• 제목/요약/키워드: Circular Disk

검색결과 142건 처리시간 0.028초

초경팁 납접형 둥근톱의 공구 마멸 (Tool Wear of the Tungsten Carbide Tipped Circular Saw)

  • 이재우
    • 한국정밀공학회지
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    • 제19권2호
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    • pp.228-236
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    • 2002
  • In this study, the carbon steels, SM20C were machined with the tungsten carbide tipped circular saw to clarify the cutting-off characteristics in terms of tool wear. The results show that an improved performance in view of both the tool wear and the cutting efficiency was obtained by using oil base cutting fluid at the cutting speed of 100m/min with the feed of 0.06mm/tooth. The rake angle of 10$^{\circ}$ , clearance angle of 8$^{\circ}$ , nose radius of R0.1mm, and end cutting edge champer of 0.1mm$\times$25$^{\circ}$ are believed as the best tool geometries. The tool wear decreases due to using the saw of the disk of STS5 and the tool material of P30.

감쇠판이 부착된 원기둥의 동유체력 특성 (Hydrodynamic Forces Characteristics of a Circular Cylinder with a Damping Plate)

  • 조일형
    • 한국해양공학회지
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    • 제25권1호
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    • pp.1-7
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    • 2011
  • The radiation of water waves by a heaving truncated circular cylinder with damping plate is solved in the frame of the three-dimensional linear potential theory. The damping plate has a distinct advantage in reducing the motion response of a floating circular cylinder by increasing the added mass and the damping coefficient. Using the matched eigenfunction expansion method, the characteristics of hydrodynamic added mass and the damping coefficient are investigated with various system parameters, such as the radius and submergence depth of the damping plate. It is found that both added mass and the damping coefficient are significantly increased due to the arranged features of the larger damping plate with shallow submergence, which are positive factors as a motion reduction device of the floating offshore platform. Also the numerical results for an oscillating submerged disk show that the added mass is negative and that the damping coefficient has a peak value at resonant frequency when submergence depth is sufficiently small.

왕복동형 압축기의 경사진 원판형 밸브리드에 대한 압력분포 측정 및 유동해석 (Flow Analysis and Measurement of Pressure Distribution along Inclined Circular Valve Reeds of Reciprocating Compressor)

  • 윤정;박종호;김태민;김경천
    • 대한기계학회:학술대회논문집
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    • 대한기계학회 2003년도 춘계학술대회
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    • pp.1942-1947
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    • 2003
  • The valve is the key part which governs the efficiency, noise and reliability of the compressor, so the development of analytical model about valve performance is necessary. As the valve leed is opened and closed by pressure pulsation, the flow characteristic of the refrigerant passing the valve is very important. In the present study, a circular disk with inclination is assumed to be the valve reed of a reciprocating compressor and numerical analysis of three dimensional velocity fields are perfomed for the radial flow through the valve model. The effective flow and force area which are required to predict the efficiency of the valve are measured and compared with the numerical analysis in this research.

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Design for Hybrid Circular Bragg Gratings for a Highly Efficient Quantum-Dot Single-Photon Source

  • Yao, Beimeng;Su, Rongbin;Wei, Yuming;Liu, Zhuojun;Zhao, Tianming;Liu, Jin
    • Journal of the Korean Physical Society
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    • 제73권10호
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    • pp.1502-1505
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    • 2018
  • We present a design for hybrid circular Bragg gratings (hCBGs) for efficiently extracting single-photons emitted by InAs quantum dots (QDs) embedded in GaAs. Finite-difference time-domain simulations show that a very high photon collection efficiency (PCE) up to 96% over a 50 nm bandwidth and pronounced Purcell factors up to 19 at cavity resonance are obtained. We also systematically investigate the geometry parameters, including the $SiO_2$ thickness, grating period, gap width and the central disk radius, to improve the device performances. Finally, the PCEs and the Purcell factors of QDs located at different positions of the hCBG are studied, and the results show great robustness against uncertainties in the location of the QD.

고유변형도법을 이용한 삼각가열에 의한 판 변형의 시뮬레이션 (Simulation of Plate Deformation due to Triangle Heating Using Inherent Strain Method)

  • 장창두;고대은;하윤석
    • 대한조선학회논문집
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    • 제45권6호
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    • pp.703-709
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    • 2008
  • In the shipyard, line heating and triangle heating are two major processes for forming curved plates in various shapes. While there have been many studies on line heating, triangle heating has been rarely studied due to its complicated heating process with irregular multi-heating paths and highly concentrated heat input. As the triangle heating process is one of the most labor-consuming jobs in shipyards, it is essential to study the automation as well as improvement of triangle heating process in order to increase hull forming productivity. In this study, a pioneering attempt to simulate triangle heating was made. A circular disk-spring model was proposed for elasto-plastic analysis procedure of triangle heating and the inherent strain method was also used to analyze the deformation of plates. Simulation results were compared with those of experiments and showed good agreement. It is shown that the present approach including analysis model used in this study is effective to simulate the triangle heating for plate forming process in shipbuilding.

HDD의 동시 회전 디스크 내부 유동 패턴의 가시화 (Visualization of the Flow Pattern Between Co-rotating Disks in HDD)

  • 공대위;주원구;도덕희
    • 한국가시화정보학회:학술대회논문집
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    • 한국가시화정보학회 2003년도 추계학술대회 논문집
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    • pp.67-70
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    • 2003
  • Hard disk drives (HDD) in computer are used extensively as data storage capacity. The trend in the computer industry to produce smaller disk drives rotating at higher speeds requires an improved understanding of fluid motion in the space between disks. Laser sheet and digital camera was used for 2-dimensional visualization of the unsteady flow between the center pair of two co-rotating disks in air with a cylindrical enclosure (or shroud). Geometric parameters are gap height (H) between disks, and gap distance (G) between disk tip and shroud. The lobe-structured boundary between inner region and outer region was detected by inserted particles, and the number of dominant vortices was determined clearly It is found from flow visualization that the number of vortex cells can be correlated with Reynolds number based on H which is defined as $Re_H={\Omega}RH/v$ ranging from $3.18\times10^3\;to\;1.43\times10^4$, and decreases as the disk speed increases. The lobe pattern by vortex cells is changed to a circular pattern for the wide gap than narrow one.

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원통형 케이스 내의 동시회전 디스크 내부 유동패턴의 가시화 (Visualization of the Flow Pattern Between Co-rotating Disks in Shroud)

  • 공대위;주원구
    • 대한기계학회:학술대회논문집
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    • 대한기계학회 2004년도 춘계학술대회
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    • pp.1661-1665
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    • 2004
  • Hard disk drives (HDD) in computer are used extensively as data storage capacity. The trend in the computer industry to produce smaller disk drives rotating at higher speeds requires an improved understanding of fluid motion in the space between disks. Laser sheet and digital camera was used for 2-dimensional visualization of the unsteady flow between co-rotating disks in air with a cylindrical enclosure (or shroud). Geometric parameters are gap height (H) between disks, and gap distance (G) between disk tip and shroud. The lobe-structured boundary between inner region and outer region was detected by inserted particles, and the number of dominant vortices was determined clearly It is found from flow visualization that the number of vortex cells can be correlated with Reynolds number based on H which is defined as $Re_H={\Omega}RH/v$ ranging from $7.96{\times}10^2$ to $1.43{\times}10^4$, and decreases as the disk speed increases. The lobe pattern by vortex cells is changed to a circular pattern for the wide gap than narrow one.

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SPH SIMULATIONS OF BARRED GALAXIES: DYNAMICAL EVOLUTION OF GASEOUS DISK

  • ANN HONG BAE;LEE HVUNG MOK
    • 천문학회지
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    • 제33권1호
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    • pp.1-17
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    • 2000
  • We have performed extensive simulations of response of gaseous disk in barred galaxies using SPH method. The gravitational potential is assumed to be generated by disk, bulge, halo, and bar. The mass of gaseous disk in SPH simulation is assumed to be negligible compared to the stellar and dark mass component, and the gravitational potential generated by other components is fixed in time. The self-gravity of the gas is not considered in most simulations, but we have made a small set of simulations including the self-gravity of the gas. Non-circular component of velocity generated by the rotating, non-axisymmetric potential causes many interesting features. In most cases, there is a strong tendency of concentration of gas toward the central parts of the galaxy. The morphology of the gas becomes quite complex, but the general behavior can be understood in terms of simple linear approximations: the locations and number of Lindblad resonances play critical role in determining the general distribution of the gas. We present our results in the form of 'atlas' of artificial galaxies. We also make a brief comment on the observational implications of our calculations. Since the gaseous component show interesting features while the stellar component behaves more smoothly, high resolution mapping using molecular emission line for barred galaxies would be desirable.

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Evolution of the spin of late-type galaxies caused by galaxy-galaxy interactions

  • Hwang, Jeong-Sun;Park, Changbom;Nam, Soo-hyeon;Chung, Haeun
    • 천문학회보
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    • 제46권1호
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    • pp.56.3-57
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    • 2021
  • We use N-body/hydrodynamic simulations to study the evolution of the spin of a Milky Way-like galaxy through interactions. We perform a controlled experiment of co-planner galaxy-galaxy encounters and study the evolution of disk spins of interacting galaxies. Specifically, we consider the cases where the late-type target galaxy encounters an equally massive companion galaxy, which has either a late or an early-type morphology, with the closest approach distance of about 50 kpc, in prograde or retrograde sense. By examining the time change of the circular velocity of the disk material of the target galaxy from each case, we find that the target galaxy tends to lose the spin through prograde collisions but hardly through retrograde collisions, regardless of the companion galaxy type. The decrease of the spin results mainly from the deflection of the orbit of the disk material by tidal disruption. It is found that the spin angular momentum of the disk of the target galaxy decreases by 15 - 20% after a prograde collision. We conclude that the accumulated effects of galaxy-galaxy interactions will play an important role in determining the angular momentum of late-type galaxies at current stage.

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슬라이드 밸브 급폐쇄에 따른 디스크 주위 비정상유동의 PIV계측에 관한 연구 (A Study on PIV Measurement of Unsteady Flow around Disk caused by Slide Type Valve Quick Closing)

  • 이철재;조대환
    • 해양환경안전학회지
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    • 제15권3호
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    • pp.251-256
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    • 2009
  • 이 연구에서는 전 유동장의 순간속도를 계측 할 수 있는 PIV계측기법을 슬라이딩 밸브의 폐쇄 직후에 적용하고 짧은 시간에 발생하는 디스크 주위의 비정상 속도를 계측하여 유동특성을 실험적으로 고찰하였다. 순간유동장을 분석한 결과를 기존의 압력변동을 측정한 연구 결과에 비교 검토한 결과 슬라이드 밸브 급폐쇄에 따른 속도변동이 크게 나타나는 시간구간은 0.1초 이내이고 주기는 0.12초로 추정되었다. 또한 원관 내부의 디스크 주위유동은 상부부터 폐쇄되면서 유로가 좁아져 순간적으로 빠르게 하류로 진행하였으며 폐쇄직후에 역류하는 속도의 크기는 4/120초까지 감소하다가 다시 증가하는 경향을 보였다. 그리고 완전 폐쇄 후 상류 측으로 역류하는 흐름의 영향으로 y/D=0.2 하부 영역에 역류하는 속도성분이 나타났으며, y/D=0.7, x/D=-0.3의 근방에서 0.2D 크기의 회전와류가 관찰되었다.

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