• 대한기계학회논문집B
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• 제20권11호
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• pp.3598-3606
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• 1996

The finite volume method for radiation is applied to investigate a radiative heating of rocket base plane due to searchlight and plume emissions. Exhaust plume is assumed to absorb, emit and scatter the radiant energy isotropically as well as anisotropically, while the medium between plume boundary and base plane is cold and nonparticipating. Scattering phase function is modelled by a finite series of Legendre polynomials. After validating benchmark solution by comparison with that of previous works obtained by the Monte-Carlo method, further investigations have been done by changing such various parameters as plume cone angle, scattering albedo, scattering phase function, optical radius and nozzle exit temperature. The results show that the base plane is predominantly heated by the plume emission rather than the searchlight emission when the nozzle exit temperature is the same as that of plume.

• Ocean and Polar Research
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• 제31권4호
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• pp.297-304
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• 2009

We investigated the response of the westerly winds over the Southern Ocean (SO) to glacial boundary conditions for the Last Glacial Maximum using the CCM3 atmospheric general circulation model. In response to glacial boundary conditions, the zonally averaged maximum SO westerly winds weakened 20-35% and were displaced toward the equator by 3-4 degrees. This weakening of the SO westerly winds arose from a substantial increase in mean sea level pressure (MSLP) in the southern part of the SO around Antarctica relative to the northern part. The increase in MSLP around Antarctica is associated with a marked temperature reduction caused by an increase in sea ice cover and ice albedo feedback during the glacial time. The weakened westerly winds in the SO and their equator-ward displacement might play a role in reducing the atmospheric $CO_2$ concentration by reducing upwelling of the carbon rich deep water during the glacial time.

• 한국수자원학회:학술대회논문집
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• 한국수자원학회 2011년도 학술발표회
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• pp.349-352
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• 2011

토양수분은 지표와 대기에서 물과 에너지를 교환하는 중요한 수문기상 인자임에도 불구하고 토양수분에 대한 중요성이 부족한 실정이다. 최근에는 위성기술의 발달로 Aqua위성에 탑재된 Advanced Microwave Scanning Radiometer E (AMSR-E)를 이용하여 토양수분을 측정하고 있다. 이는 토양수분을 측정하고 있는 가장 유용한 기기로서 25km의 낮은 공간 해상도를 가지고 있어 토양수분의 변화를 나타내는데 한계점을 가지고 있다. 본 연구에서는 AMSR-E의 공간 해상도를 높이고자 비교적 높은 해상도를 (1km) 가지고 있는 Moderate Resolution Imaging Spectroradiometer (MODIS)를 연동하였으며, MODIS의 산출물 중 Albedo, LST, NDVI 인자를 이용하였다. 이를 바탕으로 1km의 고해상도 일 별 토양수분 지도를 작성하였으며, 이 지도를 각각 관측 토양수분과 비교 검증하였다. 향후 일별 고해상도 토양수분 지도를 작성하면 우리나라에 대한 토양수분 데이터베이스를 구축해 나갈 수 있을 것이다.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 1998년도 Proceedings of International Symposium on Remote Sensing
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• pp.103-109
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• 1998

A technique on atmospheric correction algorithm for a single band (0.76-0.90 $\mu$m) reflective of Landsat TM imagery has been developed using a radiation transfer model simulation. It proceeds in two steps: First, calculation of the surface reflectance of each pixel based on precomputed planetary albedo functions for actual atmospheres(e. g. radiosonde) and two kinds of atmospheric visibility states. Second, approximate correction of the adjacency pixel effect by taking into account the average reflectance in an 7 $\times$ 7 pixel neighbourhood and using appropriate land cover classification in reflectance. The correction functions are provided by MODTRAN model.

• 천문학회보
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• 제36권2호
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• pp.103.2-103.2
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• 2011

We measure the degree of polarization of the lunar regolith to map the distributions of the age and the particle size. We use a 12cm refracting telescope with a 2k-square pixel color CCD (R band) and a polarization filter. The angular resolution obtained is 3.02 km/pixel. Our goal is to obtain a map of the lunar particle size distribution on the lunar regolith and then that of the age distribution. Polarization of the light scattered by lunar surface contains information on their mean particle size. The mean particle size of the lunar surface has been decreased by continued micro-meteoroid impact over a long period. One can estimate the age of the lunar surface if the mean particle size is known. Particle sizes can be measured through observations of polarization because the mean particle size is related to the maximum polarization and albedo. The age and the particle size of the lunar regolith can give vital information for the future lunar exploration.

• Journal of the Optical Society of Korea
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• 제19권5호
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• pp.444-448
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• 2015

We describe the radiative transfer of a Gaussian beam in a water medium using the Monte Carlo method offering basic propagation behaviors. The simulation shows how the energy of the initial Gaussian beam is redistributed as it propagates in coastal water, and also depicts the dependence of the propagation behavior on inherent optical properties of the ocean water such as the single scattering albedo as well as on laser beam parameters, e.g. the M squared. Our results may widen the applicability of LIDARs by providing a couple of design considerations for a bathymetric LIDAR.

• Journal of Astronomy and Space Sciences
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• 제9권1호
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• pp.30-40
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• 1992

세 종류의 식쌍성에 대한 반사 효과를 Wilson과 Devinney의 모델과 Russell과 Merrill의 모델로 분석하였다. 반사 효과를 Wilson과 Devinney의 광도 곡선 프로그램을 이용하여 이론적인 광도 곡선에 여러가지 유형별로 나타내었다. 그후 반사효과가 나타난 이론적인 광도 곡선을 Russell과 Merrill의 방법으로 근접 효과를 보정하여 두 모델을 비교 분석하였다. 두 별의 온도 차이와 반사도의 차이가 작은 경우에만 반사 효과에 관한한 두 모델이 일치함을 보였다.

• 천문학회보
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• 제41권1호
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• pp.81.4-82
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• 2016

Recent analysis on asteroidal thermophysical property revealed that there is a tendency that their thermal inertia decrease with their sizes at least for main belt asteroids. However, little is known about the thermal properties of comet-like bodies. In this work we utilized a simple thermophysical model to calculate the thermal inertia of a bare nucleus of comet P/2006 HR30 (Siding Spring) and an asteroid in comet-like orbit 4015 Wilson-Harrington from AKARI observation data. It is also shown that the determination of their thermal inertia is very sensitive to their spin vector, while the diameter is rather easy to be constrained to a certain range by combining multi-wavelength observational data. Thus, we set diameter and hence the geometric albedo as fixed parameters, and inferred the spin vector and thermal inertia of the targets. Further detailed analyses on these cometary bodies will shed light on our understanding of the detailed surfacial characteristics of them.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2007년도 심포지엄 논문집 정보 및 제어부문
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• pp.165-166
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• 2007

특수 분장을 이용하여 매우 정교하게 제작된 가면을 쓴 얼굴 위변조의 경우 일반적인 밝기 영상으로는 검출이 용이하지 않다. 최근의 획기적인 특수 분장 기술 발전을 고려할 때 성공적인 얼굴 인식시스템 개발을 위해 가면을 쓴 얼굴 위변조 검출 연구는 매우 중요하다. 본 연구에서는 물질의 재질에 따른 반사율의 차이를 기반으로 가면을 착용하는 얼굴 위변조를 검출하는 방법을 제안한다. 우선 알비도(albedo)에 착안하여 여러 파장대의 조명에 대해 실험하였다. 실제 얼굴 인식 시스템의 적용 환경을 고려할 때 알비도를 단순히 빛의 반사량으로 간략화 할 수 있음을 보였고, 실험결과 850nm 적외선 조명이 적합하다는 결론을 얻었다.

• 한국태양에너지학회 논문집
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• 제22권3호
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• pp.21-30
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• 2002

Images taken by geostationary satellite may be used to estimate solar irradiance fluxes at earth's surface. It is based on the empirical correlation between a satellite derived cloud index and the irradiance at the ground. For the validation. estimated solar radiation fluxes are compared with observed solar radiation fluxes at 16 sites over the Korean peninsular from January 1982 to December 2000. Estimated solar radiation fluxes show reliable results for estimating the global radiation with average deviation of -5.6 to +2.8% from the measured values and the yearly averaged horizontal global insolation of Korean peninsula was turned out to be $3.038kcal/m^2.day$.