• Composites Research
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• 제26권4호
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• pp.218-222
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• 2013

본 연구에서는 제강 과정의 부산물로 발생하는 슬래그의 구조용 충전제로써의 사용 가능성을 검토하였다. 고분자 기지 슬래그 복합재료를 제작하여 슬래그 입자의 크기(8~12 ${\mu}m$ and 12~16 ${\mu}m$), 체적 비(0-30 vol.%)에 따른 슬래그 복합재료의 기계적 특성에 대한 실험적 연구를 수행하였다. 복합재료 물성에 영향을 주는 요인인 입자 분산 도와 계면상태를 고찰하기 위해 각각 시편에 대하여 조직사진을 촬영하였다. 인장 시험 결과 슬래그 복합재료의 재료강성은 슬래그 체적비가 증가할수록 증가하였고 인장 강도는 체적비가 증가할수록 감소하였다. 슬래그 복합재료의 재료강성은 슬래그 입자의 크기의 변화에 따른 뚜렷한 경향성을 띄지 않았고 인장강도는 입자의 크기가 작을수록 높은 값을 가졌다. 조직 사진 촬영 결과 슬래그 복합재료가 양호한 계면상태를 보였고, 낮은 체적 비에서는 좋은 분산 도를 나타냈지만 체적비가 높아지면 입자들의 뭉침 현상이 발생하는 것을 알 수 있었다.

• 한국농공학회지
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• 제34권4호
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• pp.69-79
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• 1992

To estimate soil behavior and structural characteristics under the conditions of cyclic loading, freezing & thawing and initial state, several testing was performed and obtained following results. 1.After repeated freezing and thawing processes, original soil structure was destroyed and changed to globular structure from honeycomb or tube in its structure types. Also above processes resulted increasing the soil compression strain while decreasing the failure stress in stress-strain relationship and reached the soil structure into the mode of brittle fracture. Under cyclic loading conditions, soil cluster which was originally dispersed structure colloided with each other, seperated, and finally the soil failed due to the effect of overcompaction. 2.Through the stabilization processes seperated by four steps, the structure of soil skeleton was changed to quite different globular type. The degree of compressibility of soil was decreased in the normally consolidated zone, while the strength against external load increased due to soil particle stabilization. 3.Soil stress-strain chracteristics were largely influenced by repeated up and down processes of temperature. The maximum deformation was obtained in the case of temperature between 0 10˚C by the reseon of particle cluster reformation. 4.Soil compressibility was largely influenced by the optimum moisture content. Under freezing process, swelling could be found and its magnitude was proportional to the density of soil. 5.Density of soil was decreased as increasing the number or repeated freezing and thawing processes and the largest decreasing rate was found at the first turning point from freezing to thawing cycle.

• 한국식품과학회지
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• 제25권5호
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• pp.541-545
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• 1993

Sieve shaker와 Elzone particle size analyzer에 의한 두 가지 방법으로 제분방법에 따른 입자크기를 조사하였다. 제분방법별로 제조한 쌀가루의 입도분포를 측정한 결과 입자크기는 제분방법에 따라 영향을 받았으며 표준망체를 이용한 Sieve shaker 방법보다 Elzone particle size analyzer를 사용한 방법이 정확도가 우수하였다. 입도분포를 측정한 결과 Pin mill의 경우 $200{\sim}270$mesh가 30.38%으로 가장 많았고 $60{\sim}500mesh$의 분포도를 가졌다. Colloid mill은 $140{\sim}200mesh$가 가장 많았으며, $40{\sim}500mesh$의 분포도를 가졌다. Micro mill은 500mesh 이상이 41.62%로 가장 많았고 $140{\sim}500mesh$의 분포도를 보여주었다. Jet mill은 500 mesh 이상의 분포도로 입자크기가 가장 미세하였다. 또한 미세한 입자일수록 L간과 a값이 증가하였다. 쌀가루의 집합체를 살펴본 결과 습식제분은 분리된 쌀가루의 집합체형태로 구성되어 있고 건식제분은 분활된 조직체로 구성되었다. 전자주사현미경은 Elzone particle size analyzer 방법과 같은 입자분포도를 나타내었고 제분방법에 따라 구조의 특성을 보여주었다.

• 천문학논총
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• 제21권2호
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• pp.87-94
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• 2006

The COREA (COsmic ray Research and Education Array in Korea) project aims to build a ground array of particle detectors distributed over Korean Peninsular, through collaborations of high school students, educators, and university researchers, in order to study the origin of ultra high energy cosmic rays. COREA array will consist of about 2000 detector stations covering several hundreds of $km^2$ area at its final configuration and detect electrons and muons in extensive air-showers triggered by high energy particles. During the intial phase COREA array will start with a small number of detector stations in Seoul area schools. In this paper, we have studied by Monte Carlo simulations how to select detector sites for optimal detection efficiency for proton triggered air-showers. We considered several model clusters with up to 30 detector stations and calculated the effective number of air-shower events that can be detected per year for each cluster. The greatest detection efficiency is achieved when the mean distance between detector stations of a cluster is comparable to the effective radius of the air-shower of a given proton energy. We find the detection efficiency of a cluster with randomly selected detector sites is comparable to that of clusters with uniform detector spacing. We also considered a hybrid cluster with 60 detector stations that combines a small cluster with ${\Delta}{\iota}{\approx}100m$ and a large cluster with ${Delta}{\iota}{\approx}1km$. We suggest that it can be an ideal configuration for the initial phase study of the COREA project, since it can measure the cosmic rays with a wide range energy, i.e., $10^{16}eV{\leq}E{\leq}10^{19}eV$, with a reasonable detection rate.

• 한국시뮬레이션학회논문지
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• 제18권3호
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• pp.13-21
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• 2009

무선 센서 네트워크 환경에서 네트워크를 구성하는 센서 노드들은 라우팅 및 센싱 역할을 함께 수행해야 하기 때문에 각 센서 노드들은 항상 에너지 부담을 가지고 있다. 이러한 무선 센서 네트워크에 사용되는 센서는 무인으로 동작 되거나 사람이 접근하기 힘든 환경에서 동작하는 경우가 대부분이다. 또한 다량의 센서를 배치하여 무선 센서 네트워크를 형성 하는 경우가 많아 센서 노드의 크기가 작아야 하고, 가격이 저렴해야 하므로 노드에 공급할 수 있는 전원의 양과 데이터 처리 능력에 제한이 있게 된다. 본 논문에서는 무선 센서 네트워크 환경에서 센서 노드의 전력 소모를 줄이고, 망을 효율적으로 관리할 수 있는 알고리즘과 효율적인 라우팅 프로트콜을 제안하고, 제안한 알고리즘을 LEACH 프로토콜에 적용시켜 에너지 효율성을 검증하였다. Particle Sensor에서 이전 주기에 측정된 값과 현재 주기에 측정된 값을 비교하여 현재 측정된 값이 작거나 같으면 먼지가 감소하고 있다고 가정하고 다음 주기에 sleep모드를 설정해 주어 센서 노드의 에너지 소비를 줄여주는 알고리즘이다. 제안한 알고리즘의 시뮬레이션 결과를 보면 센서 노드의 에너지 소모를 향상시켜 주었고, LEACH 라우팅 프로토콜에 적용시킨 결과 네트워크의 수명을 향상 시켰다.

• 천문학회지
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• 제37권5호
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• pp.433-438
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• 2004

Clusters of galaxies generally form by the gravitational merger of smaller clusters and groups. Major cluster mergers are the most energetic events in the Universe since the Big Bang. The basic properties of cluster mergers and their effects are discussed. Mergers drive shocks into the intracluster gas, and these shocks heat the intracluster gas. As a result of the impulsive heating and compression associated with mergers, there is a large transient increase in the X-ray luminosities and temperatures of merging clusters. These merger boost can affect X-ray surveys of clusters and their cosmological interpretation. Similar boosts occur in the strong lensing cross-sections and Sunyaev-Zeldovich effect in merging clusters. Merger shock and turbulence associated with mergers should also (re)accelerate nonthermal relativistic particles. As a result of particle acceleration in shocks and turbulent acceleration following mergers, clusters of galaxies should contain very large populations of relativistic electrons and ions. Observations and models for the radio, extreme ultraviolet, hard X-ray, and gamma-ray emission from nonthermal particles accelerated in these shocks will also be described. Gamma-ray observations with GLAST seem particularly promising.

• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 1993년도 추계학술대회 논문집
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• pp.237-242
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• 1993

In the cluster tool, it is necessary to precisely control the vacuum pressure for the wafer transportation between transport module and cassette or process with the range of 10 $^{-4}$ to 5*10 $^{-5}$ torr. So we have designed the pressure control system for the transport module of the cluster tool and have evaluated its performance. Digital PID is utilized with the weighted sum of both three previous errors and one current error. The feedback signal is put into the nitrgen mass flow controller using the transport module controller. This pressure control system can prevent the transport module from the particle generation and backstreaming of hazardous process gases of the process chamber.

• 천문학회보
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• 제36권2호
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• pp.109.1-109.1
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• 2011

Shock waves are ubiquitous in astrophysical environments. In particular, shocks formed by merger of subclumps, infall of matter and internal flow motion in intracluster media (ICMs) and cluster outskirts are relatively weak with Mach number M ${\lesssim}$ a few. At such weak shocks, it has been believed that the diffusive shock acceleration (DSA) of cosmic rays is rather inefficient. Yet, the presence of nonthermal phenomena, such as radio halos and relics, suggests that contrary to the expectation, DSA as well as magnetic field amplification should operate at weak shocks in cluster environments. We recently initiated a study of weak, collisionless, astrophysical shocks using a PIC(Particle-in-Cell) code. The PIC code describes the motion of electron and ion particles under the electromagnetic field which is represented in grid zones. Here, we present a preliminary work of one-dimensional simulations. We show how shocks are set up as the turbulent electromagnetic field is developed in the shock transition layer, and discuss the implication on DSA and magnetic field amplification.

• 한국표면공학회:학술대회논문집
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• 한국표면공학회 2013년도 춘계학술대회 논문집
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• pp.207-207
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• 2013

증착온도 $700^{\circ}C$, 산소분압30mTorr에서 c-plane 사파이어 기판위에 PLD를 이용하여 ZnO nano-rod를 합성하였다. 거리가 멀어질수록 rod의 직경과 증착율이 감소하는 것을 확인 하였다. 이는 ablated particle이 가진 kinetic energy가 감소되고, cluster ion의 형성으로 인해 고온에서 rod가 형성될 수 있는 것으로 이해된다. 고진공에서는 kinetic energy가 감소되기 어렵기 때문에 nano-rod shape 형성은 불가능 할 것이며, ZnO와 같은 wurtzite 구조를 가진 물질의 타겟을 사용하여 cluster 형성 분위기에서 증착한다면 비슷한 경향을 나타낼 것으로 예상된다.

• 한국표면공학회지
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• 제39권4호
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• pp.153-159
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• 2006

Nanodiamond films were deposited on Si substrate by introducing a time dependent on/off modulation of $CH_4\;and\;O_2$ flows in a vertical-type microwave plasma enhanced chemical vapor deposition system. Surface morphology and diamond quality of the film were investigated as a function of the on/off modulation time interval. The diamond nucleation density on the substrate was enhanced under low temperature and low pressure condition. In addition, the diamond nucleation density was enhanced by increasing the on/off modulation time interval. Enhanced diamond quality was noticeable under the condition of a longer on/off modulation time interval. It was suggested that the nanodiamond nuclei formed the cluster formation.