• Title/Summary/Keyword: Radiation pressure

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Two-Dimensional Simulation of Hg Flat Fluorescent Lamps for an LCD Backlight unit (액정디스플레이 후판광원용 평판형 수은 형광램프의 2차원 시뮬레이션 연구)

  • Yoon, Hyun-Jin;Lee, Hae-June
    • The Transactions of The Korean Institute of Electrical Engineers
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    • v.56 no.7
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    • pp.1275-1281
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    • 2007
  • The discharge phenomena in a flat fluorescent lamp for the backlight unit of liquid crystal displays are simulated by sung a two-dimensional fluid model. The numerical methods for the calculation of plasma dynamics and the radiation transport are introduced for the discharge simulation and for the transmission of the vacuum ultraviolet lights. The simulation results are presented to compare the luminance and the luminance efficacy with the variation of gas pressure, gas mixture ratio, driving voltage, and frequency.

ESTIMATION OF A GENERAL ALONG-TRACK ACCELERATION IN THE KOMPSAT-1 ORBIT

  • Lee, Byoung-Sun;Lee, Jeong-Sook;Kim, Jae-Hoon
    • Journal of Astronomy and Space Sciences
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    • v.19 no.2
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    • pp.89-96
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    • 2002
  • General along-track acceleration was estimated in the KOMPSAT-1 orbit determination process. Several sets of the atmospheric drag and solar radiation pressure coefficients were also derived with the different spacecraft area. State vectors in the orbit determination with the different spacecraft area were compared in the time frame. The orbit prediction using the estimated coefficients was performed and compared with the orbit determination results. The orbit prediction with the different general acceleration values was also carried out for the comparison

Numerical Study of Transmisson and Reflection Coefficients of a BBDB-Type Floating Breakwater (공기챔버형 부소파제의 투과 및 산란파 해석)

  • Hong, Do-Chun;Kim, Hyeon-Ju;Hong, Sa-Young
    • Journal of the Society of Naval Architects of Korea
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    • v.42 no.1 s.139
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    • pp.18-23
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    • 2005
  • The transmission and reflection coefficiencies of a BBDB-type floating breakwater in water of finite depth are studied taking account of fluctuating air pressure in the air chamber. The wave potential is calculated by a hybrid integral equation consisting of a Green integral equations associated with the Rankiue Green function inside the BBDB and the Kelvin Green function outside. The transmission and reflection coefficients of the breakwater are obtained directly from the potential solution in the outer region.

A STUDY ON THE RADIATION EFFETS OF MIS DIODES BY CONDUCTANCE TECH (MIS diodes의 컨덕턴스법에 관한 광조사 효과)

  • Yi, Seung-Hwan;Park, Chan-Won;Sung, Yung-Kwon
    • Proceedings of the KIEE Conference
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    • 1989.11a
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    • pp.111-113
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    • 1989
  • Recently nitrided oxides have been investigated for the application as the replacement of thermally grown oxides in the MIS devices. In this paper, nitrided oxides which were treated by the $N_2$ plasma were fabricated with the 350 $^{\circ}C$ substrate temperature, 0.2 torr chamber pressure, 250 watt RF power, 60 seem $N_2$ flow rate, 30 mins treatment time. After the UV light is radiated on the sample, it is noticed that the interface state density, $N_{ss}$, is slightly decreased. Under the UV light, the samples are stress by $\pm$DC bias. After those treatment interface state density. $N_{ss}$, is increased.

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ASTROPHYSICS OF DUSTY STELLAR WINDS FROM AGB STARS

  • Suh, Kyung-Won
    • Journal of The Korean Astronomical Society
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    • v.47 no.6
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    • pp.219-233
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    • 2014
  • The main site of dust formation is believed to be the cool envelopes around AGB stars. Nearly all AGB stars can be identified as long-period variables (LPVs) with large amplitude pulsation. Shock waves produce by the strong pulsation and radiation pressure on newly formed dust grains drive dusty stellar winds with high mass-loss rates. IR observations of AGB stars identify various dust species in different physical conditions. Radio observations of gas phase materials are helpful to understand the overall properties of the stellar winds. In this paper, we review (i) classification of AGB stars; (ii) IR two-color diagrams of AGB stars; (iii) pulsation of AGB stars; (iv) dust around AGB stars including dusty stellar winds; (v) dust envelopes around AGB stars; (vi) mass-loss and evolution of AGB stars; and (vii) contribution of AGB dust to galactic environments. We discuss various observational evidences and their theoretical interpretations.

STUDY ON NUMERICAL ANALYSIS AND TURBULENCE MODELS FOR ARC DISCHARGES IN HIGH-VOLTAGE INTERRUPTERS (초고압 차단부 아크방전 수치해석 및 난류모델에 관한 연구)

  • Kim, W.Y.;Lee, J.C.
    • 한국전산유체공학회:학술대회논문집
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    • 2010.05a
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    • pp.201-207
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    • 2010
  • In this study, we calculated arc discharges happened in high-voltage circuit breakers for understanding the complex physics and the probability of thermal breakdown. The four main parts of arc model for this virtual-reality are radiation, PTFE abaltion, Cu evaporation and turbulence. Among these important parts the turbulence model can be critical to the reliability of computation results during high-current period because the plasma flow is affected by high eat energy and mass momentum. Two kinds of turbulence model, zero-equation model and two-equation model, are applied for these calculations and are compared with the measured pressure data inside a chamber.

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STUDY ON NUMERICAL ANALYSIS AND TURBULENCE MODELS FOR ARC DISCHARGES IN HIGH-VOLTAGE INTERRUPTERS (초고압 차단부 아크방전 수치해석 및 난류모델에 관한 연구)

  • Lee, J.C.
    • Journal of computational fluids engineering
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    • v.15 no.3
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    • pp.9-15
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    • 2010
  • In this study, we calculated arc discharges and flow characteristics driven by arcs in a thermal puffer chamber, which is one of most outstanding high-voltage interrupters, for understanding the complex physics and the probability of thermal breakdown. The four main parts of arc model for this virtual-reality are radiation, PTFE ablation, Cu evaporation, and turbulence. Among these important parts the turbulence model can be critical to the reliability of computation results during the whole arcing history because the plasma flow is affected by high heat energy and mass momentum. Two turbulence models, the Prandtl's mixing length model and the standard $k-\varepsilon$ model, are applied for these calculations and are compared with pressure-rise inside chamber and arc voltage between the contacts as well as flow characteristics near current zero.

Vibro-acoustic Analysis for Predicting the Noise of HDD (하드디스크 드라이브 소음 예측을 위한 진동 음향 연계 해석)

  • 이상희;고상철;김준태;강성우;한윤식;황태연
    • Proceedings of the Korean Society for Noise and Vibration Engineering Conference
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    • 2001.05a
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    • pp.103-108
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    • 2001
  • The structure of hard disk drive(HDD) is excited by dynamic motion of a disk-spindle motor, and it makes sound noise. Therefore, the cover and the base of HDD should be designed to reduce noise and vibration induced by spindle motor. The prediction technique of sound pressure level(SPL) of a given structural shape enables us to design a cover and a base with much less vibration and noise. In this paper, we measured the force of disk-spindle motor and predicted SPL from HDD by computational simulation. To get a SPL of HDD by computational simulation, modal analysis and forced vibration analysis were performed with ANSYS, and sound radiation was computed using SYSNOISE. The calculated results were compared with experimental results and a good agreement was obtained. With this computer simulation procedure and design of experiment(DOE), optimal thickness of noise barrier and damper was calculated.

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Transfer Function of Structure-borne Noise to Underwater Radiated Noise (고체음의 수중방사소음 전달함수)

  • 김재승;김현실;김상렬
    • Proceedings of the Korean Society for Noise and Vibration Engineering Conference
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    • 2001.05a
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    • pp.138-142
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    • 2001
  • A comparison between theoretical and measured transfer function, which relates structure-borne noise source level to underwater radiated noise, of a naval ship is presented in this study. Transfer functions are obtained by dividing far field underwater noise by the value of structure borne noise source levels below machinery mounts. In prediction, statistical energy analysis of the whole ship structure is used to get vibration levels of wetted hull plates below water line. Then, far field radiated noise is calculated by summing up contributions from each plates using vibration levels and radiation efficiencies. And 1/3-octave band underwater sound pressure at the distance of 1 m away from the hull were measured to get experimental transfer functions. The two transfer functions are compared to show resonable agreements in spite of the subtle physical differences between each other.

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Noise Radiation Analysis of the Cooling Fan in a Heavy Equipment (중장비 팬의 엔진룸을 통한 소음방사 해석)

  • 정기훈;전완호;이덕주
    • Proceedings of the Korean Society for Noise and Vibration Engineering Conference
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    • 2001.05a
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    • pp.954-960
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    • 2001
  • Axial fans are widely used in heavy machines due to their ability to produce high cooling of engines. At the same time. the noise generated by these fans causes or serious problems. This work is concerned with the low noise technique of discrete. The prediction model. which allowed the calculation of acoustic pressure at the frequency and it's harmonics, has been developed by Farrasat and the Helmholtz-Kir. The newly developed Helmholtz-Kirchhoff BEM for thin body is used to calculate the sound field of the fan that is located in a engine room. To calculate the unsteady resultant force over blade. Time-Marching Free-Wake Method are used. The fan noise of fan sys unsymmetric engine-room is predicted. In this paper. the discussion is confined to and discrete noise of axial fan and front Part of engine room in heavy equipments.

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