• 생물환경조절학회지
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• 제32권1호
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• pp.1-7
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• 2023

시설 내 작물이 이용하는 수광특성의 이해와 지속적으로 변화하는 광환경의 추적은 광합성과 증산반응 연구에서 중요하다. 또한 재배기간 동안 작물이 생장함에 따라 광이용 형태가 지속적으로 변화한다. 따라서 본 연구에서는 작물의 생육을 반영한 흡광계수 추정 모델을 개발하였다. 흡광계수의 측정을 위하여 작물의 높이에 따라 수직으로 일사량계를 5개 설치하였으며, 작물의 전 생육기간(1-85DAT) 동안 1초 단위로 측정을 하였다. 초기, 중기, 후기 각각의 생육단계에 따라 최상단 광량과 최하단의 광량의 차이가 69%, 72%, 81%로 증가하는 경향을 보였다. LAI와 초장이 증가함에 따라 흡광계수는 감소하였으며, 지수적 감소 관계를 보였다. 두 생육지표를 모두 반영한 3차원 모델에서는 Paraboloid 식이 평균 제곱근 오차(RMSE)가 1.340으로 가장 낮았고, 결정계수(R²)는 0.968로 가장 높았다. 본 연구를 통하여 작물 재배기간 동안 보다 정확한 흡광계수를 예측할 수 있게 되었고, 이는 작물의 높이에 따른 광합성 및 증산량 예측과 분석 연구에 활용될 수 있을 것으로 판단된다.

• Journal of Welding and Joining
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• 제16권4호
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• pp.125-135
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• 1998

The shielded metal arc welding (SMAW) by AC power source was performed to evaluate the arc stability by arc monitoring and analysing. In this study, the arc stability index was evaluated quantitatively by using he coefficient of resistance variation for welding time. This coefficient was obtained for the long time (20sec.) by analysing the waveforms of welding current, voltage and resistance. The coefficient was applied to indicate numerically the variation level of arc length and the degree of arc extinction. Using the coefficient of resistance variation in practical welding, the arc stability of the high titanium oxide electrode (KS E4313) turned out to be better than that of the low hydrogen electrode (KS E4316). In evaluating the skill level of welders by the coefficient, the horizontal fillet weaving welding became clear to be very discriminating because the higher level welder could weave in keeping constant arc length, but the lower level welder showed the characteristics of weaving with the unstable arc length. And it was confirmed that the welding defects as blow holes was formed when the arc stability index were high.

• 한국광학회지
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• 제35권1호
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• pp.1-8
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• 2024

유리기층에 코팅되어 있는 박막의 광학상수를 정확하게 분석하기 위해, 반투명 기층 위에 다층박막이 코팅되어 있는 시료의 유사 투과타원 상수 표현과 투과율 표현을 구체적으로 제시하였다. 두꺼운 기층에서 일어나는 다중반사로 인한 빛의 세기를 결맞지 않도록 중첩하는 동시에, 반투명 기층의 광흡수 영역에서 기층의 흡수를 정확하게 반영함으로써 다층박막이 코팅된 반투명 기층 시료의 정확한 모델링 분석이 가능하게 하였다. 흡광도가 매우 낮은 파장대역에서 투과율 측정에 기반한 분석과 타원법에 기반한 모델링 분석 방법이 가지는 박막의 소광계수의 차이를 투과율의 민감도와 타원상수의 민감도 분석을 통하여 비교 분석하였다. 투과율 분석법과 반사 타원법을 SiN 박막이 코팅된 유리기층 시료에 적용함으로써 소광계수가 매우 작을 때에도 SiN 박막의 복소굴절률과 두께를 정확하게 결정할 수 있음을 보였다.

• 한국대기환경학회:학술대회논문집
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• 한국대기환경학회 2005년도 추계학술대회 논문집
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• pp.463-465
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• 2005

• 한국대기환경학회:학술대회논문집
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• 한국대기환경학회 2004년도 춘계학술대회 논문집
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• pp.183-184
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• 2004

• 대기
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• 제18권4호
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• pp.287-297
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• 2008

The vertical profiles and optical properties of Asian dust are investigated using ground-based measurements from 1998 to 2002. Vertical profiles of aerosol extinction coefficient are evaluated using MPL (Micro Pulse Lidar) data. Optical parameters such as aerosol optical thickness ($\tau$), ${\AA}ngstr\ddot{o}m$ exponent ($\alpha$), single scattering albedo ($\omega$), refractive index, and volume size distribution are analyzed with sun/sky radiometer data for the same period. We can separate aerosol vertical profiles into three categories. First category named as 'Asian dust case', which aerosol extinction coefficient is larger than $0.15km^{-1}$ and dust layer exists from surface up to 3-4km. Second category named as 'Elevated aerosol case', which aerosol layer exists between 2 and 6km with 1-2.5km thickness, and extinction coefficient is smaller than $0.15km^{-1}$. Third category named as 'Clear sky case', which aerosol extinction coefficient appears smaller than $0.15km^{-1}$. and shows that diurnal variation of background aerosol in urban area. While optical parameters for first category indicate that $\tau$ and $\alpha$ are $0.63{\pm}0.14$, $0.48{\pm}0.19$, respectively. Also, aerosol volume concentration is increased for range of 1 and $4{\mu}m$, in coarse mode. Optical parameters for second category can be separated into two different types. Optical properties of first type are very close to Asian dust cases. Also, dust reports of source region and backward trajectory analyses assure that these type is much related with Asian dust event. However, optical properties of the other type are similar to those of urban aerosol. For clear sky case, $\tau$ is relatively smaller and $\alpha$ is larger compare with other cases. Each case shows distinct characteristics in aerosol optical parameters.

• 한국환경보건학회지
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• 제44권1호
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• pp.1-14
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• 2018

Objectives: The purpose of this study is to investigate the main cause of visibility impairment by analyzing the contributions of the light extinction coefficient of major air pollution components and the change of the light extinction coefficient by relative humidity. Methods: The characteristics of the light extinction coefficient calculated by the photochemical method using fine particle component data measured in 2015 in the Gwangju area were examined. Results: The extinction efficiency per unit mass of $PM_{2.5}$ particles was $4.5m^2/g$ and that of $PM_{10-2.5}$ particles was $0.6m^2/g$. This difference indicates that most of the visibility impairment in Gwangju was caused by $PM_{2.5}$ particles. When visibility was poor, the contribution of ammonium sulphate and ammonium nitrate was significantly increased. Relative humidity was also a major cause of visibility decay. The influx of air currents in Gwangju was mostly caused by the long distance movement of pollutants emitted from the eastern part of China. Ammonium sulphate and ammonium nitrate, which are hygroscopic secondary contaminants, were the main causative agents of visibility impairment. Conclusions: Ammonium sulphate and ammonium nitrate were the main causative agents of visibility impairment in Gwangju. The influx of air currents in Gwangju was mostly caused by the long distance movement of pollutants emitted from the eastern part of China.

• 한국안전학회지
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• 제22권6호
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• pp.13-19
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• 2007

Diesel car's smoke measurement equipment and method were investigated based on the exhaust gas regulations. Reflection photo method and light extinction method for measuring smoke were compared under conditions of both no load mode and Lug-down 3 mode. Free acceleration mode at no load condition was used for regular inspection of diesel car, and Lug-down 3 mode was used for fine inspection of the diesel car. A correlation between no load mode and Lug-down 3 mode was investigated in this research. The smoke measured with reflection photo method was 1.5${\sim}$2 times higher than that of light extinction method The correlation coefficient between reflection photo method and light extinction method for measuring smoke was 0.83, which shows comparatively high correlation between the two methods for measuring smoke in diesel engines.

• 한국대기환경학회지
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• 제10권2호
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• pp.137-145
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• 1994

A visibility analysis model based on the Mie theory is applied to the measurements during the fall, 1993 in Seoul. Model estimations of the total extinction coefficient $b_{ext}$, and the particle scattering coefficient, $b_{sp}$ are in good agreement with the measured values by a transmissometer and a nephelometer, respectively. These values show strong dependency on the mass loading of fine particles( $D_{p}$ ＜3.0${\mu}{\textrm}{m}$) but show no apparent relation with that of coarse particles(3.0${\mu}{\textrm}{m}$＜ $D^{p}$ ＜10${\mu}{\textrm}{m}$). Relative humidity plays an important role in determining the size of particles which in turn, affects the optical efficiency of aerosol. Based on the composition analysis with cut size nitrate concentration is higher than the sulfate concentration in PM3-10 but they are comparable to each other in PM3. Considering in 1985, it demonstrates a drastic increase of nitrate concentration between 1985 and 1993. It is found that measured and estimated light extinction budget were in good agreement within 10% and that scattering by particles is responsible for about 50-55% and 70-80 % of total extinction during clear and smoggy periods respectively.y.

• 천문학회보
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• 제44권2호
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• pp.67.4-67.4
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• 2019

We present extinction coefficients in the photometric filter system ugriz of the Sloan Digital Sky Survey, over a wide range of stellar properties based on theoretical stellar spectra generated using the ATLAS9 stellar models. Our computed coefficient values are essentially independent of a bulk metallicity or alpha-element abundance of a star, while they are a sensitive function of effective temperature and to a moderate extent of surface gravity of a star.