• Journal of the Korean earth science society
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• v.31 no.4
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• pp.348-353
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• 2010

The scattered light of solar radiance near the infrared ray area was observed to measure $H_2O$ and $O_2$ absorption lines. The changes of $H_2O$ and $O_2$ equivalent width were calculated on the basis of the measurement. $O_2$ equivalent width showed negative correlation with the amount of solar radiance; $O_2$ equivalent width had a tendency to diminish as the amount of the solar radiance increased and to increase as the amount of the solar radiance decreased. On the other hand, $H_2O$ equivalent width showed the positive correlation with the amount of solar radiance. Especially it was noted that the sum of equivalent width of absorption lines created by $H_2O$ and $O_2$ in a day was fairly constant. It is implied that the constant equivalent width is caused by the complementary development of photodissociation and recombination in $O_2$ and $H_2O$.

• Transactions of the Korean Society of Mechanical Engineers
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• v.14 no.6
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• pp.1639-1644
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• 1990

Effects of radiation on the wall-friction and heat transfer in the convergent and divergent nozzle of a rocket motor are investigated in the present paper. Radiative heat transfer cools down the core gas, and the decrease in the gas temperature reduces the convective heat transfer on the wall. Radiation heat transfer is estimated by using mean-beam-length approach and core flow is assumed to be one-dimensional isentropic. The compressible thermal boundary layer is solved by a finite difference method. The Cebeci-Smith eddy viscosity model is adopted for the present study. Convective heat transfer is reduced at the throat of the nozzle and is almost compensated with an increase in radiative transfer. In the sequel total heat transfer rate is slightly reduced. However, radiation heat transfer is dominant in the converging part of the nozzle.

• Journal of the Korean Society for Aeronautical & Space Sciences
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• v.43 no.12
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• pp.1079-1088
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• 2015

Parallelism and performance enhancement of calculating view factors in KSDS developed by KARI is introduced in this paper. View factor is an essential parameters of radiation thermal analysis for a spacecraft, and the amount of computation of them is not negligible. Especially, independent integration of view factors at each position of the orbit because the relative displace between solar panel and main body of a satellite varies with the position on the orbit. This paper introduces a range of parallelism of computing view factor and their performance, detection of obstructions by spatial search algorithm based on KD-Tree, and the reduction of the calculation of view factors of a satellite with relative motion between solar panel and main body, called updating fractional view factor matrix, for satellite thermal analysis.

• Journal of the Korean earth science society
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• v.38 no.2
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• pp.129-140
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• 2017

Global solar radiation was calculated in this research using ground-base measurement data, meteorological satellite data, and GWNU (Gangneung-Wonju National University) solar radiation model. We also analyzed the accuracy of the GWNU model by comparing the observed solar radiation according to the total cloud cover. Our research was based on the global solar radiation of the GWNU radiation site in 2012, observation data such as temperature and pressure, humidity, aerosol, total ozone amount data from the Ozone Monitoring Instrument (OMI) sensor, and Skyview data used for evaluation of cloud mask and total cloud cover. On a clear day when the total cloud cover was 0 tenth, the calculated global solar radiations using the GWNU model had a high correlation coefficient of 0.98 compared with the observed solar radiation, but root mean square error (RMSE) was relatively high, i.e., $36.62Wm^{-2}$. The Skyview equipment was unable to determine the meteorological condition such as thin clouds, mist, and haze. On a cloudy day, regression equations were used for the radiation model to correct the effect of clouds. The correlation coefficient was 0.92, but the RMSE was high, i.e., $99.50Wm^{-2}$. For more accurate analysis, additional analysis of various elements including shielding of the direct radiation component and cloud optical thickness is required. The results of this study can be useful in the area where the global solar radiation is not observed by calculating the global solar radiation per minute or time.

• The Bulletin of The Korean Astronomical Society
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• v.35 no.1
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• pp.67.2-67.2
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• 2010

구형 분자운에서의 복사전달문제를 탈출확률방법에 기초하여 non-local method로 풀었다. 매질을 여러 개의 구간으로 나누고 각 구간에서 물리량이 일정하다고 가정하여 복사전달식을 전개하였고 뉴턴방법을 채택하여 수렴속도를 빠르게 하였다. 이번 연구에서는 분자운 내부의 속도구배가 작든 크든 상관없이 복사전달식을 풀 수 있도록 수치코드를 개발하였다. 우리의 계산 결과는 속도구배가 큰 경우에는 LVG방법을 사용한 결과와 일치하고, 분자운이 정적인 경우에도 이전 연구의 결과와 일치한다. 앞으로 이 방법에 line-overlap과 saturation효과를 추가하여 만기형 별에서의 SiO메이저 연구에 활용할 계획이다.

• Transactions of the Korean Society of Mechanical Engineers
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• v.16 no.5
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• pp.983-991
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• 1992

This investigation is carried out numerically for the two dimensional natural convection and surface radiation heat transfer in a square enclosure. The bottom and top walls are isothermal at hot and cold temperatures respectively whereas the left and right side walls are adiabatic except a transparent window on the right side partially. The exchange of radiant energy is obtained by the net radiation method and the shape factor by the crossed string method. The changes in temperature and Nusselt number distributions of the walls due to the surface radiation and insolation are also investigated.

• Korean Journal of Remote Sensing
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• v.24 no.2
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• pp.213-222
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• 2008

Although hyperspectral sensing data have shown great potential to derive various surface information that is not usually available from conventional multispectral image, the acquisition of proper hyperspectral image data are often limited. To use ground-based hyperspectral camera image for remote sensing studies, radiometric calibration should be prerequisite. The objective of this study is to develop radiometric calibration procedure to convert image digital number (DN) value to surface reflectance for the 120 bands ground-based hyperspectral camera. Hyperspectral image and spectral measurements were simultaneously obtained from the experimental target that includes 22 different surface materials of diverse spectral characteristics at wavelength range between 400 to 900 nm. Calibration coefficients to convert image DN value to at-sensor radiance were initially derived from the regression equations between the sample image and spectral measurements using ASD spectroradiometer. Assuming that there is no atmospheric effects when the image acquisition and spectral measurements were made at very close distance in ground, we were also able to derive calibration coefficients that directly transform DN value to surface reflectance. However, these coefficients for deriving reflectance values should not be applied when the camera is used for aerial image that contains significant effect from atmosphere and further atmospheric correction procedure is required in such case.

• Proceedings of the Korea Society for Energy Engineering kosee Conference
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• 1993.05a
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• pp.112-115
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• 1993

복사관을 이용한 가열방식은 복사관내에서 연료를 연소시킬 때 얻어지는 열이 관을 통하여 복사됨으로서 피가열물을 가열하는 방식으로서 분위기제어가 필요한 열처리로 등에 널리 사용되고 있다. 본 연구에서는 연속 소둔설비용으로서 저 NOx화 및 복사관의 표면온도를 상대적으로 균일하게 가열시키는 특성을 가진 버너의 개발을 위한 것으로서 실기규모 연소실험을 수행하였다. 연소실험은 기존버너 및 편심노즐버너에 대해서 수행하였으며 특히 개발실험용 버너의 실험과정에서는 새로 고안된 버너의 성능평가로부터 최적화에 이르기까지의 종합적인 실험을 수행하였다. 개발실험에 의해 편심노즐을 특징으로 하는 2단연소식 복사관버너를 고안하였으며 시제품버너의 성능실험결과 기존버너보다 NOx방출량에서 30%의 감소를 보여주었으며 복사관에서의 온도의 균일성이 향상되었음을 확인하였다.

• Proceedings of the Korea Institute of Fire Science and Engineering Conference
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• 2012.04a
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• pp.206-209
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• 2012

산불에 영향을 미치는 인자는 일반적으로 산림 연료와 기상 그리고 지형인자로 구분할 수 있다. 이중 지형인자는 경사와 사면의 방향 그리고 해발고, 사면의 길이 등 여러 조건들이 복합적으로 이루어진 산의 형세를 이룬다. 지형 조건 중 경사는 산불 발생 후 확산속도에 영향을 주며 사면의 방향은 태양복사에너지 일사량에 따른 연료의 건조와 연료의 온도 등에 영향을 줌으로써 산불의 발생과 확산에 영향을 준다. 특히 산불이 시작되는 이른 봄철에는 강설 후 사면향에 따라 적설지역과 눈이 녹아 건조한 지역이 사면의 향에 따라 큰 차이를 나타내고 있으며 이로 인해 산불위험 예보시에도 사면향에 따른 산불발생위험을 달리 적용해야 할 필요성이 있다. 이에 본 연구에서는 사면의 방향에 따른 산불위험성을 평가하기 위해 먼저 태양복사에너지의 일사량 분석을 실시하였고 산불사례조사를 통해 사면의 방향에 따라 산불발생 위험과 피해면적을 비교, 분석하였다. 그 결과 태양복사에너지 일사량이 가장 많은 사면의 향인 남사면을 중심으로 산불발생이 높은 것으로 분석되었다.

• Journal of the Korean earth science society
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• v.39 no.1
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• pp.89-102
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• 2018

We analyzed the meteorological and radiation characteristics of Seoul metropolitan area using data from energy flux towers that were installed and operated by the Weather Information Service Engine (WISE). The meteorological and radiation variables included temperature, pressure, wind speed, wind direction, relative humidity, surface temperature, rainfall amount, upward and downward solar radiation, upward and downward longwave radiation, albedo and emissivity from 14 energy flux stations located in the Seoul metropolitan area from July 2016 to July 2017. According to the monthly data during the period, the albedo is low and emissivity is high at the Jungnang station in the urban and opposite at Bucheon station in the suburban area. For a station in natural state, the albedo was higher than urban stations because solar radiation reflects effectively. Relatively high temperatures were shown at stations located in urban area with low albedo and high emissivity, in general. However, temperature was high at Gajwa and Ttukseom stations, the albedo was relatively high due to the station environment surrounded by glass wall buildings and the Han river. In the station located in suburban area, both emissivity and temperature were low. Among these stations, Bucheon station had the highest emissivity values because the surface temperature was relatively lower than that of the suburban area. As a result, the albedo decreased and the emissivity increased at stations in urban areas. Additionally, Seoul metropolitan area had less than $100Wm^{-2}$ of net radiation, which implied that radiation energy could be absorbed in the atmosphere.