutionary population synthesis (EPS) models for galaxies is mainly based on a small number of LMC star clusters. However, each LMC star cluster with intermediate age contains only a few AGB stars so that it suffers from a stochastic effect. Therefore a large number of them are needed for solid calibration of the EPS models. We study physical properties of a large number of LMC star clusters to estimate the Ks band luminosity fraction of AGB stars in star clusters as a function of age. We discuss the stochastic effect in calibrating models, and the importance of this calibration for studying the evolution of not only nearby galaxies but also of high-z galaxies.

• 천문학회보
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• 제42권2호
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• pp.42.2-42.2
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• 2017

The Large Magellanic Cloud (LMC) is a unique target to study the detail structures of molecular clouds and star-forming regions, due to its proximity and face-on orientation from us. Most part of the astrophysical subjects for the LMC have been investigated, but the magnetic field is still veiling despite its role in the evolution of the interstellar medium (ISM) and in the main force to influence the star formation process. Measuring polarization of the background stars behind interstellar medium allows us to describe the existence of magnetic fields through the polarization vector map. In this presentation, I introduce the near-infrared polarimetric results for the $39^{\prime}{\times}69^{\prime}$ field of the northeastern region of the LMC and the N159/N160 star-forming complex therein. The polarimetric observations were conducted at IRSF/SIRPOL 1.4 m telescope. These results allow us to examine both the global geometry of the large-scale magnetic field in the northeastern region and the close structure of the magnetic field in the complex. Prominent patterns of polarization vectors mainly follow dust emission features in the mid-infrared bands, which imply that the large-scale magnetic fields are highly involved in the structure of the dust cloud in the LMC. In addition, local magnetic field structures in the N159/N160 star-forming complex are investigated with the comparison between polarization vectors and molecular cloud emissions, suggesting that the magnetic fields are resulted from the sequential formation history of this complex. I propose that ionizing radiation from massive stellar clusters and the expanding bubble of the ionized gas and dust in this complex probably affect the nascent magnetic field structure.

• 천문학회보
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• 제42권1호
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• pp.44.2-44.2
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• 2017

Multiple stellar systems composed of triple, double+double or double+triple, etc. are very rare and interesting objects for understanding the star formation and dynamical evolution. However, only six systems have been found to be a doubly eclipsing quadruple, which consists of two eclipsing binaries, and four systems to be a triply eclipsing hierarchical triple. Recently, the 15 doubly eclipsing multiple candidates located in the Large Magellanic Cloud (LMC) have been reported by the OGLE project. In order to examine whether these candidates are real multiple systems with eclipsing features, we performed a high-cadence time-series photometry for the LMC using the KMTNet (Korea Microlensing Telescope Network) 1.6 m telescopes in three site (CTIO, SAAO, and SSO) during 2016-2017. The KMTNet data will help reveal the photometric properties of the multiple-star candidates. In this paper, we present the VI light curves and their preliminarily analyses for 12 of the 15 eclipsing systems in the LMC, based on our KMTNet observations and the OGLE-III survey data from 2001-2009.