• 동력기계공학회지
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• 제3권3호
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• pp.60-69
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• 1999

The noise and vibration sources of rotary compressor for room air-conditioner are pressure pulsation of compression process, cavity resonance of inner space, structural radiation noise of shell and impact noise of discharge valve. Among them, pressure pulsation is very important noise and vibration source. Because it transferred various kinds of noise and vibration like as mentioned above. In this reason, muffler and resonator are used in order to absorb and remove these noises. But an analytical prediction using acoustic analysis does not coincident with the experimental result. The difference between analysis and actual state is due to the assumption of analysis. This paper covered with new concept of muffler design based on the turbulence kinetic energy of flow by using CFD. From this analysis, it is possible to decide the best position of discharge port of muffler. Therefore $2{\sim}3dB$ noise reduction effect is acquired in rotary compressor of 5000 BTU grade. Also new approach of resonator design is suggested. From this study, the characteristics of resonator and surge hole (a kind of resonator without pipe length) are identified. The former is useful for pure tone noise (narrow frequency band), and the latter is effective for broad frequency band. This paper shows that it is very available to use 3 dimensional analysis of resonator in order to predict more exact tuning frequency. The result is proved by a lot of experiments. From combination of fluid analysis and acoustic analysis, up stream position is effective location of resonator concerning turbulence motion of fluid.

• 한국통신학회논문지
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• 제25권5A호
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• pp.696-701
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• 2000

마이크로파 통신하는 여러 응용 장치들에서 송, 수신 장치들 사이의 전파경로에 따라 수신아테나에 수신되는 전압이 달라진다. 교통제어를 목적으로 하는 ETC(Electronic Toll Collection)시스템은 고속도로의 자동요금징수시스템으로 노변장치(Beacon)와 차량 탑재장치(On Board Unit) 등으로 구성되며 이 장치들 사이의 전파경로는 다중 경로이다. 따라서 수신안테나의 전압은 거리에 따라서 그 키기가 크게 감소되는 페이딩 현상이 발생된다. 본 연구에서는 모델화된 ETC 시스템의 전파 다중경로를 사용하여 주파수변화에 따른 효과, 환경 변화, 편파, 및 안테나 방사패턴 등의 영향들을 고려하여 페이딩 현성이 최소로 되는 조건을 구하였다. 분석결과, 강우 시 수직 편파의 경우 페이딩 효과가 크게 감소되며 일반적으로 원형 편파일 경우 페이딩 효과가 비교적 적었다. 큰 방향성의 안테나를 사용하면 근거리에서 페이딩 효과가 감소하였다. 공간과 주파수 다이버시티 기술을 적용하면 페이딩에 의한 영향을 감소시킬 수 있었다. 이러한 결과들을 차량 탑재장치에서 수신된 전압의 크기(dB)와 노변장치와 차량 사이거리로 도시하였으며 실험에 의한 결\ulcorner와 비교 검토하였다.

• 한국화재소방학회논문지
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• 제21권1호
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• pp.90-97
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• 2007

주거공간에 사용되는 벽지의 화재 위험성을 평가하기 위하여 몇 종류의 벽지 시료에 대한 연소특성과 연소가스의 독성을 분석하였다. 본 연구에서 재의 잔량은 고온의 전기로를 이용하여 측정하였으며 TGA를 이용하여 열적 특성을 분석하였다. 연소시간과 연기농도의 측정은 콘히터와 가스분석계를 사용하였고 연기밀도는 ASTM E662의 장치를 이용하였다. 실험결과 실크벽지는 다른 벽지에 비해 낮은 온도에서 열분해가 시작되었는데 이는 실크벽지가 낮은 열유속(heat flux)에서도 착화될 수 있으므로 다른 벽지보다 화재 위험성이 높다. 실크벽지의 복사 열유속에 의한 착화시간은 다른 시료들에 비해 짧아서 화재 시 피난 시간이 짧아져야 하며 비닐이 코팅된 실크벽지 연소 시 일산화탄소의 발생 농도가 가장 높아서 독성의 위험이 높을 것으로 보인다. 실크벽지와 실크방염 벽지의 비닐 코팅으로 연기밀도가 높게 나타났다.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 1998년도 Proceedings of International Symposium on Remote Sensing
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• pp.301-306
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• 1998

Korea Aerospace Research Institute (KARI) is developing a Korea Multi-Purpose Satellite I (KOMPSAT-I) which accommodates Electro-Optical Camera (EOC), Ocean Scanning Multi-spectral Imager (OSMI), and Space Physics Sensor (SPS). The satellite has the weight of about 500kg and will be operated on the 10:50 AM sun-synchronized orbit with the altitude of 685 km. The satellite will be launched in 1999 and its lifetime is expected to be over 3 years. The main mission of EOC is the cartography to provide the images from a remote earth view for the production of 1/25000-scale maps of KOREA. EOC collects 510 ~ 730 nm panchromatic imagery with the ground sample distance(GSD) of 6.6 m and the swath width of 17 km by push broom scanning. EOC also can scan $\pm$45 degree across the ground track using body pointing method. The primary mission of OSMI is worldwide ocean color monitoring for the study of biological oceanography. It will generate 6 band ocean color images with 800 km swath width and 1km GSD by whiskbroom scanning. OSMI is designed to provide on-orbit spectral band selectability in the spectral range from 400 nm to 900 nm through ground command. This flexibility in band selection can be used for various applications and will provide research opportunities to support the next generation sensor design. SPS consists of High Energy Particle Detector (HEPD) and ionosphere Measurement Sensor (IMS). HEPD has missions to characterize the low altitude high-energy Particle environment and to study the effects of radiation environment on microelectronics. IMS measures densities and temperature of electrons in the ionosphere and monitors the ionospheric irregularities at the KOMPSAT orbit.

• 한국방사선학회논문지
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• 제9권3호
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• pp.125-130
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• 2015

방사선은 의료 분야 뿐 아니라 공업 분야, 농업 및 식품생명 분야 등에 이용되고, 소규모 방사선이용시설의 운영이 증가하고 있는 상황이다. 이에 소규모 방사선이용시설의 해체에 대한 관심을 가질 필요성이 있고, 시설 해체 시 발생될 문제점에 대해 예측해 볼 필요성이 있다. 원자력발전소 등의 대형방사선이용시설의 해체에 대한 대비는 진행되고 있으나, 상대적으로 위험성이 적은 소규모 방사선이용시설의 해체에 대해서는 대비가 부족한 상황이다. 사이클로트론의 방사화나 브라질 고이아니아의 방사성물질 누출사고를 생각해보면 소규모 방사선이용시설의 사고 시 그 영향은 대형 방사선이용시설에 비해 작지 않다. 이에 따라 본 연구에서는 국내에 비해 상대적으로 소규모 방사선이용시설 해체 사례가 많은 국외의 사례 중 국내에서 많이 가동되고 있는 사이클로트론, 방사선치료시설 등 시설별 특징에 대해 분석하였다. 또한, 소규모 방사선이용시설 해체 시 각 시설별 또는 공통적인 문제점으로는 시설과 선원의 재사용, 공간 부족, 이해 당사자의 개입, 대중의 방사선 노출이 나타났다. 이를 바탕으로 향후 소규모 방사선이용시설 해체 시 문제점을 해결할 수 있는 방안을 마련할 때 도움이 될 것으로 사료된다.

• 천문학회지
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• 제31권2호
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• pp.161-171
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• 1998

We have mapped about 1.5 square degree regions of Lynds 1299, a well isolated dark cloud in the Outer Galaxy (l = $122^{\circ}$, b = $-7^{\circ}$), in the J = 1- 0 transition of $^{12}CO$ and $^{13}CO$ with the 13.7 m radio telescope at Taeduk Radio Astronomy Observatory (TRAO). We found that there are two velocity components in the molecular emission, at $V_{LSR} = -52 km S^{-1}$ (Cloud A) and -8.8 km $s^{-1}$ (Cloud B), respectively. We have derived physical parameters of two molecular clouds and discussed three different mass estimate techniques. We found that there are large discrepancies between the virial and LTE mass estimates for both clouds. The large virial mass estimate reflects the fact that both are not gravitationally bound. We adopt the mass of $5.6 {\times}10^3 \;M{\bigodot}$ for Cloud A and $1.2{\times}10^3 \;M{\bigodot}$) for Cloud B using conversion factor. Cloud A is found to be associated with a localized star forming site, and its morphology is well matching with that of far-infrared (FIR) dust emission. It shows a clear ring structure with an obvious velocity gradient. We suggest that it may be a remnant cloud from a past episode of massive star formation. Cloud B is found to be unrelated to Cloud A (d = 800 pc) and has no specific velocity structure. The average dust color temperature of the uncontaminated portion of Cloud A is estimated to be 24$\~$27.4 K. The low dust temperature may imply that there is no additional internal heating source within the cloud. The heating of the cloud is probably dominated by the interstellar radiation field except the region directly associated with the new-born B5 star. Overall, the dust properties of Cloud A are similar to those of normal dark cloud even though it does have star forming activity.

• 천문학회지
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• 제29권2호
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• pp.223-243
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• 1996

We have constructed a line-by-line model of the A-X system of CO in order to analyze the CO bands appearing in the UV spectra of comets. The model includes electronic, rotational, vibrational transitions, excitations by solar UV radiation, and effects of neutral and electron collisions. The major bands of the A-X system occur in the $1200 - 1800{\AA}$ range where the temporal variation of solar irradiation is significant. The solar spectrum in this spectral range shows many emission lines, which cause a significant Swings effect. We derived fluorescence efficiencies of the bands as functions of heliocentric velocity and cometocentric distance using a high resolution spectrum of the sun. We compared our model with a spectrum of comet P/Halley obtained with the IUE, and estimated that the UV Swings effects are less than 20 fluorescence efficiencies for the most bands of the A-X system. We discuss the temporal variation of solar UV irradiation and its effects on the fluorescence efficiencies. The study of the A-X system also requites knowledge of vibrational and rotational fluorescent processes in the infrared and radio regions because the majority of CO molecules in the coma is in the ground rotational states. The solar infrared spectrum near 5 microns, where the fundamental band of CO occurs, contains strong absorption lines of the fundamental band and hot bands of CO and its isotopes. We derived fluorescence efficiencies of the infrared band as functions of heliocentric velocity and cometrocentric distance. The solar absorption lines near 5 microns cause a 20 reduction of the g-factor of the fundamental band at heliocentric velocities close to 0 km/sec. We discuss the effects of neutral and electron collisions on the fluorescence efficiencies of the infrared and UV bands.

• 한국전자파학회논문지
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• 제18권2호
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• pp.143-150
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• 2007

본 논문에서는 400 MHz ISM 대역에서 사용 가능한 마이크로스트립 선로로 급전되는 개방 종단을 갖는 미앤더 슬롯 안테나를 새롭게 제안하였다. 본 논문에서 제안된 슬롯 안테나와 기존의 슬롯 안테나의 주된 차이점은 좁은 범위로 제약된 공간에서 기존의 슬롯 안테나를 소형화하기 위하여 개방 종단을 도입했다는 점이다. 본 논문이 제안하는 안테나의 타당성을 검토하기 위하여 공진 주파수 및 방사 패턴의 결과를 시뮬레이션해 보았고, 그 결과들을 실험적으로 측정해 보았다. 본 논문이 제안하는 안테나의 공진 주파수 및 방사 패턴의 시뮬레이션 결과와 측정 결과가 잘 일치함을 알 수 있었다.

• International Journal of Advanced Culture Technology
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• 제3권1호
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• pp.129-137
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• 2015

The study of photocatalysis of nano titanium dioxideon the cotton fabrics have been investigatedthrough self-cleaning properties. The mini-emulsion technique was employed to prepare the encapsulation of titanium dioxide nano particles in polystyrene beads prior used. The mini-emulsion was coated on the cotton fabrics using Pad-dry method.The loading amount of TiO2particles into the mini-emulsion were various from 1%wt to 40%wt. The particles sizes of the TiO2-encapsulated polystyrene mini-emulsion were investigated by dynamic light scattering. It was noticed that the particle size of the mini-emulsion was in the range of 100- 200 nm. The morphology of treated cotton fabrics were investigated using scanning electron microscopy. The crystal structure of TiO2-encapsulated PS mini emulsion which coated on cotton fabrics were examined by X-ray diffraction spectroscopy. In order to investigate the photocatalytic activities of TiO2 through the selfcleaning characteristics of the cotton fabrics, colorant stains were created on the samples. Coffee stains were used as colorant organic stains. The result shown that the coffee stained on the cotton fabrics significantly showed the improving of the self-cleaning properties under UV radiation.

• Nuclear Engineering and Technology
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• 제42권5호
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• pp.568-575
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• 2010

Flow Accelerated Corrosion is an active degradation mechanism of CANDU feeder. The tight bend downstream to Gray loc weld connection, close to reactor face, suffers significant wall thinning by FAC. Extensive in-service inspection of feeder wall thinning is very difficult because of the intense radiation field, complex geometry, and space restrictions. Development of a knowledge-based inspection program is important in order to guarantee that adequate wall thickness is maintained throughout the whole life of feeder. Research results and plant experiences are reviewed, and the plant inspection databases from Wolsong Units One to Four are analyzed in order to support developing such a knowledge-based inspection program. The initial thickness before wall thinning is highly non-uniform because of bending during manufacturing stage, and the thinning rate is non-uniform because of the mass transfer coefficient distributed non-uniformly depending on local hydraulics. It is obvious that the knowledge-based feeder inspection program should focus on both fastest thinning locations and thinnest locations. The feeder wall thinning rate is found to be correlated proportionately with QV of each channel. A statistical model is proposed to assess the remaining life of each feeder using the QV correlation and the measured thicknesses. W-1 feeder suffered significant thinning so that the shortest remaining life barely exceeded one year at the end of operation before replacement. W-2 feeder showed far slower thinning than W-1 feeder despite the faster coolant flow. It is believed that slower thinning in W-2 is because of higher chromium content in the carbon steel feeder material. The average Cr content of W-2 feeder is 0.051%, while that value is 0.02% for W-1 feeder. It is to be noted that FAC is reduced substantially even though the Cr content of W-2 feeder is still very low.