• 대한조선학회논문집
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• 제39권1호
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• pp.49-60
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• 2002

용접법은 선박 생산 공정에 있어서 금속 접합을 위해 가장 많이 사용되고 있다. 용접은 금속 접합을 위해 유용한 방법이지만 국부적 가열, 용융, 냉각으로 이어지는 열하중에 의하여 잔류응력과 잔류변형을 발생시킨다. 잔류응력은 구조물의 강도에 부정적인 영향을 끼치고, 잔류변형은 조립 작업에 부정적인 영향을 끼치게 된다. 그러므로 역학적 방법에 의한 잔류응력과 잔류변형의 예측은 이들을 제어할 수 있는 방법을 작업 전에 제시할 수 있도록 하므로, 선체 강도 확보와 선박 생산성 향상을 위하여 매우 중요한 문제라고 볼 수 있다. 본 논문에서는 이러한 배경에서 용접 현상을 가장 잘 시뮬레이션할 수 있는 방법인 유한요소법을 이용한 3차원 열탄소성 해석을 이용하였다. 열탄소성 해석을 위하여 온도분포를 계산한 후 계산된 온도분포를 이용하여 용접변형 및 응력을 순차적으로 계산하였다. 온도분포 계산을 위하여 용융과정을 엔탈피 방법을 이용하여 구현하였으며, 용접비드의 용입은 요소생성법을 이용하여 구현하였다. 본 연구에서 제안된 해석과정은 기존 연구에서 제시한 실험결과와 정성적으로 일치하는 결과를 주는 것을 확인하였다.

• 전기전자학회논문지
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• 제8권1호
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• pp.54-62
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• 2004

본 논문에서는 $GF(3^m)$상의 전류모드CMOS 승산기의 설계에 관하여 논의한다. 피 승산항에 원시원소 α를 곱함으로써 나타나는 피 승산항의 변화를 표준기저 표현을 이용하여 수식으로 전개하였다. $GF(3^m)$ 승산 회로를 구성하기 위하여 전류모드 CMOS를 사용하여 GF(3)상의 가산기와 승산기를 설계하였고 시뮬레이션 결과를 보였다. 기본 게이트들을 이용하여 $GF(3^m)$ 승산기를 설계하였고 m=3인 경우에 대하여 예를 보였다. 본 논문에서 제안한승산회로는 그 구성이 블록의 형태로 이루어지므로 $GF(p^m)$ 상에서 p와 m에 대한 확장이 용이하며, VLSI 구현에 유리하다 할 수 있다. 본 논문에서 제안한승산회로를 타 승산회로와 비교하였고, 개선효과를 확인하였다.

• 항공우주기술
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• 제11권2호
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• pp.109-116
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• 2012

우주발사체의 액체추진공급시스템에서 사용되는 연료 벤트/릴리프밸브는 안전밸브의 조합체로 지상에서 연료를 주입할 때와 비행 중에 추진제 탱크의 과압을 해소하는 역할을 한다. 벤트/릴리프밸브는 구동가스 공급에 의해 벤트밸브를 작동시키는 벤트모드와 설정된 압력을 유지하기 위해 자동으로 밸브를 개폐하는 릴리프모드로 작동한다. 본 논문에서는 해외발사체에 사용된(Saturn) 벤트/릴리프밸브 샘플을 이용하여 한국형발사체의 규격에 적용한 밸브 설계를 검토하였다. 또한 설계 검증 및 기본적인 작동 특성을 분석하기 위해 AMESim 상용코드를 이용하여 해석 모델을 구성하였다. 밸브 모델을 이용해서 동특성 해석을 수행하여 설계 변수에 대해 밸브 개폐 작동시간, 작동성능, 개폐압력을 예상하였다. 이를 통해 연료 벤트/릴리프밸브 설계변수에 따른 작동성을 파악하여 시제품 제작 전 의 상세설계 및 설계 경계조건을 제시하였다.

• 천문학회보
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• 제42권2호
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• pp.39.2-39.2
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• 2017

Over the last decade, deep studies of nearby galaxies have led to the discovery of vast stellar envelopes that are often rich in substructure. These components are naturally predicted in models of hierarchical galaxy assembly, and their observed properties place important constraints on the amount, nature, and history of satellite accretion. One of the most effective ways of mapping the peripheral regions of galaxies is through resolved star studies. Using wide-field cameras equipped to 8 m class telescopes, it has recently become possible to extend these studies to systems beyond the Local Group. Located at a distance of 3.6 Mpc, M81 is a prime target for wide-field mapping of its resolved stellar content. In this talk, we present the detailed results from our deep wide-field imaging survey of the M81 group with the Hyper Suprime-Cam (HSC), on the Subaru Telescope. We report on the analysis of the structures, stellar populations, and metallicities of old dwarf galaxies such as NGC3077, IKN, KDG061, as well as young stellar systems such as Arp's Loop and Holmberg IX. Several candidates for yet-undiscovered faint dwarf galaxies and young stellar clumps in the M81 group will also be introduced. The peculiar galaxy NGC3077 has been classified as the irregular galaxy. Okamoto et al. (2015, ApJ 809, L1) discovered an extended halo structure with S-shape elongated tails, obvious feature of tidal interaction. With a help of numerical simulation by Penarrubia et al. (2009, ApJ 698, 222), we will demonstrate that this tidal feature was formed during the latest close encounters between M81, M82, and NGC 3077, which induced star formation in tidally stripped gas far from the main bodies of galaxies. It is not clear whether the latest tidal interaction was the first close encounters of three galaxies. If NGC3077 is still surrounded by the dark matter halo, it implies that NGC3077 has undergone the first tidal stripping by larger companions. Kinematic studies of inter galactic globular clusters and planetary nebulae would tell us the past history of tidal interaction in this group of galaxies.

• 마이크로전자및패키징학회지
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• 제23권4호
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• pp.43-48
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• 2016

3-Dimensional System in Package (3-D SiP) structure (Amkor calls it mPossum-molded Possum) using double side Surface Mount Technology (SMT) and double side molding was evaluated in order to achieve small/thin form factor as well as good functionality by integration and double side layout. As the new platform on laminate substrate basis, molding process was challenge in mold flow balance at top and bottom side and package warpage control over the overall assembly process. There were two types of different molding process evaluated with 1) 1-step molding which was done at both side at the same time and 2) 2-step molding which was done at the conventional molding process twice. Mold simulation helped to narrow down the material selections and parameters available before actual sample build. There were many challenges for this first trial in design/ parameter and material types but optimized them to enable this structure.

• Nuclear Engineering and Technology
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• 제48권3호
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• pp.785-794
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• 2016

The Argonne National Laboratory of the United States and the Kharkov Institute of Physics and Technology of the Ukraine have been collaborating on the design, development and construction of a neutron source facility at Kharkov Institute of Physics and Technology utilizing an electron-accelerator-driven subcritical assembly. The electron beam power is 100 kW using 100-MeV electrons. The facility was designed to perform basic and applied nuclear research, produce medical isotopes, and train nuclear specialists. The biological shield of the accelerator building was designed to reduce the biological dose to less than 5.0e-03 mSv/h during operation. The main source of the biological dose for the accelerator building is the photons and neutrons generated from different interactions of leaked electrons from the electron gun and the accelerator sections with the surrounding components and materials. The Monte Carlo N-particle extended code (MCNPX) was used for the shielding calculations because of its capability to perform electron-, photon-, and neutron-coupled transport simulations. The photon dose was tallied using the MCNPX calculation, starting with the leaked electrons. However, it is difficult to accurately tally the neutron dose directly from the leaked electrons. The neutron yield per electron from the interactions with the surrounding components is very small, ~0.01 neutron for 100-MeV electron and even smaller for lower-energy electrons. This causes difficulties for the Monte Carlo analyses and consumes tremendous computation resources for tallying the neutron dose outside the shield boundary with an acceptable accuracy. To avoid these difficulties, the SOURCE and TALLYX user subroutines of MCNPX were utilized for this study. The generated neutrons were banked, together with all related parameters, for a subsequent MCNPX calculation to obtain the neutron dose. The weight windows variance reduction technique was also utilized for both neutron and photon dose calculations. Two shielding materials, heavy concrete and ordinary concrete, were considered for the shield design. The main goal is to maintain the total dose outside the shield boundary less than 5.0e-03 mSv/h during operation. The shield configuration and parameters of the accelerator building were determined and are presented in this paper.

• 천문학회보
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• 제42권1호
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• pp.52.1-52.1
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• 2017

Galaxy clusters are the most massive gravitationally bound systems and thus probably the most recent objects to form. One of promising routes to understand the assembly history of galaxy clusters is to measure observable quantities of components in clusters that are sensitive to the evolutionary state of the cluster. Recent deep observations on the nearby clusters show distinct diffuse intracluster light (ICL), that the light from stars are not bound any individual cluster galaxy, however until now this component has not been well studied due to its faint nature, with typical brightness of ~100 times fainter than the sky background. As shown in galaxy cluster simulation studies, the ICL abundance increases during various dynamical exchanges of galaxies such as the disruption of dwarf galaxies, major mergers between galaxies and the tidal stripping of galaxies. Thus, the ICL is an effective tool to measure the evolutionary stage of galaxy clusters. Moreover, the investigation of the ICL evolution mechanism will allow us understand the galaxy evolution process therein. In this pilot study, we target the Coma cluster, where the existing ICL studies are limited only in the central region. With large and uniform deep optical images from the Subaru telescope, available only recently (Okabe et al. 2014), we are developing a robust ICL measurement technique, extracting the ICL surface brightness and color profiles, which will allow us to study the origin of the ICL and its connection to the evolutionary history of the Coma cluster. For the next phase, we plan to utilize the plenty of spectroscopy data from the MMT telescope to compare ICL properties with the star formation history of the brightest cluster galaxies (BCG), and discuss the ICL formation mechanism of the Coma cluster by comparing the distribution of cluster galaxies with the distribution of diffuse light inside the Coma cluster.

• 한국정밀공학회지
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• 제27권5호
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• pp.56-62
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• 2010

This paper presents the development process of roof carrier assembly using a one side release system for a vehicle. An RV(Recreational Vehicle) or SUV(Sports Utility Vehicle) has a roof carrier system on an upper surface of a roof panel for loading large or long size baggage. Such a roof carrier system is comprised of a roof rack longitudinally mounted on a roof panel and cross bar perpendicularly installed in the horizontal direction. Several locking mechanisms used in most vehicle roof carrier systems are composed with both side releasable locking ones. The obvious drawback to this arrangement is that when the user desires to reposition the cross bar, first one of the locking members must be unlocked and then the user must walk around to the opposite side of the vehicle to unlock the other member. In this paper, we proposed a newly locking mechanism, which allows a user simultaneously place both locking members of the roof carrier in locked and unlocked positions. In order to estimate design compatibility, structural and modal analysis is performed. Furthermore, a prototype based on the proposed design has been made, and then durability test carried out. From the simulation and experimental results, the proposed roof carrier system is proved effective and safe.

• 한국가구학회지
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• 제27권3호
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• pp.237-245
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• 2016

Single households currently account for 26.5% of all households and their number is expected to continue to rise, reaching 34.5% by 2035. An analysis of the consumption trends and needs of single households shows that they are rising as a new consumer group with a focus on investment on the individual and favouring: small but high-tech products: efficient use of limited resources: safety and peace of mind: self-improvement and leisure. Products which meet such demands are having an impact on the growth of home-furnishing market. An analysis of companies in Korea's home-furnishing market, with examples like the lifestyle company IKEA, shows a variety of brands such as SPA brand, furniture specialist, distributor and character products. And yet most are OEM products which lack differentiated product lines and compete with similar display and distribution structure. We needs the Single household consumption tendency of home-furnishing market and differentiation strategy through product analysis. In order to increase the value of companies in the home-furnishing market, in addition to differentiated design, product competitiveness must aspire to higher customer satisfaction with easy assembly, innovation in logistics, innovative sales methods such as virtual-reality simulation for products and space, individually-tailored furniture for the needs of single household and products which combine smart technology. For home-grown home-furnishing brands to have competitiveness, they must leverage on the strengths of the industry, offering differentiated and competitive products in a wider range of areas with convergence functions as well as differentiation in consumer interface and application of advancing technology; in-depth product research is called for.

• 한국물환경학회지
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• 제26권1호
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• pp.168-176
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• 2010

This study proposes the improvement of the present Total Maximum Daily Load (TMDL) management system of MOE (Ministry of Environment). The margin of safety (MOS) is calculated by a method using standard error and a method using variability and uncertainty. The allocation of pollutant loads are calculated using three methods, equal load reduction method, equal percent removal method and method using equity standards. This study applied the improved TMDL management system to the Anyangcheon watershed. Since MOS varies from 12% to 44% due to the high variability of measured and simulated data, it must not be ignored in the TMDL. The method using equity standards is the most proper in this application since the others produced unrealistic allocations. Area, runoff, water use quantity, population and budget are considered for equity standards. This study shows that this allocation method can be also applicable for the administrative units as well as the sub-watersheds. Finally, Hydrologic Simulation Program-FORTRAN (HSPF) with the allocated pollutant load was used to confirm whether it satisfy the water quality standard or not. This study will be helpful to improve the MOS and allocation system TMDL in the future.