• 제목/요약/키워드: Rotating-axis

검색결과 288건 처리시간 0.025초

부분용융법을 이용한 BSCCO 초전도 튜브 특성 (Characteristics of BSCCO Superconductor Tube Using Partial Melting Process)

  • 박용민;장건익
    • 한국초전도저온공학회:학술대회논문집
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    • 한국초전도저온공학회 2001년도 학술대회 논문집
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    • pp.25-28
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    • 2001
  • Bi-2212 HTS tube was fabricated by centrifugal forming process(CFP). As a variation of melt casting process(MCP) or centrifugal casting technique, the centrifugal forming process is a flexible method for manufacturing Bi-2212 bulk tubes and has been optimized to achieve smooth surface and uniform thickness. At this process, the slurry was prepared in the mixing ratio of 10:1 between Bi-2212 powder and binder and initially charged into the rotating mold under the speed of 300~450 rpm Heat-treatment was performed at the temperature ranges of 860 ~ $890^{\circ}C$ in air for partial melting. The HTS tube fabricated by centrifugal forming process at $890^{\circ}C$ under the rotating speed of 450 rpm was highly densified and the plate-like grains with more than 20$\mu$m were well oriented along the rotating axis. The measured Tc and Jc at 10K were around 85K and 3,000A/cm2 respectively.

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열처리 조건에 따른 Bi-2212 초전도 튜브의 특성 (Characteristics of Bi-2212 Superconductor Tube Depending on Heat-treatment Conditions)

  • 박용민;장건익
    • 한국전기전자재료학회논문지
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    • 제14권7호
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    • pp.606-610
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    • 2001
  • Bi-2212 HTS tube was fabricated by centrifugal forming and partial melting processes. Bi-2212 bulk tube has been optimized to achieve smooth surface and uniform thickness. The slurry was prepared in the mixing ratio of 10:1 between Bi-2212 powder and binder and initially charged into the rotating mold under the speed of 300~450 rpm. Heat-treatment was performed at the temperature ranges of 860~89$0^{\circ}C$ in air for partial melting. the HTS tube fabricated by centrifugal forming process at 89$0^{\circ}C$ under the rotating speed of 450 rpm was highly densified and the plate-like grains with more than 20${\mu}{\textrm}{m}$ were well oriented along the rotating axis. The measured Tc and J$_{c}$ at 10K on specimen heat treated at 89$0^{\circ}C$ was around 85 K and 1,200 A/$\textrm{cm}^2$ respectively.y.

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하나의 실린더가 회전하는 수평 환형 공간에서의 혼합 대류 (Mixed Convection in a Horizontal Annulus with a Rotating Cylinder)

  • 유주식;하대홍
    • 한국전산유체공학회지
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    • 제6권3호
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    • pp.1-9
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    • 2001
  • Mixed convection in a horizontal annulus is considered, and the effect of a forced flow on the natural convective flow is investigated. The inner cylinder is hotter than the outer cylinder, and the outer cylinder is rotating with constant angular velocity with its axis at the center of the annulus. The unsteady streamfunction-vorticity equation is solved with a finite difference method. For the fluid with Pr=0.7, there appear flows with two eddies, one eddy, or no eddy according the Rayleigh and Reynolds numbers. The rotation of the outer cylinder reduces the heat transfer rate at the wall of the annulus. The oscillatory multicellular flow of a low Prandtl number fluid with Pr=0.01 can be effectively suppressed by the forced flow.

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2차 모멘트 난류모형에 의한 회전하는 평행 평판유동 해석 (Numerical Simulation of Rotating Channel Flows Using a Second Moment Turbulence Closure)

  • 신종근;최영돈
    • 대한기계학회논문집B
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    • 제24권4호
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    • pp.578-588
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    • 2000
  • A low-Reynolds-number second moment turbulence closure is improved with the aid of DNS data. For the model coefficients of pressure-strain terms, we adopted Shima's model with some modification. Shin and Choi's new dissipation-rate equation is employed to simulate accurately the turbulence energy dissipation rate distribution in the near wall sublayer. The results of computations are compared with DNS, LES data and experimental data for turbulent plane channel flow with rotation about spanwise axis. The present second moment closure achieves a level of agreement similar to that for the non-rotating. In particular, it accurately captures the distribution of turbulence energy dissipation rate in the near wall region.

배경회전이 있는 싱크 유동의 이론 및 수치해석 (Theoretical and Numerical Analysis of Sink Flows under a Background Rotation)

  • 서용권;여창호
    • 한국가시화정보학회지
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    • 제2권2호
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    • pp.38-44
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    • 2004
  • Theoretical and numerical studies are given to the sink flows within a rotating circular tank driven by the fluid withdrawal from a bottom circular hole. It was found that, when the upper free surface was set with no-slip boundary conditions, the Ekman boundary-layer develops not only above the bottom surface but under the top surface. The sink fluid is coming from the two Ekman layers, and the mass transfer from the bulk, inviscid region is dependent on the rotational speed. It is also remarkable to see that all the fluid gathered along the axis flows in a form of rapidly rotating fluid column haying almost the same diameter as the bottom hole.

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불안정 성층화를 가진 원통형 용기 내의 회전유동에 관한 연구 (Rotating Flows in a Circular Cylinder with Unstable Stratification)

  • 김재원
    • 한국전산유체공학회지
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    • 제3권2호
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    • pp.27-38
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    • 1998
  • Rotating flow of a stratified fluid contained in a circular cylinder with unstable temperature gradient imposed on the side wall of it has been numerically studied. The temperatures at the endwall disks are constant. The top disk of the container is coider than that of the bottob disk, as much as the temperature difference n${\Delta}$T, (0${\leq}$n${\leq}$3). Flows in the vessel are driven by an impulsive rotation of the hot bottom disk with respect to the central axis of the cylinder. Flow details have been acquired. For this flow, the principal balance in the interior core is characterized by a relationship between the radial temperature gradient and the vertical shear in the azimuthal velocity. As the buoyancy effect becomes appreciable, larger portions of the meridional fluid transport are long-circuit from the bottom disk to the interior region via the side wall.

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Astrophysical Jet Engine and the Rotating Disk-Jet System of NGC 1333 IRAS 4A2

  • 최민호;강민주
    • 천문학회보
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    • 제36권1호
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    • pp.84.2-84.2
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    • 2011
  • Astrophysical jets play important roles in many interesting astronomical phenomena, such as star formation, gamma-ray bursts, and active galactic nuclei. The jets are thought to be driven by rotating disks through magneto-centrifugal processes. However, quantitative understanding of the jet-driving mechanism has been difficult because examples showing rotation in both disk and jet are rare. One of the important quantities in the models of jet engine is the size of the jet-launching region. The bipolar jet of the NGC 1333 IRAS 4A2 protostar shows a lateral velocity gradient, which suggests that the SiO jet is rotating around its axis. The jet rotation is consistent with the rotation of the accretion disk. The disk-jet rotation kinematics suggests that the jet-launching region on the disk, or the outflow foot-ring, has a radius of about 2 AU, which supports the disk-wind models.

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골프공 회전 무게중심 검출 시스템 (A development of automatic detecting equipment for rotation axis of golf ball)

  • 이재웅;현웅근;오준호
    • 한국정보통신학회:학술대회논문집
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    • 한국정보통신학회 2016년도 추계학술대회
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    • pp.540-545
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    • 2016
  • 본 연구에서는 딤플공의 회전축을 찾아가는 상태를 측정하는 영상 기반 시스템을 개발였다. 공기압으로 골프공을 부양시키면 표면에 딤플이 있는 골프공은 자이로의 원리에 의해 강하게 회전하면서 부양하고 47g의 골프공 무게에 의해 일정 높이에서 정지하면서 무게중심 회전축울 중심으로 일정하게 회전하게 된다. 본 장치는 공기 중으로 부양하면서 회전하는 골프공이 고정된 회전축을 찾기까지의 시간을 검출하는 장치 및 최적의 공기압을 찾아내는 시스템이다.

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10kW급 상반전 풍력터빈 로터의 설계와 성능 평가에 관한 연구 (Design and Performance Evaluation of a 10kW Scale Counter-Rotating Wind Turbine Rotor)

  • 황안둥;양창조
    • 해양환경안전학회지
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    • 제20권1호
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    • pp.104-112
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    • 2014
  • 상반전 풍력터빈은 설계와 성능 관점에서 최근 각광을 받기 시작하고 있다. 본 논문은 NREL S822, S823을 이용하여 설계 및 모델링한 상반전 풍력터빈에 대해 연구를 수행하였다. 본 논문은 수치해석 기법을 통하여 단일 풍력터빈과 상반전 풍력터빈을 각각 설계하고, 그 성능을 다양한 조건에서 비교하고자 하였다. 그 결과 상반전 풍력터빈은 단일 풍력 터빈에 비해 TSR 3~5 영역에서 보다 높은 성능계수를 나타냈으며, 그 보다 더 높은 TSR 영역에서는 낮은 성능계수를 나타내었다. 이것은 로터 상 하류의 간섭의 간섭 때문이며, 또한 본 연구에서는 낮은 영역의 TSR에서 운전되는 상반전 풍력터빈의 유효성을 함께 보였다.