• 제목/요약/키워드: Solar light

검색결과 1,244건 처리시간 0.028초

질소 도핑 TiO2의 Methylene Blue 광분해 제거에의 적용 (Application of Photocatalytic Decomposition of Methylene Blue on N-doped TiO2)

  • 백미화;최수아;김동수
    • 한국물환경학회지
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    • 제26권4호
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    • pp.707-712
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    • 2010
  • Nitrogen-doped $TiO_2$ particles have been successfully prepared using titanium tetraisopropoxide as the Ti source and urea as the nitrogen source. As-prepared nitrogen-doped $TiO_2$ was characterized by X-ray diffraction (XRD), scanning electron microscopy (SEM), Brunauer-Emmett-Teller method (BET) and ultraviolet-visible light (UV-vis) absorption spectra techniques. Photocatalytic degradation of Methylene Blue (MB) has been carried out in both solar light (UV-vis) and the visible region (${\lambda}=420nm$). Nitrogen-doped $TiO_2$ exhibits higher activity than the commercial $TiO_2$ photocalyst, particularly under visible-light irradiation because bandgap of nitrogen-doped $TiO_2$ becomes remarkably decreased.

조명용 LED의 광전궤환을 이용한 가시광 무선인식장치 (Visible Light Identification System Using Optoelectronic Feedback of A Lighting LED)

  • 이성호
    • 센서학회지
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    • 제20권3호
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    • pp.193-198
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    • 2011
  • In this paper, we used optoelectronic feedback to generate the carrier frequency for the ASK modulation of a lighting LED. A solar cell was used for photo-detector in the feedback circuit, and the LED light was ASK modulated by controlling the ON/OFF state of the switch that is installed in the feedback loop. The oscillation frequency of the optoelectronic feedback loop was about 50 kHz and the data rate of the ASK modulation was 9.6 kbps. In experiments, the optoelectronic feedback circuit was used for the ASK modulation of a lighting LED in the transponder of a visible light identification system, and data exchange between the transponder and the reader was successfully carried out.

자연채광을 고려한 건축공간 설계방법 연구 - 전시공간 중심으로 - (A Study of Architectural Space Design Method Considering Daylight Penetration Control - Focusing on the Spaces for Exhibition -)

  • 태원진
    • 한국태양에너지학회 논문집
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    • 제25권4호
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    • pp.45-51
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    • 2005
  • Appling natural light to the spaces for the exhibition requires the compromises between the expectations of visitors whom are preferable to perceive the details of the works of art, and preservation of light sensitive artworks of least exposure to light. To solve the compromises, it requires a careful planing to control the penetration of the daylight by physical and mechanical devices such as diffusive glasses and blinds. The control of light penetration can also be achieved by providing spaces inside and outside of the building. The aim of this study is suggest the conceptual methods to control the daylight by space design. Museums and galleries using daylight were investigated how the daylight is controlled by the integrated spaces in the exhibition spaces. This study presents nine ways of controlling daylight penetration by space design.

2019 Total Solar Eclipse Expedition of KASI

  • Bong, Su-Chan;Yang, Heesu;Lee, Jae-Ok;Kim, Jinhyun;Jeon, Young-Beom;Jang, Bi-Ho;Seough, Jungjoon;Park, Young-Deuk
    • 천문학회보
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    • 제45권1호
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    • pp.69.2-69.2
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    • 2020
  • Korea Astronomy and Space Science Institute (KASI) is developing a coronagraph to measure the coronal electron density, temperature, and speed utilizing spectral change of the K-corona around 400 nm. However, near UV light is more affected by atmospheric effect on the ground than visible light. For the total solar eclipse on July 2 2019, KASI organized an expedition team to test the possibility of the similar measurement scheme in the visible light. The observation site was in Las Flores, San Juan, Argentina. We built an imaging spectrograph using micro lenslet array and grism, named Coronal Integral Field Spectrograph (CorIFS). In addition, images of white light corona, wide field background, and all sky were taken with various camera settings. We present the preliminary results of the expedition.

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수상 회전식 태양광 발전시설 설치에 따른 농업용 저수지의 수질변화 평가 (Evaluation of the Water Quality Changes in Agricultural Reservoir Covered with Floating Photovoltaic Solar-Tracking Systems)

  • 이인주;주진철;이창신;김가영;우도영;김재학
    • 대한환경공학회지
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    • 제39권5호
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    • pp.255-264
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    • 2017
  • 본 연구는 수상 태양광 발전시설의 설치로 인한 농업용 저수지의 수질변화를 평가하기 위해 경기도 안성시 금광저수지에 위치한 수상 회전식 태양광 발전시설에서 발전시설 설치에 따른 차광구역 6지점과 비차광구역 4지점을 선정하여 1년 동안 총 16회에 걸쳐 차광으로 인한 수질변화를 시간과 수심 별로 분석하였다. 이를 위해 수온, pH, DO, Chl-a, BGA 항목을 0.3 m, 1 m, 3 m, 5 m의 수심별로 측정하고, 표층의 시료를 채수하여 COD, TN, TP 항목을 분석하였다. 연구결과, 금광저수지 내 10곳의 측정지점 간의 관측된 전 수질항목에서 차이는 유의확률(p - value) 0.05 이상으로 유의수준(${\alpha}=0.05$)에서 서로 다르지 않다고 통계학적으로 분석되었다. 이러한 결과를 토대로 측정지점을 차광구역(site 1~6)과 비차광구역(site 7~10)으로 그룹화 후 시간 및 수심에 따른 변화를 확인하였다. 차광구역과 비차광구역 간의 수온, pH, DO, COD, TN, TP, Chl-a, BGA의 계절 및 수심에 따른 차이는 유의한 수준에서 통계학적으로 다르지 않았다(p > 0.05). Chl-a와 BGA의 경우, 7월에 비차광구역보다 차광구역에서 일부 높은 농도가 관측되었으나 이는 기록적인 가뭄과 낮은 저수량, 발전시설 구조물에 부착된 부착조류의 과다성장으로 인한 일시적 현상으로 전체 수질은 통계학적으로 유의할 만한 차이가 없는 것으로 조사되었다. 이러한 결과는 수상 회전식 태양광 발전시설의 설치로 인한 저수지 수면의 차광이 전체 수면적 대비 0.5% 미만으로 일사량 유입 감소효과는 취송 및 방류를 통한 저수지 수체의 혼합 효과 대비 미미했기 때문인 것으로 판단된다. 향후, 수상 태양광 발전시설 설치로 인한 수질변화를 면밀히 연구하기 위해서는 보다 넓은 면적의 태양광 발전시설의 설치로 인한 차광과 함께 장기적인 수질 및 수생태계 관측이 필요할 것으로 판단된다.

태양광 활용을 위한 효율적 LED 조명기구 설계 방안 (Energy Efficient LED Lighting Design to utilize the Sun Light)

  • 정학근;한수빈;장철용
    • 한국태양에너지학회 논문집
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    • 제31권2호
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    • pp.31-36
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    • 2011
  • LED is expected as an environmentally friendly next generation light source with its good reliability and long lifetime. The light sources for illumination have a variety of applications in the indoor and outdoor, and the variation of optical power and color rendering of the light source limits their applications. Therefore, it is necessary to research the LED lamp and its luminaire to minimize the variation of dynamic characteristics and to improve the color rendering due to that illuminating environment. Daylight is very good light source to human and can be used as primary or a secondary light source with benefits of energy, productivity and health.This paper presents the design method of LED lighting system to improve poor property in terms of CR(color redering) characteristic to use daylight effectively.

Self-textured Al-doped ZnO transparent conducting oxide for p-i-n a-Si:H thin film solar cell

  • 김도영;이준신;김형준
    • 한국재료학회:학술대회논문집
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    • 한국재료학회 2009년도 추계학술발표대회
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    • pp.50.1-50.1
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    • 2009
  • Transparent conductive oxides (TCOs) play an important role in thin-film solar cells in terms of low cost and performance improvement. Al-doped ZnO (AZO) is a very promising material for thin-film solar cellfabrication because of the wide availability of its constituent raw materials and its low cost. In this study, AZO films were prepared by low pressurechemical vapor deposition (LPCVD) using trimethylaluminum (TMA), diethylzinc(DEZ), and water vapor. In order to improve the absorbance of light, atypical surface texturing method is wet etching of front electrode using chemical solution. Alternatively, LPCVD can create a rough surface during deposition. This "self-texturing" is a very useful technique, which can eliminate additional chemical texturing process. The introduction of a TMA doping source has a strong influence on resistivity and the diffusion of light in a wide wavelength range.The haze factor of AZO up to a value of 43 % at 600 nm was achieved without an additional surface texturing process by simple TMA doping. The use of AZO TCO resulted in energy conversion efficiencies of 7.7 % when it was applied to thep-i-n a-Si:H thin film solar cell, which was comparable to commercially available fluorine doped tin oxide ($SnO_2$:F).

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SUN FLUX VARIATIONS DUE TO ORBITING PLANETS: THE SOLAR SYSTEM AS A NON-COMPACT PLANETARY SYSTEM

  • Barbier, Hugo;Lopez, Ericson D.;Tipan, Bryan;Vasconez, Christian L.
    • 천문학회지
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    • 제53권3호
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    • pp.69-75
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    • 2020
  • We study the photometric phase curves for the planets of our solar system which can be considered as a prototypical non-compact planetary system. We focus on modeling the small variations caused by three effects: reflection, ellipsoidal, and Doppler beaming. Theoretical predictions for these photometric variations are proposed, considering a hypothetical external observer. Unlike similar studies of multi-planetary systems, the physical and geometrical parameters for each planet of the solar system are well-known. Therefore, we can accurately evaluate the relationships that shape the planetary light curves for a fictitious external observer. Our results suggest that, for all planets, the ellipsoidal effect is very weak while the Doppler beaming effect (DBE) is, in general, dominant. In fact, the DBE seems to be the principal cause of variations of the light curves for the planets of the solar system. However, for Mercury and Venus the Doppler beaming and reflection effects have similar amplitudes. The phase curves obtained for the planets of the solar system show new interesting features of interest for the study of other non-compact planetary systems.

Perez Model을 적용한 태양광 시스템 별 최적 설치 조건 및 최대 발전량 분석 (An Analysis of Optimal Installation Condition and Maximum Power Generation of Photovoltaic Systems Applying Perez Model)

  • 이재덕;김철환
    • 전기학회논문지
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    • 제61권5호
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    • pp.683-689
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    • 2012
  • Photovoltaic(PV) system is one of power generation systems. Solar light in PV system is like the fuel of the car. The quantity of electricity generation, therefore, is fully dependent on the available quantity of solar light on the system of each site. If a utility can predict the solar power generation on a planned site, it may be possible to set up an appropriate PV system there. It may be also possible to objectively evaluate the performances of existing solar systems. Based on the theories of astronomy and meteorology, in this paper, Perez model is simulated to estimate the available quantity of solar lights on the prevailed photovoltaic systems. Consequently the conditions for optimal power generation of each PV system can be analyzed. And the maximum quantity of power generation of each system can be also estimated by applying assumed efficiency of PV system. Perez model is simulated in this paper, and the result is compared with the data of the same model of Meteonorm. Simulated site is Daejeon, Korea with typical meteorological year(TMY) data of 1991~2010.

비정질실리콘 태양전지에 대한 장시간 성능예측: 확장지수함수 모형 및 컴퓨터 모의실험 (Long-Term Performance of Amorphous Silicon Solar Cells with Stretched Exponential Defect Kinetics and AMPS-1D Simulation)

  • 박상현;유종훈
    • 한국진공학회지
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    • 제21권4호
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    • pp.219-224
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    • 2012
  • 태양광에 노출되어있는 동안 비정질실리콘 태양전지에서 일어나는 장시간 성능변화에 대해서 연구하였다. 그리고 결함밀도의 운동학 모형을 통해서 태양광으로 인한 태양전지 성능변화를 예측하였다. 특히, 전하운반자 수명이 결함밀도에 의해서 크게 영향을 받기 때문에 비정질실리콘 태양전지의 광유도 성능감소(light-induced degradation)가 확장지수함수 완화법칙(stretched-exponential relaxation)을 따르는 결함밀도에 의해서 물리적으로 설명된다. 그리고 확장지수함수 완화법칙과AMPS-1D 컴퓨터 프로그램의 모의실험에 의해서 비정질실리콘 태양전지의 광유도 성능감소를 계산했고, 모의실험의 결과를 옥외에 설치한 태양전지의 측정데이터에 비교하였다. 본 연구는 상온에서 다음과 같은 특성을 갖는 전형적인 비정질실리콘pin 태양전지에 대해서 모의실험을 진행했다: 두께${\approx}$300 nm, 내부전위${\approx}$1.05 V, 초기 결함밀도${\approx}5{\times}10^{15}cm^{-3}$, 초기 단락전류${\approx}15.8mA/cm^2$, 초기 채우기비율${\approx}0.691$, 초기 개방전압${\approx}0.865V$, 초기 변환효율${\approx}9.50%$.