• 태양에너지
• /
• 제10권2호
• /
• pp.69-76
• /
• 1990

[ $TiO_2$ ] 박막을 물에 담그고 빛을 조사하였을때의 물의 광전기화학적 분해현상을 관찰하였다. $TiO_2$ 박막은 스프레이법에 의해 $SnO_2$ 네사글라스를 만들고 이 네사글라스 위에 딥-코오팅법을 이용하여 $TiO_2$ 박막을 코오팅하였다. 다양한 두께의 $TiO_2$ 박막의 I-V 특성을 조사하였고 SEM에 의해 그 표면 상태를 알아 보았다. 필름의 두께가 $1.8{\mu}m$ 일때 광전기 전류가 최대로 나타남을 볼 수 있었다. $TiO_2$ 박막을 산성 수용액(pH=1)에 담그고 Xe-램프를 광원으로 하여 광전기 화학반응에 의한 물의 광 분해에 의해 산소 및 수소 가스가 발생함을 볼 수 있었다.

• 한국태양에너지학회 논문집
• /
• 제30권6호
• /
• pp.118-124
• /
• 2010

In order to develop commercial model of 10kW dish-Stirling solar thermal power system, modification for the exiting facility was taken for a year as a Leading Project in KIER. During the project, solar tracking system, control and monitoring system and high durability reflector were developed and long term operation were performed. The solar tracking system was tested for four months to investigate the degree of precision and adapted to the control system for an actual operation from October in 2009. The sun tracking accuracy of ${\pm}4$ mrad using modified control system was obtained and the system operated successfully during the experimental period. The monitoring system displays engine pressure, electric generation amounts, generator RPM, receiver temperatures, and etc. from Stirling engine and weather data of Direct Normal Irradiation, Horizontal Global Insolation, wind speed & direction, and atmosphere temperature from weather station. According to the operating results in a clear sky day, electric power of 6,890 W was generated at the DNI value of 850 W/$m^2$ and the averaged solar-to-electricity efficiency during a whole day reached to 18.99%. From the overall operating results, linear power generation trend could be observed with increasing DNI value. The solar-to-electricity efficiency achieved to 19% around the DNI value of 700 W/$m^2$ and increased to 20% when the DNI value goes up to 900 W/$m^2$.

• 한국태양에너지학회 논문집
• /
• 제27권1호
• /
• pp.47-54
• /
• 2007

Interests on renewable energy are increased due to oil price and environmental problems aroused from the fossil energy usage. In this study, performances of a solar assisted hybrid heat pump system are analyzed by experimental method. The developed system could runs at two types of operating mode. When the storage temperature is higher than the set temperature, the stored hot water in storage tank is supplied to the load directly. On the other hand, when the storage temperature lower than the set temperature, the water inside of the storage tank is used as heat source of the heat pump. In this study, the system control temperature for the alternation of the operating mode is set to $40^{\circ}C$ of the storage tank outlet. As results, it is founded that the COP of the developed heat pump system shows between 3.0 and 3.5. It is resonable performance for the heating system with a renewable energy as secondary heat source. The solar collect used in this study could supplies heat to the storage tank at over 400 W/m2 solar intensity. If the irradiation is lower than the 400 W/m2, the circulation pump stored and it could not supply heat to the storage tank. It is found that the difference temperature between the outlet of the storage tank and collector is $3^{\circ}C$. Even though, the extended study should be conducted to get a optimum performance of the developed system with various operating condition and control strategies.

• 한국항공우주학회지
• /
• 제35권1호
• /
• pp.33-39
• /
• 2007

본 논문은 대기층을 통한 파장별 태양복사를 고려한 3차원 지상 물체의 표면 온도 분포를 예측하는 소프트웨어를 개발하는데 도움을 줄 것이다. 다양한 가스로 구성된 대기층을 통과하는 파장별 태양복사 에너지를 계산하기 위해서 LOWTRAN7을 이용하였으며, 여기서 얻어진 결과는 파장별 흡수 또는 총괄흡수 방식으로 에너지보존방정식에 반영하였다. 원통형 물체 위의 시간별 표면온도 분포를 나타내기 위해서 준 내재적 방법을 사용하여 계산하였으며 물체의 파장별 표면 복사 특성을 이용하기 위해서 태양복사를 흡수하거나 물체의 표면 방사가 이루어지는 모델을 사용하였다. 본 논문에서는 개발된 S/W의 성능 향상을 위하여 파장별 태양복사 분석 방법과 총괄태양복사 분석 방법을 각각 적용하여 본 결과 이들 두 방법 사이에는 약 3% 이내의 차이를 나타내었으나 두 방법 모두 실용적 관점에서 충분한 결과를 나타내었음을 알 수 있었다.

• Korean Chemical Engineering Research
• /
• 제60권2호
• /
• pp.255-259
• /
• 2022

태양광을 이용한 증기 발생 방법은 순수한 물이 고갈되는 현재 사회에서 해수나 폐수에서 물을 수확할 수 있는 매우 유망한 기술이다. 태양광을 이용한 증기 발생 중에서 멤브레인을 이용한 증류법은 현재 개발 중에 있지만 멤브레인이 물과 직접 접촉하여 효율적인 증발량을 늘리기가 어려웠다. 본 연구에서는 PDMS (polydimethylsiloxane)와 산화 그래핀(GO)으로 구성된 태양열 멤브레인 증기 발생기와 부분적으로 멤브레인 전체에 절친 젖음성 제어를 통해 증발량을 개선하는 것을 제안하여 실험적 연구를 수행했다. 국부적인 젖음성 제어로 태양광과의 열교환 영역에서 열 국지화 및 온도 상승에서 상당한 개선을 보여주었다. 1sun(=1000 W/m)의 조사에서 1.54 kg m^-2 h^-1의 증발 능력을 갖습니다. 그 결과, 태양열 멤브레인 증기 발생 시스템은 국부적인 물 회수 성능 메커니즘을 이해 및 실험적 확인을 수행할 수 있었다.

• 대한전기학회:학술대회논문집
• /
• 대한전기학회 2009년도 춘계학술대회 논문집 전기설비전문위원
• /
• pp.183-185
• /
• 2009

In this thesis, output voltage, current and power of solar module were classified by irradiation and module temperature from data of overall operating characteristics collected for one year in order to manage efficient photovoltaic generation system and deliver maximum power. In addition, from these data, correlations between irradiation, module temperature of photovoltaic cell and amount of power given by photovoltaic cell was quantitatively examined to deduce optimization of the design and construction of photovoltaic generation system. The results of this thesis can be summarized as follows. As I-Y characteristics according to a temperature range of 10$\sim$50[], the area of I-V characteristics were increased with an increase in temperature. Since this area corresponds to the power, output power is thought to have increased with temperature.

• 대한전기학회:학술대회논문집
• /
• 대한전기학회 2009년도 춘계학술대회 논문집 전기설비전문위원
• /
• pp.186-188
• /
• 2009

In this thesis, output voltage, current and power of solar module were classified by irradiation and module temperature from data of overall operating characteristics collected for one year in order to manage efficient photovoltaic generation system and deliver maximum power. In addition, from these data, correlations between irradiation, module temperature of photovoltaic cell and amount of power given by photovoltaic cell was quantitatively examined to deduce optimization of the design and construction of photovoltaic generation system. The results of this thesis can be summarized as follows. As output power characteristics according to a temperature range of 10$\sim$50[], output power was increased with an increase in temperature. Since output power increases with temperature increase, the result corresponds well to the related equation on temperature and output power.

• 분석과학
• /
• 제11권1호
• /
• pp.13-19
• /
• 1998

Allylthiourea를 포함하고 있는 광전기화학전지를 이용하여, 태양에너지 변환을 위한 염료 감응시, 감응전류는 광조사 시간 증가에 따라 증감 현상을 보였다. 광조사 전후 염료 용액을 분광학적으로 분석한 결과 감응제와 초감응제 사이의 침전형성 반응과 염료의 광표백 현상이 광전류 감소와 관련되어 있는 것으로 확인되었다.

• 방사선산업학회지
• /
• 제4권3호
• /
• pp.285-288
• /
• 2010

Polyimide films have excellent thermal stability, reliable mechanical properties and low dielectric constant. Therefore, this material is widely used in many industrial fields such as microelectronics, flexible circuits, semiconductor products and aerospace materials. In space applications, earth-orbiting hardware operates in environments that generally include neutral particles, charged particles such as trapped protons and electrons, solar protons, and cosmic rays. Under these conditions, polyimide films were changed in the optical, electrical and mechanical properties. Therefore, in this study, we evaluated the effects of electron beam irradiation on polyimide. The O-H functional groups were created on the polyimide film surface in the results of FT-IR spectra. And it was found that the dielectric constants were changed as a function of electron beam dose.

• 천문학회보
• /
• 제46권1호
• /
• pp.50.1-50.1
• /
• 2021

Gravitational instability (GI) can produce massive gas giants on wide orbits by fragmentation of protoplanetary disks (PPDs). While most previous works focus on PPDs around solar mass stars, gas giants have been observed in systems with a wide range of stellar masses including M dwarfs. We use the GIZMO code to perform global three-dimensional simulations of self-gravitating disks around low-mass stars. Our models consider heating by turbulent viscosity and stellar irradiation and the β cooling occurring over the dynamical time. We run various models with differing disk-to-star mass ratio q and disk temperature. We find that strongly gravitating disks either produce spirals or undergo fragmentation. The minimum q value for fragmentation is 0.2-0.7, with a smaller value corresponding to a more massive star and/or a smaller disk. The critical q value depends somewhat sensitively on the disk temperature, suggesting that the stellar irradiation is an important factor in determining GI. We discuss our results in comparison with previous work as well as recent ALMA observations.