• Journal of the Korean Society for Aeronautical & Space Sciences
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• v.40 no.9
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• pp.737-744
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• 2012

The finite volume method for radiation is applied for the analysis of radiative base heating by SE and PE of the aircraft exhaust plume. The exhaust plume is considered as an absorbing, emitting, and scattering medium, while the base plane is assumed to be cold and black. The radiative properties of non-gray gases are obtained through the WSGGM, and the particle is modelled as spheres. The present method is validated by comparing the results with those of the backward Monte-Carlo method and then the radiative base heating characteristics are analyzed by changing such various parameters as particle concentration, temperature, and scattering phase function. The results show that the radiative heat flux coming into the base plane decreases with altitude and distance, but it increases as the particle temperature increases. The forward scattering of particles increases PE while it decreases SE.

• Transactions of the Korean Society of Mechanical Engineers
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• v.16 no.5
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• pp.952-964
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• 1992

The interaction of natural convection and radiation heat transfer in a two dimensional square enclosure containing absorbing, emitting and linear anisotropically scattering gray medium is numerically analyzed. P-1 and P-3 approximation is introduced to calculate radiation heat transfer. The effects of scattering albedo, wall emissivity, scattering anisotropy, and optical thickness on the characteristics of the flow and temperature field and heat transfer are investigated. Temperature and velocity profiles depend a great deal on the scattering albedo, and the importance of this effect increases with decrease in albelo. Planck number is another important parameter in radiation heat transfer. The increase in scattering albedo increases convection heat transfer and decreases radiation heat transfer at hot wall. However, the increase in scattering albedo decreases both convection and radiation heat transfer at cold wall. The increase in optical thickness decreases radiation heat transfer. The scattering anisotropy has important effects on the radiation heat transfer only. The highly forward scattering leads to an increase of radiation heat transfer whereas the highly backward scattering leads to an decrease of radiation heat transfer. The effect of scattering anisotropy decreases when reducing the wall emissivity.

• The Proceeding of the Korean Institute of Electromagnetic Engineering and Science
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• v.2 no.4
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• pp.47-54
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• 1991

본 논문에서는 전자파 해석에 관련된 기존의 해석 기법들을 간략하게 비교, 검토하고 GTD / UTD를 기본으로하여 고주파 해석 기법에 관련된 몇가지 문제들을 다룬다. 전자파 해석이란 전자파의 복사(radiation), 산란(scattering) 및 결합(coupling)에 관련된 문제의 해석을의미 한다. 전자파 해석은 여러 목적을위해 응용되고 있으며 EMC / EMI문제의 분석 및 대책 수립에도 응용될 수 있다. EMC / EMI 문제의 근원은 전자파의 간섭(interference) 현상이다. Emitting source로부터 복사(radiation)되는 간섭파는 여러 경로를 통해서 receptor로 coupling된다. 일반적으로 emitter와 receptor사이에는 여러 복잡한 구조물이 산란체로 작용하고 있으므로, emitter와 receptor사이의 직접경로(direct path)를 통한 coupling과 함께 구조물에 의한 전자파의 반사 및 회절을 통한 간접경로(indirect path)의 coupling도 고려되어야 한다. 따라서 EMC / EMI문제는 자유공간(free space)상에 있는 antenna 사이의 송수신 문제보다 매우 복잡하고 정확한 couplin의 계 산에 적지않은 어려움이 있다. EMC / EMI대책수립은 일차적으로 coupling path의 차단을 통해서 가능하므로 전자 파의 coupling path의 분석과 전자파의 복사 및 산란 mechanism에 대한 해석이 필수적이다.

• Transactions of the Korean Society of Mechanical Engineers
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• v.15 no.1
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• pp.341-348
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• 1991

An efficient tool to deal with a multi-dimensional radiative heat transfer is in strong demand to analyze various thermal problems combined either with other modes of heat transfer or with combustion phenomena. The current study examined the discrete ordinates method (DOM) for a coupled radiative and conductive heat transfer in rectangular enclosures in which either nonscattering or scattering medium is present. The results were compared with the other benchmarked approximate solution. The efficiency and accuracy of the DOM were thus validated.

• Korean Journal of Remote Sensing
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• v.4 no.1
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• pp.17-29
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• 1988

본 연구에서는 지면의 표적물 및 하늘과 구름애서 산라되어 나오는 방향성 복사량을 효 율적으로 측정하고, 이들 산란광에 의한 Remote Sensing(원격탐사) 자료해석상의 영향을 조사 연 구하기 위해 만들어진 나선형식으로 회전하며 거의 전반구를 11초 이내에 주사하는 Sphere-Scanning Radiometer의 자료를 분석하는 데 필요한 software(S/W)들을 개발하였다. 개발 된 S/W 에는 개개의 측정자료가 기록될 순간에 측정기의 Field of View (FOV)에 의해 실제로 산란광이 집적된 지표면상의 부분을 시각적으로 나타내 주고 복사강도를 Grey Level로 나타낼 수 있는 도면표시 Algorithm과 FOV각의 크기에 따라 overlap부분의 면적을 계산하는 Algorithm 등이 포함되어 있다. 또한, 실험농장에서 본 radiometer로 측정한 자료를 이 S/W를 사용하여 분 석해 본 결과 밝혀진 몇 가지 방향성 복사량의 특성들을 간단히 소개 하였다.

• Journal of the Korean Society for Nondestructive Testing
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• v.21 no.6
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• pp.658-662
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• 2001

The classification of surface flaw types was performed on the basis of angular dependence of backscattered ultrasound. The copper line adhered on the surface, cower line filled in groove, pure groove and the normal edge were adopted as various surface flaw patterns of glass specimen. A backward longitudinal profile was formed probably by the longitudinal wane scattering at and near 1st critical angle. The wave trains at the peak angles of the backward radiation profiles showed different shapes according to the superposition ratio of scattered and leaky waves. The asymmetry of the backward radiation profile arose due to the scattering effect of flaw. The additive resonance effect of copper line appeared in the left side of the profile. The peak angles of both the longitudinal and radiation profiles were shifted toward small angle by the scattering effect.

• Bulletin of the Korean Space Science Society
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• 2011.04a
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• pp.31.3-31.3
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• 2011

달의 양방향 분포 함수는 Hapke에 의하여 처음 이론적 모델이 만들어졌고, 이후 Foote에 의해 아폴로 11호의 달 토양 샘플 10084의 양방향 분포 함수가 측정된 바 있다. 이 연구에서는 실제 크기의 달의 표면에 Hapke의 양방향 분포 함수를 적용하여 광학 모델은 개발하였다. 달 표면의 산란특성 중 반 무한하고 매끄러운 지면에 적용되는 후방산란 효과와 산란각에 따른 위상 함수가 적용된 모델이 사용되었으며, 위상함수로는 Henyey-Greenstein 함수가 사용되었다. 달의 3D 모델에 사용된 매개 변수는 Foote가 측정한 Hapke의 변수를 따랐으며 달의 단일 산란 알베도는 w=0.33, 핫스팟의 넓이는 h=0.017, Legendre 다항 계수인 b와 c에는 각각 b=0.308, c=0.425의 값이 사용되었다. 구성된 달의 양방향 분포 함수를 이용한 통합적 광선 추적 수치 모사 결과, 달 반사광의 복사 휘도율은 1차 근사 해석적 방법을 이용한 계산 결과의 복사 휘도율과 측정 오차 범위 이내의 오차를 보였다.

• Publications of The Korean Astronomical Society
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• v.24 no.1
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• pp.43-51
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• 2009

We present a Monte-Carlo simulation code, which solves the problem of dust-scattering in interstellar dust clouds with arbitrary light source distribution and dust density structure, and calculate the surface brightness distribution. The method is very flexible and can be applied to radiative transfer problems occurring not only in a single dust cloud, but also in extragalactic dust environment. We compare, for performance test, the result of Monte-Carlo simulation with the well-known analytic approximation for a spherically symmetric homogeneous cloud. We find that the Code approximation gives a very accurate result.

• International Union of Geodesy and Geophysics Korean Journal of Geophysical Research
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• v.21 no.1
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• pp.31-46
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• 1993

A radiative transfer model with two-stream/delta-Eddington approximation has been developed to calculate the vertical distributions of atmospheric heating rates and radiative fluxes. The performance of the model has been evaluated by comparison with the results of ICRCCM (Intercomparison of radiative codes in climate models). It has been demonstrated that the presented model has a capability to calculate the solar radiation not only accurately but also economically. The characteristics of ultraviolet-B radiation (UV-B; 280-320nm) are examined by comparison of relation between the flux at the top of atmosphere and that at the surface. The relation of UV-B is quadratic due to the strong ozone absorption in this band. Also, the dependence of the UV-B radiation on the stratospheric ozone depletion and stratospheric aerosol haze due to volcanic eruption on the stratospheric ozone depletion and stratospheric aerosol haze due to volcanic eruption has been tested with various solar zenith angles. The surface UV-B increases as the solar zenith angle increases. The existence of stratospheric aerosols causes an increase in the planetary albedo due to the aerosols' backscattering. The planetary albedo with aerosol's effect has been increases as the solar zenith angle is not sensitive. It may be caused by the fact that the aerosols' scattering effect becomes saturated with the relatively long path length in a large solar zenith angle. Finally, the regional impact of stratospheric aerosols due to volcanic eruption on the intensity of UV-B radiation at the surface has been estimated. A direct effect is that the flux is diminished at the low latitudes, while it is enhanced in the high latitudes by the aerosols' photon trap or twilight effect. In the high latitudes, both aerosols' scattering and ozone absorption have strong and opposite impacts to the surface UV-B radiation is located at the mid-latitudes during spring season in both hemispheres.

• Korean Journal of Optics and Photonics
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• v.31 no.2
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• pp.59-70
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• 2020

We discuss a modified numerical model based on the Monte Carlo radiative transfer (MCRT) method, i.e., the MCRT matrix method, for the analysis of atmospheric scattering effects in three-dimensional flash LIDAR systems. Based on the MCRT method, the radiative transfer function for a LIDAR signal is constructed in a form of a matrix, which corresponds to the characteristic response. Exploiting the superposition and convolution of the characteristic response matrices under the paraxial approximation, an extended computer simulation model of an overall flash LIDAR system is developed. The MCRT matrix method substantially reduces the number of tracking signals, which may grow excessively in the case of conventional Monte Carlo methods. Consequently, it can readily yield fast acquisition of the signal response under various scattering conditions and LIDAR-system configurations. Using the computational model based on the MCRT matrix method, we carry out numerical simulations of a three-dimensional flash LIDAR system operating under different atmospheric conditions, varying the scattering coefficient in terms of visible distance. We numerically analyze various phenomena caused by scattering effects in this system, such as degradation of the signal-to-noise ratio, glitches, and spatiotemporal spread and time delay of the LIDAR signals. The MCRT matrix method is expected to be very effective in analyzing a variety of LIDAR systems, including flash LIDAR systems for autonomous driving.