• 대기
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• 제29권1호
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• pp.61-74
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• 2019

To investigate the observational environment, sky line and skyview factor (SVF) are calculated using a digital elevation model (DEM; 10 m spatial resolution) and 3 dimensional (3D) sky image at radiation site, Gangneung-Wonju National University (GWNU). Solar radiation is calculated using GWNU solar radiation model with and without the sky line and the SVF retrieved from the 3D sky image and DEM. When compared with the maximum sky line elevation from Skyview, the result from 3D camera is higher by $3^{\circ}$ and that from DEM is lower by $7^{\circ}$. The SVF calculated from 3D camera, DEM and Skyview is 0.991, 0.998, and 0.993, respectively. When the solar path is analyzed using astronomical solar map with time, the sky line by 3D camera shield the direct solar radiation up to $14^{\circ}$ with solar altitude at winter solstice. The solar radiation is calculated with minutely, and monthly and annual accumulated using the GWNU model. During the summer and winter solstice, the GWNU radiation site is shielded from direct solar radiation by the west mountain 40 and 60 minutes before sunset, respectively. The monthly difference between plane and real surface is up to $29.18M\;m^{-2}$ with 3D camera in November, while that with DEM is $4.87M\;m^{-2}$ in January. The difference in the annual accumulated solar radiation is $208.50M\;m^{-2}$ (2.65%) and $47.96M\;m^{-2}$ (0.63%) with direct solar radiation and $30.93M\;m^{-2}$ (0.58%) and $3.84M\;m^{-2}$ (0.07%) with global solar radiation, respectively.

• 한국신재생에너지학회:학술대회논문집
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• 한국신재생에너지학회 2009년도 춘계학술대회 논문집
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• pp.139-142
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• 2009

The worldwide energy market is enlarging rapidly according to current issues like globalization, deregulation, global warming and strengthening for environmental regulation as well as the energy technology is developing speedily by the add of information and communication techniques. In spite of these advanced techniques in the field of the renewable energy, solar power depends on the governmental aid largely in comparison with other renewable energy sources because of the high initial investment cost. Therefore it is important to investigate scrupulously for the expected erection site of solar power plant from the planning stage. This paper shows actual measurement data of solar radiation of scheduled solar power locations in the waterworks site with consideration of waterworks facilities and regional specialties and presents the data which was analyzed comparably with the radiation data of adjacent locations served by national authorities. In addition, these data were analyzed using RETScreen and used for making decision on the business validity.

• 태양에너지
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• 제11권3호
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• pp.3-8
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• 1991

우리나라의 오지 또는 섬 등지에 태양에너지 이용기기의 설치는 대체에너지 이용차원에서도 실현되어야 할 분야이다. 이러한 태양에너지 이용기기의 설계를 위한 필수자료는 신뢰성있는 일사량의 측정 및 그의 분석이다. 그러나 국내에는 15개 지역에 일사량을 측정할 수 있는 시스템이 설치되어 있지만 전력수급이 쉽지 않은 오지에서의 정확한 일사자원의 평가는 불가능하다. 따라서 본 연구를 통하여 무인자동일사량 측정시스템(KIER 시스템)을 개발하여 기존의 HWS 시스템과 같이 우리나라의 독도에 설치하여 그 성능을 비교하였다. 그 결과 절대오차가 3% 내외로 신뢰도가 높았으며, 1989년 10월부터 8개월 동안의 전 일사량의 평균치는 약 $2,330W/m^2$ day로 독도에서 태양에너지 이용시스템의 설치 및 활용가능성이 높은 것을 알 수 있었다. 본 KIER 시스템은 앞으로 독도 이외의 오지지역에도 설치를 추진할 예정이다.

• 한국지구과학회지
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• 제40권2호
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• pp.119-134
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• 2019

기상청 일사관측소 관측환경 분석을 위하여 수치표고모델(DEM)과 태양복사모델을 이용하여 주변지형에 의한 차폐와 하늘시계요소(SVF) 및 일사량을 산출하였다. 지형고도자료(10 m 해상도)를 통해 관측소를 중심으로 주변 25 km내의 지형들을 이용하여 스카이라인과 SVF를 계산하였다. 또한, 일사관측소별 산출된 천기도와 스카이라인을 중첩하여 지형에 의한 차폐를 분석하였다. 특히 인천 관측소는 주변지형의 차폐가 적었고 청송군과 추풍령 관측소는 주변 지형에 의한 차폐가 큰 관측소로 나타났다. 태양복사모델을 이용하여 동일 조건에서 지형 특성에 따른 일사량을 산출하여 지형에 의한 기여도를 분석하였다. 연누적 일사량 계산결과, 청송군 관측소의 경우 수평면 일사량과 비교하였을 때 직달일사량은 12.0% 이상 차폐되었고 산란일사량은 5.6% 그리고 전천일사량은 4.7% 감소하였다. 평균 일누적 일사량을 기준으로 편차를 분석하였을 때 0.3% 이상 전천일사량이 감소되는 지점은 6개 관측소였다. 42개 관측소 중 8소는 관측소의 이전 또는 관측장비의 이동설치가 시급한 것으로 분석되었고 1/2 이상(24소)의 관측소는 일사관측환경에 대한 검토가 필요한 것으로 분석되었다. DEM자료는 관측소 주변의 인공구조물과 식생 등이 포함되지 않기 때문에 더 상세한 관측환경분석이 요구된다.

• KIEAE Journal
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• 제11권1호
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• pp.15-20
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• 2011

Computer simulation of buildings and solar energy systems is being used increasingly in energy assessments and design. For the six locations (Seoul, Incheon, Daejeon, Deagu, Gwangju and Busan) in South Korea where the global hourly solar irradiation (GHSI) is currently measured, GHSI was calculated using a comparatively simple cloud cover radiation model (CRM) and sunshine fraction radiation model (SFRM). The result was that the measured and calculated values of GHSI were similar for the six regions. Results of cloud cover and sunshine fraction models have been compared with the measured data using the coefficient of determination (R2), root-mean-square error (RMSE) and mean bias error (MBE). The strength of correlation R2 varied within similar ranges: 0.886-0.914 for CRM and 0.908-0.934 for SFRM. Average MBE for the CRM and SFRM were 6.67 and 14.02 W/m2, respectively, and average RMSE 104.36 and 92.15 W/m2. This showed that SFRM was slightly accurate and used many regions as compared to CRM for prediction of GHSI.

• 환경영향평가
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• 제24권3호
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• pp.205-216
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• 2015

전 지구와 남한, 북한, 일본 지역을 중심으로 한 동북아시아 지역에 대한 기온, 강수량, 일사량의 미래 변화를 정량적으로 평가하기 위해 총 34개 GCM에 의해 작성된 CMIP5 기후변화 시나리오를 분석하였다. 그 결과 동북아시아 지역에서 전 지구 평균보다 기온과 강수량이 증가하는 것으로 예측되었다. 특히 RCP 8.5 시나리오의 2080년대 북한 지역에서는 비록 GCM 간 예측의 불확실성이 크지만 과거 30년(1971-2000년)에 비해 기온은 $5.1^{\circ}C$, 강수량은 18% 증가하는 것으로 예측되었다. 일사량의 경우 전 지구 평균 일사량은 RCP 2.6 시나리오를 제외한 모든 RCP 시나리오에서 대체로 시간이 경과할수록 감소하는 것으로 예측되었으나 동북아시아 지역에서는 대체로 시간이 경과할수록 운량 감소의 영향으로 일사량이 증가하는 것으로 예측되었다.

• 한국신재생에너지학회:학술대회논문집
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• 한국신재생에너지학회 2008년도 추계학술대회 논문집
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• pp.171-173
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• 2008

The amount of incident solar rays on inclined surfaces with various directions has been widely utilized as important data in installing solar collector, hot water system, and designing solar buildings and house. This is because the performance of the solar energy applied systems is much affected by angle and direction of incident rays. Recognizing those factors mentioned above are of importance, actual experiment has been performed in this research to obtain the angle of inclination with which the maximum incident rays can be absorbed. The results obtained in this research could be used in designing optimal solar thermal systems.

• 설비공학논문집
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• 제24권6호
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• pp.461-466
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• 2012

Recently, building energy systems with solar collector and solar module have increased to improve energy problem, a heat island, a global warming and carbon dioxide emissions. In this study, value of solar radiation in areas was analyzed using TRNSYS simulation, and the optimum tilt and orientation angle for installing a photovoltaic module was examined. Average values of the weather data in the past twenty years in areas were used as input data. The results show that the tilt angle of a photovoltaic module for gaining the annual maximum solar radiation varies in different localities, and values of the annual solar radiation gained by using the variable photovoltaic module increased by 2.5 percent as compared with that gained by using the fixed photovoltaic module. When fixed photovoltaic module is installed, it should be examined the tilt and orientation angle for installing a photovoltaic module was examined.

• 천문학회보
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• 제38권2호
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• pp.94.1-94.1
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• 2013

Whistler mode chorus waves, which are observed outside the plasmasphere of the Earth's magnetosphere, play a major role in accelerating and scattering energetic electrons in the radiation belts. In this study we developed a predicting scheme of the global distribution of chorus by using the Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellite data. First, we determined global spatial distributions of chorus activity, and identified fit functions that best represent chorus intensities in specific L-MLT zones. Second, we determined the specific dependence of average chorus intensity on preceding solar wind conditions (e.g., solar wind speed, IMF Bz, energy coupling degree) as well as preceding geomagnetic states (as represented by AE, for example). Finally, we combined these two results to develop the predicting functions for the global distribution and intensity of chorus. Implementing these results in the radiation belt models should improve the local acceleration effect by chorus waves.

• 한국태양에너지학회 논문집
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• 제35권1호
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• pp.9-19
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• 2015

Pyranometer have many uncertainty factors (sensitivity function, thermal offset, other spectral effect, geometric, environment, and equipment etc.) than pyrheliometer. The solution for most of the uncertainty factors have been researched, but the problem for thermal offset is being continued research so far. Under the clear sky, due to the thermal offset of pyranometer, the diffuse and global radiation have been negative value for the nighttime and lower value for the daytime, respectively. In order to understand the uncertainty of the thermal offset effect, solar radiation are observed and analyzed using Ji and Tsay method and data from modified pyranometer. As a result of performing temperature correction using the modified pyranometer, the slope (dome factor; k) and intercept ($r_0$) from a linear regression method are 0.064 and $3.457g{\cdot}m^{-2}{\cdot}k^{-1}$, respectively. And the solar radiation is decreased significantly due to the effect of thermal offset during nighttime. The solar radiation from modified pyranometer increased approximately 8% higher than its observed by general pyranometer during daytime. By the way, these results did not generalize because its result is for only single case in clear sky. Accordingly, it is to required for accurate results obtained by the various cases (clear, cloudy and rainy) with longterm observations.