• 한국정보과학회논문지:정보통신
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• 제30권6호
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• pp.787-798
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• 2003

IPv6(IP version 6)는 QoS(Quality of Service) 제공을 위해 플로우 레이블이라는 새로운 필드를 정의하고 있다. 기존 플로우 레이블 부여 방안인 랜덤 넘버(Random Number) 방식은 플로우에 대한 식별자 기능만을 수행함으로써 다양한 실시간 트래픽 특성에 따른 차별화된 서비스 제공에는 제약이 따른다. 본 논문에서는 플로우 레이블 필드를 플로우의 구성요소 및 QoS 파라미터로 사용하는 하이브리드(Hybrid) 방안을 제시하였다. 즉, 플로우 레이블에 사용되는 파라미터를 사용자가 표시하게 함으로써 실시간 트래픽에 대한 종단간 품질 보장과 함께 백본의 전송 자원을 효율적으로 사용할 수 있는 방법을 제시한다. 본 논문에서는 백본을 MPLS-TE(Multi Protocol Label Switching - Traffic Engineering) 환경으로 가정하고 시뮬레이션을 통해 랜덤 넘버 방식과 제안된 하이브리드 방식에 대한 성능을 평가하였다. 그 결과 하이브리드 방식이 랜덤 넘버 방식에 비해 처리 성능 및 백본 자원의 활용 측면에서 효율적인 것을 알 수 있었다.

• 한국재료학회지
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• 제32권9호
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• pp.384-390
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• 2022

A spin coating process for RRAM, which is a TiN/TiO₂/FTO structure based on a PTC sol solution, was developed in this laboratory, a method which enables low-temperature and eco-friendly manufacturing. The RRAM corresponds to an OxRAM that operates through the formation and extinction of conductive filaments. Heat treatment was selected as a method of controlling oxygen vacancy (V_O), a major factor of the conductive filament. It was carried out at 100 ℃ under moisture removal conditions and at 300 ℃ and 500 ℃ for excellent phase stability. XRD analysis confirmed the anatase phase in the thin film increased as the heat treatment increased, and the Ti³⁺ and OH- groups were observed to decrease in the XPS analysis. In the I-V analysis, the device at 100 ℃ showed a low primary SET voltage of 5.1 V and a high ON/OFF ratio of 10⁴. The double-logarithmic plot of the I-V curve confirmed the device at 100 ℃ required a low operating voltage. As a result, the 100 ℃ heat treatment conditions were suitable for the low voltage driving and high ON/OFF ratio of TiN/TiO₂/FTO RRAM devices and these results suggest that the operating voltage and ON/OFF ratio required for OxRAM devices used in various fields under specific heat treatment conditions can be compromised.

• 한국농림기상학회지
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• 제23권1호
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• pp.1-14
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• 2021

양파는 생산량 변동에 따른 가격 변화폭이 커 수급조절 대책이 필요한 대표적인 농산물로 대책의 실효성 증대를 위해서는 정확한 생산량 예측이 요구된다. 양파는 주로 노지에서 재배되기 때문에 기상변화로 인해 생산량의 정확한 추정이 어렵다. 많은 선행연구가 다양하게 시도되었지만 신뢰도 높은 분석결과를 도출하기 위한 양질의 생육 실측자료가 부족한 실정이었다. 선행연구는 기상여건을 통제한 실험설계를 통해 얻어낸 자료를 분석하거나 기상자료와 생육자료 간 지역적 범위가 동일하지 않는 연구가 대다수여서 생육요인과 기상요인 간의 관계를 명확하게 규명하기에는 한계가 있었다. 본 연구는 자연적으로 노출된 환경에서 수집한 생육 실측조사 자료와 함께 실측 대상 지역의 추정 기상자료를 사용하여 생육요인과 기상요인 간 관계를 실증적으로 분석하였다. 양파의 생산량은 구중으로 결정되지만 지상부 생육상황에 따라 구의 생장이 부진할 수 있기 때문에 본 연구에서는 구중뿐만 아니라 지상부 생장과 어떤 기상요인이 중요한지 탐색하였다. 시기별로 생육요인과 통계적으로 유의한 상관관계를 갖는 기상요인을 탐색한 후, 랜덤 포레스트 기법을 이용하여 요인들의 영향력 및 중요도를 분석하였다. 주목할만한 결과로 3월 초에는 일사량이 지상부 생육에 긍정적인 영향을 주었으며, 3월 말에는 강수량과 지상부 생장 간 음의 상관관계에 있어 가뭄에 의한 피해를 언급한 기존 문헌과 상이하였다. 또한 수확기에는 강수량과 일조시간이 지상부와 지하부 생육에 미치는 영향이 유의하게 반대로 나타났다. 본 연구에서 밝혀낸 생육시기별 중요 기상요인은 양파의 생육모형과 생산량 예측모형 개발 연구를 위한 기초자료로 유용하게 활용될 것으로 기대된다.

• 대한기계학회논문집A
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• 제23권6호
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• pp.968-978
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• 1999

The effective elastic properties of materials containing spherical inclusions were calculated by the elastic wave scattering theory. In the formulation additional scattering fields by the presence of random multiple scatterers that affects the effective properties were found by the single scattering approximation. In calculating the scattering fields the ensemble average on the displacements and strains inside the scatterer was found from the static approximation at long wavelength limit. The displacements were assumed to be equal to the incident field, while the strains were calculated by Eshelby's equivalent inclusion principle on the single inclusion problem. Four different models were considered and they reflected different degrees of multiple scattering effects based on the approximation introduced in the process of embedding the inclusion in the matrix. The expressions for the effective elastic constants were given in each model, and their relations to the results obtained from other scattering theory and elasticity theory were discussed. The theoretical predictions were compared with experimental results on the epoxy matrix composites containing tungsten particles of different sizes and volume fractions

• 천문학회지
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• 제40권4호
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• pp.165-169
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• 2007

The numerical simulations associated with the interaction of High Velocity Clouds (HVC) with the Magnetized Galactic Interstellar Medium (ISM) are a powerful tool to describe the evolution of the interaction of these objects in our Galaxy. In this work we present a new project referred to as Theoretical Virtual i Observatories. It is oriented toward to perform numerical simulations in real time through a Web page. This is a powerful astrophysical computational tool that consists of an intuitive graphical user interface (GUI) and a database produced by numerical calculations. In this Website the user can make use of the existing numerical simulations from the database or run a new simulation introducing initial conditions such as temperatures, densities, velocities, and magnetic field intensities for both the ISM and HVC. The prototype is programmed using Linux, Apache, MySQL, and PHP (LAMP), based on the open source philosophy. All simulations were performed with the MHD code ZEUS-3D, which solves the ideal MHD equations by finite differences on a fixed Eulerian mesh. Finally, we present typical results that can be obtained with this tool.

• Wind and Structures
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• 제18권6호
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• pp.599-618
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• 2014

In this study, a square rectangular tall building is considered to investigate the effects of turbulence integral length scale and turbulence intensity on the along-wind responses, across-wind responses and torsional responses of the tall building by Large Eddy Simulation (LES). A recently proposed inflow turbulence generator called the discretizing and synthesizing random flow generation (DSRFG) approach is applied to simulate turbulent flow fields. It has been proved that the approach is able to generate a fluctuating turbulent flow field satisfying any given spectrum, desired turbulence intensity and wind speed profiles. Five profiles of turbulence integral length scale and turbulence intensity are respectively generated for the inflow fields by the DSRFG approach for investigating the effects of turbulence integral length scale and turbulence intensity on the wind-induced responses of the tall building. The computational results indicate that turbulence integral length scale does not have significant effect on the along-wind (displacement, velocity and acceleration) responses, across-wind displacement and velocity responses, while the across-wind acceleration and torsional responses vary without a clear rule with the parameter. On the other hand, the along-wind, across-wind and torsional responses increase with the growth of turbulence intensity.

• 대한기계학회논문집
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• 제19권9호
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• pp.2181-2193
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• 1995

The effective elasticity and conduction of composite materials containing arbitrarily oriented multiple phases has been analyzed using the concept of orientation-dependent average fields and concentration factors. The analysis provided closed form expressions for the effective stiffnesses and conductivities. Under the prescribed boundary conditions, the concentration factors were evaluated by the equivalent inclusion principle, through which the interaction between various phases is approximated by the Mori-Tanaka mean-field approximation. SiC particulate(SiC$_{p}$) reinforce aluminum(Al) matrix composites were fabricated and their elastic constants and electrical conductivities were measured together with a careful study of their microstructure. The measured properties showed a systematic anisotropy and this behavior could be attributed to the preferred orientation of SiC$_{p}$. The theoretical model developed was applied to the computation of the anisotropic properties of these composites. Both two-phase and three-phase composites were considered based on the microstructural information. The SiC$_{p}$ was modeled as an ellipsoid with planar random orientation distribution in the extruded Al/SiC$_{p}$ composites. The effect of extraneous phase such as intermetallic compounds was also investigated.tigated.

• 천문학회지
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• 제29권spc1호
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• pp.151-154
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• 1996

We examine the observations of large-scale magnetic fields in the Universe. We begin at the largest scale with clusters of galaxies and work our way down through galaxies and finally to the Milky Way. on which we concentrate in detail. We examine the observations of the Galactic magnetic field, and their interpretation, under the philosophy that the Galactic magnetic field is like that in other spiral galaxies. We use pulsar data. diffuse Galactic synchrotron emission, and starlight polarization data to discuss the Galaxy's global magnetic configuration and the uniform ($B_u$), random ($B_r$), and total ($B_t$) components of the field strength. We find disagreement among conclusions derived from the various data sets and argue that the pulsar data are not the best indicator for large-scale Galactic field. Near the Solar circle, we find that the azimuthal average of $B_t$ is 4.2$\mu$G and we adopt $B_u\~$2.2 and $B_r\~3.6{\mu}G$. $B_t$ is higher in spiral arms, reaching $\~5.9{\mu}G$. $B_t$ is higher for smaller $R_{Gal}$, reaching $\~8.0{\mu}G$ for $R_{Gal}$ = 4.0 kpc. The pattern of field lines is not concentric circles but spirals. The inclination of the magnetic spiral may be smaller than that of the Galaxy's spiral arms if our sample, which refers primarily to the interarm region near the Sun, is representative. However, it is not inconceivable that the local field lines follow the Galaxy's spiral pattern, as is observed in external galaxies.

• Environmental Engineering Research
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• 제17권2호
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• pp.83-88
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• 2012

Currently, the technology of $CO_2$ capture and storage (CCS) has become the main issue for climate change and global warming. Among CCS technologies, the prediction of $CO_2$ behavior underground is very critical for $CO_2$ storage design, especially for its safety. Hence, the purpose of this paper is to model and simulate $CO_2$ flow and its heat transfer characteristics in a storage site, for more accurate evaluation of the safety for $CO_2$ storage process. In the present study, as part of the storage design, a micro pore-scale model was developed to mimic real porous structure, and computational fluid dynamics was applied to calculate the $CO_2$ flow and thermal fields in the micro pore-scale porous structure. Three different configurations of 3-dimensional (3D) micro-pore structures were developed, and compared. In particular, the technique of assigning random pore size in 3D porous media was considered. For the computation, physical conditions such as temperature and pressure were set up, equivalent to the underground condition at which the $CO_2$ fluid was injected. From the results, the characteristics of the flow and thermal fields of $CO_2$ were scrutinized, and the influence of the configuration of the micro-pore structure on the flow and scalar transport was investigated.

• Biotechnology and Bioprocess Engineering:BBE
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• 제8권2호
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• pp.64-75
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• 2003

Aptamers are functional nucleic acids that can specially bind to proteins, peptides, amino acids. nucleotides, drugs, vitamins and other organic and inorganic compounds. The aptamers are identified from random DNA or RNA libraries by a SELEX (systematic evolution of ligands by exponential amplification) process. As aptamers have the advantage, and potential ability to be released from the limitations of antibodies, they are attractive to a wide range of therapeutic and diagnostic applications. Aptamers, with a high-affinity and specificity, could fulfil molecular the recognition needs of various fields in biotechnology. In this work, we reviewed some aptamer Selection techniques, properties, medical applications of their molecules and their biotechnological applications, such as ELONA (enzyme linked oligonucleotide assay), flow cytometry, biosensors, electrophoresis, chromatography and microarrays.