• 제목/요약/키워드: Solar Intensity

검색결과 352건 처리시간 0.029초

Solar Cells Characteristics Tester

  • Jirawath, Parnklang;Amnard, Jenjirodpipat;Santi, Hanklar
    • 제어로봇시스템학회:학술대회논문집
    • /
    • 제어로봇시스템학회 2000년도 제15차 학술회의논문집
    • /
    • pp.511-511
    • /
    • 2000
  • The equipment is used for testing the electrical characteristics of solar cells that were connected to be a solar panel, which can be found anywhere of solar power plant. This device was built from power switch devices f3r sinking the high current of the solar panel. The processor is a controller, which controls the quantity of the current, which flow through the switching devices and collect the characteristic of the solar panel. The tester can measure the current, voltage, temperature, and light intensity, which are main factors that affect the electrical characteristics of solar cells. 12 bits resolution signal converter is used to change the measuring levels so we can change measuring levels to 4096 levels, and these data are stored in tile memory. The equipment can also calculate the maximum power of the solar system panel.

  • PDF

국내 일사량 성분의 상세분석 (Detailed Analysis of Solar Radiation Components in Korea)

  • 조덕기;윤창열;김광득;강용혁
    • 한국신재생에너지학회:학술대회논문집
    • /
    • 한국신재생에너지학회 2011년도 추계학술대회 초록집
    • /
    • pp.129.2-129.2
    • /
    • 2011
  • Knowledge of the detailed solar radiation components are essential for modeling many solar systems. This is particularly the case for applications that concentrate the incident energy to attain high photo-dynamic efficiency achievable only at the higher intensities. In order to estimate the performance of concentrating solar systems, it is necessary to know the intensity of the beam radiation, as only this component can be concentrated. The Korea Institute of Energy Research(KIER) has began collecting detailed solar radiation component data since August, 1988. KIER's component data will be extensively used by solar system users or designers as well as by research institutes.

  • PDF

풍력발전시스템 출력에 대한 난류강도의 영향 연구 (A Study on the Effect of Wind Turbulence Intensity on the Power Performance of Wind Turbine System)

  • 현승건;주영철;김건훈
    • 한국태양에너지학회 논문집
    • /
    • 제32권4호
    • /
    • pp.17-23
    • /
    • 2012
  • The installed capacity of wind turbines in Korea are growing and enlarging by the central government's supporting program. But the majority area having the abundant wind energy resources is composed of mountainous and complex district, thus the turbulence intensity of there is so high and belongs to the turbulence characteristic A category of IEC design requirement. This paper presents the effect of the turbulence intensity on the power performance of a wind turbine system. Particularly, the effect of the power curve of the wind turbine system due to the turbulence intensity has analyzed. As a result, the power curve has a high turbulence characteristic shows the lower value than normal one in high wind speed regime and the AEP will be reduced at the relatively high turbulence area.

복잡지형에서 난류강도를 고려한 풍력발전단지설계 (Wind Farm Design Considering Turbulence Intensity on Complex Terrain)

  • 박미호;고경남;허종철
    • 한국태양에너지학회 논문집
    • /
    • 제33권6호
    • /
    • pp.1-11
    • /
    • 2013
  • The investigation on wind farm design using CFD technique was carried out to reduce turbulence intensity in a wind farm. A potential wind farm in Gasiri of Jeju Island was selected for the design and the commercial S/W of Meteodyn WT was used for applying CFD technique. The initial layout of wind turbines was derived using WindPRO which is mainly used for wind farm design in Korea. Then, the distribution of turbulence intensity on complex terrain was calculated and visible by Meteodyn WT. Based on the distribution, wind turbines were positioned properly. As a result, wind turbines could be deployed at positions with minimum turbulence intensity as well as maximum Annual Energy Production, AEP, using Meteodyn WT. It is necessary to take into account turbulence intensity in wind farm design to avoid wind turbine failure.

태양광/광촉매를 이용한 오폐수 살균특성 (Disinfection Characteristic of Sewage Wastewater Treatment Using Solar Light/TiO2 Film System)

  • 조일형;이내현;안상우;김영규;이승목
    • 한국환경과학회지
    • /
    • 제15권7호
    • /
    • pp.677-688
    • /
    • 2006
  • Currently, the application of $TiO_2$ photocatalyst has been focused on purification and treatment of wastewater. However, the use of conventional $TiO_2$ slurry photocatalyst results in disadvantage of stirring during the reaction and of separation after the reaction. And the usage of artificial UV lamp has made the cost of photocatalyst treatment system high. Consequently, we studied that solar light/$TiO_2$ film system was designed and developed in order to examine disinfection characteristics of sewage wastewater treatment. The optimum conditions for disinfection such as solar light intensity, characteristic of sewage wastewater, amounts of $TiO_2$ and comparison of solar ligth/$TiO_2$ systems with UV light/$TiO_2$ system was examined. The results are as follows: (1) photocatalytic disinfection process with solar light in the presence of $TiO_2$ film more effectively killed total coliform (TC) than solar light or $TiO_2$ film absorption only. (2) The survival ratio of TC and residual ratio of organic material (BOD, CODcr) decreased with remain resistant material. (3) The survival ratio of TC and residual ratio of organic material (BOD, CODcr) decreased with the increase of amounts of $TiO_2$. (4) TC survival ratio decreased linearly with increasing UV light intensity. (5) The disinfection effect of solar light/$TiO_2$ slurry system decreased more than UV light/$TiO_2$ film systems. (6) The disinfection reaction followed first-order kinetics. We suggest that solar light instead of using artificial UV light was conducted to investigate the applicability of alternative energy source in the disinfection of TC and the degradation of organic material.

우주선 Intensity 조정자로서 자기구름과 그 주위의 행성간 충격파 sheath 영역의 역할 (Magnetic Cloud and its Interplanetary Shock Sheath as a Modulator of the Cosmic Ray Intensity)

  • 오연수
    • Journal of Astronomy and Space Sciences
    • /
    • 제25권2호
    • /
    • pp.149-156
    • /
    • 2008
  • 우주선 intensity가 갑작스럽게 감소하는 대표적인 현상인 Forbush Decrease(FD)는 행성간 충격파(Interplanetary shock), 자기 구름(Magnetic cloud)과 같은 태양풍 이벤트와 밀접한 관련성을 가지고 있다. FD 현상에 대해 태양풍 이벤트 중 자기구름이 어느 정도 효과적으로 작용하는 지에 대해 알아보기 위해 1998-1999년의 2년 동안 발생한 44개의 자기 구름을 분석하였다. 그 결과 44개 중 11개의 자기 구름이 FD 현상과 관련이 있었으며, 자기 구름 영역이나 자기구름과 관계된 행성간 충격파의 sheath 영역의 평균 자기장 세기, 자기장 교란도 그리고 태양풍 속도와 같은 행성간 자기장 및 태양풍의 물리적 특성이 FD 현상과의 관련성을 대표해준다는 것을 밝혀냈다. 특히, 행성간 충격파 sheath 영역의 자기장 및 태양풍의 물리량이 자기장 세기가 13nT, 자기장 교란도는 3nT, 및 태양풍 속도가 평균 550km/s 이상의 태양풍 이벤트에서 FD 발생에 효과적으로 작용하는 것으로 분석되었다.

Dynamic Response of Charge Transfer and Recombination at Various Electrodes in Dye-sensitized Solar Cells Investigated Using Intensity Modulated Photocurrent and Photovoltage Spectroscopy

  • Kim, Gyeong-Ok;Ryu, Kwang-Sun
    • Bulletin of the Korean Chemical Society
    • /
    • 제33권2호
    • /
    • pp.469-472
    • /
    • 2012
  • Intensity modulated photocurrent spectroscopy and intensity modulated photovoltage spectroscopy were investigated to measure the dynamic response of charge transfer and recombination in the standard, $TiCl_4$-treated and the combined scattering layer electrode dye-sensitized solar cells (DSSCs). IMPS and IMVS provided transit time ($\tau_n$), lifetime ($\tau_r$), diffusion coefficient ($D_n$) and effective diffusion length ($L_n$). These expressions are derived that generation, collection, and recombination of electrons in a thin layer nanocrystalline DSSC under conditions of steady illumination and with a superimposed small amplitude modulation. In this experimental, IMPS/IMVS showed that the main effect of $TiCl_4$ treatment is to suppress the recombination of photogenerated electrons, thereby extending their lifetime. And the Diffusion coefficient of combined scattering layer electrode is $6.10{\times}10^{-6}$ higher than that of the others, resulting in longer diffusion length.

Empirical estimation of daily artifact of HMI Doppler velocities in the umbral region

  • Cho, Il-Hyun;Cho, Kyung-Suk;Bong, Su-Chan;Kim, Yeon-Han;Park, Young-Deuk
    • 천문학회보
    • /
    • 제39권1호
    • /
    • pp.71.1-71.1
    • /
    • 2014
  • To investigate physical properties of Solar pores, we use SDO/HMI data from 2010 to 2013. For this, we select single and isolated pores from the active region (Axx, Bxo, Bxi and Bxc-type) listed in Solar Region Summary. Pore is defined by connected pixels satisfying the intensity threshold from pixel of minimum intensity. We try to obtain area, intensity, magnetic field, and Doppler velocity of pores from HMI data. After removing the effects of orbital motion of the SDO satellite and differential rotation of the Sun, we identify that significant daily variations of Doppler velocity with non-zero ordinates still remain in the umbral region, and the artifact is quite dependent on the strength of magnetic field and radial component of velocity of SDO satellite. In this study we develope empirical model to remove the artifact. A preliminary result on the elimination of the artifact will be presented.

  • PDF

집광식 태양광발전시스템 설치를 위한 태양광자원 성분분석에 관한 연구 (A Study on the Analysis of Solar Radiation Components for the Installation of Concentrating Photovoltaic System)

  • 조덕기;강용혁
    • 한국태양에너지학회 논문집
    • /
    • 제27권2호
    • /
    • pp.53-59
    • /
    • 2007
  • Knowledge of the solar radiation components are essential for modeling many solar photovoltaic systems. This is particularly the case for applications that concentrate the incident energy to attain high photo-dynamic efficiency achievable only at the higher intensities. In order to estimate the performance of concentrating PV systems, it is necessary to know the intensity of the beam radiation, as only this component can be concentrated. The Korea Institute of Energy Research(KIER) has began collecting solar radiation component data since August, 1996. KIER's component data will be extensively used by concentrating PV system users or designers as well as by research institutes.

Abnormality of GCR intensities measured by ground NMs in solar minimum of solar cycles 23/24

  • Lee, Eo-Jin;Yi, Yu
    • 한국우주과학회:학술대회논문집(한국우주과학회보)
    • /
    • 한국우주과학회 2009년도 한국우주과학회보 제18권2호
    • /
    • pp.26.1-26.1
    • /
    • 2009
  • Many solar, interplanetary and geomagnetic activity parameters have 11-year cycle on the average in sync with solar sunspot number. The galactic cosmic ray (GCR) intensity measured by ground Neutron Monitor (NM) is one of those parameters showing the unprecedented activity levels in the current solar minimum (2008-2009) of solar cycles 23/24. We defined abnormality as the ratio of deviation from long term mean over mean amplitude of solar cycle change. The abnormality distribution map was drawn using all the data of NM stations available online. The implications of those unprecedented levels of GCR intensities of different cutoff rigidities will be discussed.

  • PDF