• Proceedings of the Korea Society for Simulation Conference
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• 2000.04a
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• pp.113-118
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• 2000

웹 사용자의 수가 증가하면서 웹서버에 대한 접속 횟수가 급격히 증가하고 있다. 이것은 망의 부하와 서버의 부하를 증가시켜 웹 사용자가 원하는 정보의 전달을 지연시킨다. 프락시 서버는 이러한 문제를 해결하는 방법으로 서버 파일의 복사본을 클라이언트 가까이 위치시켜 망과 서버의 부하를 감소시킨다. 그러나 웹사용에서 프락시 서버의 도입효과에 대한 구체적인 연구결과가 없으므로 시스템 관리자가 프락시 서버의 도입여부를 결정하기가 힘들다. 본 논문에서는 웹사용 환경에서 프락시 서버의 성능을 평가할 수 있는 모델을 제시하고 시뮬레이션을 통해 이를 분석하고 평가한다.

• Korean Journal of Optics and Photonics
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• v.25 no.5
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• pp.245-253
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• 2014

We report a realistic field-performance simulation for a new MWIR camera. It is designed for early detection of missile plumes over a distance range of a few hundred kilometers. Both imaging and radiometric performance of the camera are studied by using real-scale integrated ray tracing, including targets, atmosphere, and background scene models. The simulation results demonstrate that the camera would satisfy the imaging and radiometric performance requirements for field operation.

• Journal of the Korean earth science society
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• v.39 no.1
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• pp.53-66
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• 2018

The information of surface reflectance ($R_{sfc}$) is important for the heat balance and the environmental/climate monitoring. The $R_{sfc}$ sensitivity to error-induced variables for the Geostationary Environment Monitoring Spectrometer (GEMS) retrieval from geostationary-orbit satellite observations at 300-500 nm was investigated, utilizing polar-orbit satellite data of the MODerate resolution Imaging Spectroradiometer (MODIS) and Ozone Mapping Instrument (OMI), and the radiative transfer model (RTM) experiment. The variables in this study can be cloud, Rayleigh-scattering, aerosol, ozone and surface type. The cloud detection in high-resolution MODIS pixels ($1km{\times}1km$) was compared with that in GEMS-scale pixels ($8km{\times}7km$). The GEMS detection was consistent (~79%) with the MODIS result. However, the detection probability in partially-cloudy (${\leq}40%$) GEMS pixels decreased due to other effects (i.e., aerosol and surface type). The Rayleigh-scattering effect in RGB images was noticeable over ocean, based on the RTM calculation. The reflectance at top of atmosphere ($R_{toa}$) increased with aerosol amounts in case of $R_{sfc}$<0.2, but decreased in $R_{sfc}{\geq}0.2$. The $R_{sfc}$ errors due to the aerosol increased with wavelength in the UV, but were constant or slightly decreased in the visible. The ozone absorption was most sensitive at 328 nm in the UV region (328-354 nm). The $R_{sfc}$ error was +0.1 because of negative total ozone anomaly (-100 DU) under the condition of $R_{sfc}=0.15$. This study can be useful to estimate $R_{sfc}$ uncertainties in the GEMS retrieval.

• Korean Journal of Remote Sensing
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• v.25 no.1
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• pp.45-59
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• 2009

This research presents the effect of Asian dust on the derived sea surface temperature (SST) from measurements of the Advanced Very High Resolution Radiometer (AVHRR) instrument flown onboard NOAA polar orbiting satellites. To analyze the effect, A VHRR infrared brightness temperature (TB) is estimated from simulated radiance calculated from radiative transfer model on various atmospheric conditions. Vertical profiles of temperature, pressure, and humidity from radiosonde observation are used to build up the East Asian atmospheric conditions in spring. Aerosol optical thickness (AOT) and size distribution are derived from skyradiation measurements to be used as inputs to the radiative transfer model. The simulation results show that single channel TB at window region is depressed under the Asian dust condition. The magnitude of depression is about 2K at nadir under moderate aerosol loading, but the magnitude reaches up to 4K at slant path. The dual channel difference (DCD) in spilt window region is also reduced under the Asian dust condition, but the reduction of DCD is much smaller than that shown in single channel TB simulation. Owing to the depression of TB, SST has cold bias. In addition, the effect of AOT on SST is amplified at large satellite zenith angle (SZA), resulting in high variance in derived SSTs. The SST depression due to the presence of Asian dust can be expressed as a linear function of AOT and SZA. On the basis of this relationship, the effect of Asian dust on the SST retrieval from the conventional daytime multi-channel SST algorithm can be derived as a function of AOT and SZA.

• Journal of Bio-Environment Control
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• v.22 no.2
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• pp.108-115
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• 2013

This study was conducted to suggest a model to calculate the overall heat transfer coefficient of single layer covering for various greenhouse conditions. There was a strong correlation between cover surface temperature and inside air temperature of greenhouse. The equations to calculate the convective and radiative heat transfer coefficients proposed by Kittas were best fitted for calculation of the overall heat transfer coefficient. Because the coefficient of linear regression between the calculated and measured cover surface temperature was founded to 0.98, the slope of the straight line is 1.009 and the intercept is 0.001, the calculation model of overall heat transfer coefficient proposed by this study is acceptable. The convective heat transfer between the inner cover surface and the inside air was greater than the radiative heat transfer, and the difference increased as the wind speed rose. The convective heat transfer between the outer cover surface and the outside air was less than the radiative heat transfer for the low wind speed, but greater than for the high wind speed. The outer cover convective heat flux increased proportion to the inner cover convective heat flux linearly. The overall heat transfer coefficient increased but the cover surface temperature decreased as the wind speed increased, and the regression function was founded to be logarithmic and power function, respectively.

• Korean Journal of Optics and Photonics
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• v.2 no.4
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• pp.203-208
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• 1991

We investigated the nonradiative energy transfer process from Rhodamine 6G to Malachite Green in ethylen glycol solvent using time correlated single photon counting system equipped with a modelocked Ar ' laser. The reduced concentration and critical transfer distance for various acceptor concentration were obtained by using a full-fitting analysis of the fluorescence decay curves. We found that Huber model is more suitable than Forster model and the influence of energy migration through the dipole-dipole interaction becomes more significant for the low acceptor concentrations relative to the donor concentration($5\times 10^4$mol/l).

• Journal of the Korean Society for Aeronautical & Space Sciences
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• v.31 no.6
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• pp.88-95
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• 2003

The weighted sum of gray gas model(WSGGM) is applied to arbitrary mixtures of CO$_2$ and H$_2$0 gases. To evaluate this model, the spectral and total intensities are obtained for two different problem types. One has uniform, parabolic and boundary layer type temperature profiles with uniform partial pressure, and the other has nonuniform partial pressure and temperature profile. The results obtained from the two different problem types show fairly good agreements with the results obtained by the statistical narrow band model(SNB model) which is regarded as the reference solutions. The WSGGM and its data base provided by this study can be used for analysis of radiative transfer by combustion gases with different thermal loadings and chemical compositions.

• 한국HCI학회:학술대회논문집
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• 2006.02a
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• pp.219-224
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• 2006

3 차원 입력 장치는 키보드나 마우스 같은 일반적인 입력 장치로는 받아 들이기 어려운 3 차원 입력을 사용자로부터 간편하고 직관적인 방법으로 받아들일 수 있다는 측면에서 활발히 연구 및 사용되고 있다. 또한 햅틱 장치는 가상 물체의 조작에 따른 시각적인 피드백 외에 가상 물체의 느낌을 피드백 힘을 통해 사용자에게 전달해 줌으로써 컴퓨터와 사용자간의 상호 작용에 큰 도움을 준다. 본 논문은 햅틱 피드백이 적용된 실시간 가변형 모델과 효과적인 3 차원 입력에 대한 기반 연구를 하고자 한다. 그리고 이에 대한 한 가지 사례로써 햅틱 장치를 이용한 가상 판화 시스템을 제작 한다. 가상 판화 시스템은 시각 처리 부분과 촉각 처리 부분, 그리고 사용자의 3 차원 입력을 돕는 인터페이스 부분으로 구성되어 있다. 시각 처리 부분은 3 차원 공간 상에서 사용자의 조각에 따른 판화 표면의 변형을 처리하며 촉각 처리 부분은 실제 판화를 제작할 때 느끼는 촉각을 햅틱 인터페이스를 이용하여 사용자에게 전달한다. 이를 위해 먼저 시각 처리 부분에서는 NURBS 기반의 자유 형상 변형 (FFD)기법을 이용하였는데 가상 조각도에 의한 물체 표면의 지역적인 변형을 구현하기 위해 조각도가 닿는 부분에 대해 기조 격자점 (control point)을 증가시켜 원하는 부분에 대한 지역적인 변화를 용이하도록 하였고 다음으로 촉각 처리 부분에서는 S-chain 모델을 이용하였는데 S-chain 모델을 객체 전체에 적용하지 않고 접촉이 일어날 경우 그 접촉점을 기준으로 S-chain 모델을 지역적으로 적용하는 방법을 고안하여 실제 구현에 이용하였다. 인터페이스 적인 측면에서 사용자의 3 차원 입력장치를 통한 인터렉션은 사용자로 하여금 보다 자유로운 입력을 허용하지만 이에 따른 깊이 지각 문제를 발생시킨다. 이러한 문제를 최소화 시키고 사용자의 깊이 지각을 강화시키기 위해 사용자에게 제공되는 시각적 자극을 변형시키고 다양한 정보를 제공하도록 하였다. 가상 판화 시스템은 가상 환경에서 사용자의 조작에 따른 다양한 결과물을 제작 및 출력해 볼 수 있도록 해준다. 또한 가상 환경에서 이러한 기반을 제공함으로써 가상 환경의 장점인 복사, 이동 및 영구 보존 특성을 동시에 얻을 수 있다. 본 논문은 이러한 작업을 위한 기반 기술로써 햅틱 및 가변형 모델, 3 차원 입력 장치에 대한 시각적 인터페이스에 대해 다루고 이 기반 기술을 바탕으로한 가상 판화 시스템의 구현에 대하여 논하고자 한다.

• The Bulletin of The Korean Astronomical Society
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• v.35 no.2
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• pp.69.1-69.1
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• 2010

장주기 Mira 변광성의 외피층에서 발생하는 SiO 메이저에 대해 non-local한 1차원 수치계산 결과를 처음으로 제시한다. 별의 유체역학적인 맥동모델에서 얻은 시간에 따른 별 주위 가스의 속도, 온도, 밀도 분포를 사용하여 계산하였다. 임의의 속도장을 갖는 구형 분자운에서의 복사전달문제를 풀었던 이전 연구에서 개발한 수치계산코드를 이용하였고, 특정 구간에서 급격한 변화를 겪는 물리량을 잘 반영할 수 있도록 수정하였다. 또한 계산에 사용되는 거대희소행렬을 압축희소행렬로 변환하여 메모리를 절약하였고 비선형방정식의 자코비안을 해석적으로 구하여 계산속도를 향상시켰다. v=1, J=1-0, J=2-1과 v=2, J=1-0 SiO 메이저의 공간분포, 상대세기 등에 대해 이전의 LVG 모델을 이용한 연구결과와 정성적으로 비교 논의한다.

• Korean Journal of Remote Sensing
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• v.15 no.2
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• pp.131-146
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• 1999

The satellite visible data have been successfully applied to study the ocean color. Another ocean color sensor, the Ocean Scanning Multi-spectral Imager (OSMI) on the Korea Multi-Purpose Satellite (KOMPSAT) will be launched in 1999. In order to understand the characteristics of future OSMI images, we have first discussed the simulation models and procedures in detail, and produced typical patterns of radiances at visible bands by using radiative transfer models. The various simulated images of full satellite passes and Korean local areas for different seasons, water types, and the satellite crossing equator time (CET) are presented to illustrate the distribution of each component of radiance (i.e., aerosol scattering, Rayleigh scattering, sun glitter, water-leaving radiance, and total radiance). A method to evaluate the image quality and availability is then developed by using the characteristics of image defined as the Complex Signal Noise Ratio (CSNR). Meanwhile, a series of CSNR images are generated from the simulated radiance components for different cases, which can be used to evaluate the quality and availability of OSMI images before the KOMPSAT will be placed in orbit. Finally, the quality and availability of OSMI images are quantitatively analyzed by the simulated CSNR image. It is hoped that the results would be useful to all scientists who are in charge of OSMI mission and to those who plan to use the data from OSMI.