10 research outputs found

    Spatial mapping of short-term solar radiation prediction incorporating geostationary satellite images coupled with deep convolutional LSTM networks for South Korea

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    A practical approach to continuously monitor and provide real-time solar energy prediction can help support reliable renewable energy supply and relevant energy security systems. In this study on the Korean Peninsula, contemporaneous solar radiation images obtained from the Communication, Ocean and Meteorological Satellite (COMS) Meteorological Imager (MI) system, were used to design a convolutional neural network and a long short-term memory network predictive model, ConvLSTM. This model was applied to predict one-hour ahead solar radiation and spatially map solar energy potential. The newly designed ConvLSTM model enabled reliable prediction of solar radiation, incorporating spatial changes in atmospheric conditions and capturing the temporal sequence-to-sequence variations that are likely to influence solar driven power supply and its overall stability. Results showed that the proposed ConvLSTM model successfully captured cloud-induced variations in ground level solar radiation when compared with reference images from a physical model. A comparison with ground pyranometer measurements indicated that the short-term prediction of global solar radiation by the proposed ConvLSTM had the highest accuracy [root mean square error (RMSE) = 83.458 Wcenterdotmโˆ’2, mean bias error (MBE) = 4.466 Wcenterdotmโˆ’2, coefficient of determination (R2) = 0.874] when compared with results of conventional artificial neural network (ANN) [RMSE = 94.085 Wcenterdotmโˆ’2, MBE = โˆ’6.039 Wcenterdotmโˆ’2, R2 = 0.821] and random forest (RF) [RMSE = 95.262 Wcenterdotmโˆ’2, MBE = โˆ’11.576 Wcenterdotmโˆ’2, R2 = 0.839] models. In addition, ConvLSTM better captured the temporal variations in predicted solar radiation, mainly due to cloud attenuation effects when compared with two selected ground stations. The study showed that contemporaneous satellite images over short-term or near real-time intervals can successfully support solar energy exploration in areas without continuous environmental monitoring systems, where satellite footprints are available to model and monitor solar energy management systems supporting real-life power grid systems

    Forecasting for concentrated solar thermal power plants in Australia

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    Up to 50% of electricity needs in Australia could be supplied by solar power. At these high levels of solar power generation, solar forecasting is necessary to manage the impact of solar variability. However, there has been little research on using solar forecasting in Australia. This study used modelling to investigate the benefits of using short-term and long-term solar forecasts to operate a concentrated solar thermal (CST) plant for a year at four sites that covered different climate zones within the Australian National Electricity Market. Using 1-hour ahead short-term forecasts increased net value by 0.90โˆ’0.90-2.07 million for a CST plant with storage, and by 0.76โˆ’0.76-3.10 million for a CST plant without storage. It also improved reliability by reducing the equivalent forced outage rate by 21-38 percentage points for a CST plant with storage, and by 16-42 percentage points for a CST plant without storage. Using 1-hour forecasts achieved 59%-94% of the net value achievable if the 48-hour forecast were perfect. At each site, the highest net value and reliability were achieved by a CST plant with storage and using 1-hour forecasts, thus a CST plant should have both storage and short-term forecasts. If only one can be used, then a CST plant with storage and without 1-hour forecasts achieves higher net value, whereas a CST plant without storage and with 1-hour forecasts achieves higher reliability. These results demonstrated that using short-term forecasts is beneficial for CST plants that operate in electricity markets that allow updated bids to be submitted at short-term time frames. The results can be used to estimate the return on investment in obtaining short-term forecasts for operating a CST plant. Furthermore, the research method can be adapted into a tool for estimating value to assist CST plant project planning

    Calculation of Solar Irradiance from Weather Station Data and Satellite Images by Regionally Training Artificial Neural Network Models

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    ํ•™์œ„๋…ผ๋ฌธ (์„์‚ฌ)-- ์„œ์šธ๋Œ€ํ•™๊ต ๋Œ€ํ•™์› : ๊ณต๊ณผ๋Œ€ํ•™ ์—๋„ˆ์ง€์‹œ์Šคํ…œ๊ณตํ•™๋ถ€, 2019. 2. ๋ฐ•ํ˜•๋™.There are primarily two ways to estimate the solar irradiance of a certain area. One method is to directly measure the solar irradiance with a pyranometer, and the other is to indirectly estimate solar irradiance by satellite images. The former is good at accurately measuring solar irradiance with constant time intervals, but has a disadvantage in that the extent of measurement is limited to a small area. In contrast, although the latter can provide a wide range of estimation, the accuracy of its real time estimation is not so reliable. In order to complement the shortcomings of these two methods, this study uses COMS satellite images and Automated Synoptic Observing System (ASOS) weather observation data of the KMA (Korea Meteorological Administration). The interactions of multiple variables from these data sources with solar irradiance are so complex that it is difficult to build physical models to completely explain these mechanisms. Therefore, artificial neural network (ANN) is used for estimation, and the accuracy of ANN models are improved by training data regionally and applying average ensemble models. In order to train data for each region, solar irradiance regions need to be determined. Cloud indices (CI) were calculated from the visible channel of a COMS geostationary satellite, and its dimension was reduced by principal component analysis (PCA). Then, the data were classified into several regions by applying K-means clustering, and the optimal number of clusters was determined by L-method using the CH index. As a result, Korea was divided into 13 irradiance regions, 12 of which are practically used to build models, with the exception of one region of the sea. Ten input variables for the training of an artificial neural network were selected from 14 variablesthe 14 variables are composed of three variables of solar geometry, five variables from KMA ASOS stations, and six variables from COMS satellite images. A feature selection process was conducted by the mutual information feature selection method. From 10 selected variables, the multi-layer perceptron networks were built in MATLAB software environment. Data from 2016 were used for a training dataset, and data from 2017 were used for a validation dataset. The result of cross validation showed 0.96 of correlation coefficient 80.87 W/ใŽก of RMSE and 22.5% of rRMSE. In particular, a clear day showed a higher accuracy with 0.98 of correlation coefficient and 15% of rRMSE. However, a cloudy and overcast day showed lower accuracy. After ANN models were built by training a dataset from 2016, the model was applied to the dataset from 2017 for validation. Since the validation results showed similar accuracy with training, the model could be applied to any time series data. In addition, July to August showed lower accuracy because it is the rainy season in Korea. The regionally trained ANN ensemble models showed better accuracy than globally trained models, and also better than single models. Finally, the solar irradiances at 94 KMA ASOS stations were calculated from these models, so the annual and monthly solar irradiances of these sites in 2017 were calculated. The results of the calculation of annual solar irradiance showed that the irradiance is highly related to the irradiance regions. The monthly solar irradiance increased from January to May and June, and it decreased dramatically in the rainy season โ€“ July and August. These regional solar irradiance models can make it possible to estimate the solar irradiance of points that have no measured data from a pyranometer. These models can be applied to anywhere meteorological data is observed. Therefore, this can contribute to calculating hourly, daily, monthly, and annual solar irradiance more densely and accurately than existing solar irradiance measuring networks.์–ด๋Š ์ง€์—ญ์˜ ์ผ์‚ฌ๋Ÿ‰์„ ํŒŒ์•…ํ•˜๋Š” ๋ฐ๋Š” ๋‘ ๊ฐ€์ง€ ๋ฐฉ๋ฒ•์„ ์‚ฌ์šฉํ•  ์ˆ˜ ์žˆ๋‹ค. ์ฒซ ๋ฒˆ์งธ๋Š” ์ผ์‚ฌ๊ณ„๋ฅผ ์ด์šฉํ•˜์—ฌ ์ผ์‚ฌ๋Ÿ‰์„ ์ง์ ‘ ์ธก์ •ํ•˜๋Š” ๋ฐฉ๋ฒ•์ด๊ณ , ๋‹ค๋ฅธ ๋ฐฉ๋ฒ•์€ ์œ„์„ฑ์˜์ƒ์„ ์ด์šฉํ•˜์—ฌ ์ผ์‚ฌ๋Ÿ‰ ๊ฐ’์„ ๊ฐ„์ ‘์ ์œผ๋กœ ์ถ”์ •ํ•˜๋Š” ๋ฐฉ๋ฒ•์ด๋‹ค. ์ผ์‚ฌ๊ณ„๋ฅผ ์ด์šฉํ•˜๋ฉด ์‹œ๊ฐ„๋ณ„๋กœ ์ •ํ™•ํ•œ ์ผ์‚ฌ๋Ÿ‰ ๊ฐ’์„ ์•Œ ์ˆ˜ ์žˆ์ง€๋งŒ, ์‹œ์Šคํ…œ ๊ตฌ์ถ•์— ๋งŽ์€ ๋น„์šฉ์ด ๋“ค๊ณ  ์ผ์‚ฌ๋Ÿ‰์„ ํŒŒ์•…ํ•  ์ˆ˜ ์žˆ๋Š” ๋ฒ”์œ„๊ฐ€ ์ œํ•œ์ ์ด๋ผ๋Š” ๋‹จ์ ์ด ์žˆ๋‹ค. ๋ฐ˜๋ฉด ์œ„์„ฑ์˜์ƒ์„ ์ด์šฉํ•˜๋Š” ๋ฐฉ๋ฒ•์€ ๋„“์€ ์˜์—ญ์— ๊ฑธ์นœ ์ผ์‚ฌ๋Ÿ‰์„ ์•Œ ์ˆ˜ ์žˆ๋‹ค๋Š” ์žฅ์ ์ด ์žˆ์ง€๋งŒ, ์‹ค์‹œ๊ฐ„ ์ผ์‚ฌ๋Ÿ‰ ์‚ฐ์ถœ์˜ ์ •ํ™•๋„๊ฐ€ ๋†’์ง€ ์•Š๋‹ค๋Š” ๋‹จ์ ์ด ์žˆ๋‹ค. ๋ณธ ์—ฐ๊ตฌ์—์„œ๋Š” ์ด ๋‘ ๊ฐ€์ง€ ๋ฐฉ๋ฒ•์˜ ๋‹จ์ ์„ ๋ณด์™„ํ•˜๊ธฐ ์œ„ํ•ด ์ฒœ๋ฆฌ์•ˆ ๊ธฐ์ƒ์œ„์„ฑ ์˜์ƒ๊ณผ ๊ธฐ์ƒ์ฒญ์˜ ์ข…๊ด€๊ธฐ์ƒ๊ด€์ธก ์ž๋ฃŒ๋ฅผ ์ด์šฉํ•˜์—ฌ ์ผ์‚ฌ๋Ÿ‰์„ ์ถ”์ •ํ•˜์˜€๋‹ค. ์ด๋•Œ, ์ผ์‚ฌ๋Ÿ‰์— ์˜ํ–ฅ์„ ๋ฏธ์น˜๋Š” ๋ณ€์ˆ˜๋“ค ๊ฐ„์˜ ๋ฌผ๋ฆฌ์‹์„ ์•Œ๊ธฐ ์–ด๋ ต๊ธฐ ๋•Œ๋ฌธ์— ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ฐฉ๋ฒ•์„ ํ™œ์šฉํ•˜์˜€์œผ๋ฉฐ, ๊ถŒ์—ญ๋ณ„๋กœ ์ธ๊ณต์‹ ๊ฒฝ๋ง์„ ํ›ˆ๋ จ์‹œํ‚ค๊ณ  ์—ฌ๋Ÿฌ ๊ฐœ์˜ ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ ๊ฒฐ๊ณผ๋ฅผ ํ‰๊ท ํ•œ ์•™์ƒ๋ธ” ๋ชจ๋ธ์„ ํ™œ์šฉํ•จ์œผ๋กœ์จ ์ •ํ™•๋„๋ฅผ ํ–ฅ์ƒ์‹œ์ผฐ๋‹ค. ์ธ๊ณต์‹ ๊ฒฝ๋ง ํ›ˆ๋ จ์— ์•ž์„œ์„œ ์ฒœ๋ฆฌ์•ˆ ๊ธฐ์ƒ์œ„์„ฑ์˜ ๊ฐ€์‹œ๊ด‘ ์ฑ„๋„ ์˜์ƒ์œผ๋กœ๋ถ€ํ„ฐ ์ผ๋ณ„ ๊ตฌ๋ฆ„์ง€์ˆ˜๋ฅผ ์‚ฐ์ถœํ•œ ๋’ค, ์ฃผ์„ฑ๋ถ„ ๋ถ„์„์„ ํ†ตํ•ด ์ฐจ์›์„ ์ถ•์†Œํ•˜๊ณ  K ํ‰๊ท  ๊ตฐ์ง‘ํ™”๋ฅผ ์ ์šฉํ•จ์œผ๋กœ์จ ์ผ์‚ฌ๋Ÿ‰ ๊ถŒ์—ญ์„ ๋ถ„๋ฅ˜ํ•˜์˜€๋‹ค. ๊ถŒ์—ญ์˜ ๊ฐœ์ˆ˜๋Š” ๋ถ„๋ฅ˜๊ฐ€ ์ž˜ ๋˜์—ˆ๋Š”์ง€ ํ‰๊ฐ€ํ•˜๋Š” CH ์ง€์ˆ˜๋ฅผ ํ™œ์šฉํ•œ L-method ๋ฐฉ๋ฒ•์„ ํ†ตํ•ด ๊ฒฐ์ •ํ–ˆ์œผ๋ฉฐ, ์ด๋ฅผ ํ†ตํ•ด ํ•œ๊ตญ์„ ์ด 13๊ฐœ์˜ ๊ถŒ์—ญ, ๋ฐ”๋‹ค๋ฅผ ์ œ์™ธํ•˜๋ฉด 12๊ฐœ์˜ ๊ถŒ์—ญ์œผ๋กœ ๋ถ„๋ฅ˜ํ•˜์˜€๋‹ค. ์ธ๊ณต์‹ ๊ฒฝ๋ง ํ›ˆ๋ จ์„ ์œ„ํ•œ ์ž…๋ ฅ๋ฐ์ดํ„ฐ๋กœ๋Š”, ํƒœ์–‘์˜ ์œ„์น˜๋ฅผ ๋‚˜ํƒ€๋‚ด๋Š” 3๊ฐœ์˜ ๋ณ€์ˆ˜, ๊ธฐ์ƒ๊ด€์ธก์†Œ ์ž๋ฃŒ์˜ 5๊ฐœ์˜ ๋ณ€์ˆ˜, ์ฒœ๋ฆฌ์•ˆ ์˜์ƒ์„ ํ†ตํ•ด ์–ป์€ 6๊ฐœ์˜ ๋ณ€์ˆ˜ ์ด 14๊ฐœ์˜ ๋ณ€์ˆ˜๋“ค ์ค‘์—์„œ ์ƒํ˜ธ์ •๋ณด๋Ÿ‰ ํŠน์ง• ์ถ”์ถœ์„ ์ด์šฉํ•˜์—ฌ 10๊ฐœ์˜ ๋ณ€์ˆ˜๋ฅผ ์„ ํƒํ•˜์˜€๋‹ค. ์„ ํƒ๋œ 10๊ฐœ์˜ ๋ณ€์ˆ˜๋ฅผ ๊ฐ€์ง€๊ณ  MATLAB ์†Œํ”„ํŠธ์›จ์–ด๋ฅผ ํ™œ์šฉํ•˜์—ฌ ๋‹ค์ค‘๊ณ„์ธต์‹ ๊ฒฝ๋ง์„ ๊ตฌ์ถ•ํ–ˆ์œผ๋ฉฐ, 2016๋…„ ์ž๋ฃŒ๋ฅผ ํ›ˆ๋ จ์ž๋ฃŒ๋กœ, 2017๋…„ ์ž๋ฃŒ๋ฅผ ๊ฒ€์ฆ์ž๋ฃŒ๋กœ ์„ค์ •ํ•˜์˜€๋‹ค. 38๊ฐœ ์ผ์‚ฌ๋Ÿ‰ ๊ด€์ธก ์ง€์ ์— ๋Œ€ํ•ด ๊ต์ฐจ๊ฒ€์ฆ์„ ์ˆ˜ํ–‰ํ•œ ๊ฒฐ๊ณผ ์ƒ๊ด€๊ณ„์ˆ˜ 0.96, RMSE 80.87 W/ใŽก, rRMSE 22.6% ์ •๋„์˜ ์ •ํ™•๋„๋ฅผ ๊ธฐ๋Œ€ํ•  ์ˆ˜ ์žˆ์—ˆ์œผ๋ฉฐ, ํŠนํžˆ ๋ง‘์€ ๋‚ ์—๋Š” ์ƒ๊ด€๊ณ„์ˆ˜ 0.98, rRMSE 15% ์ •๋„์˜ ๋†’์€ ์ •ํ™•๋„๋ฅผ ๋ณด์˜€๋‹ค. ํ•˜์ง€๋งŒ ๊ตฌ๋ฆ„์˜ ์–‘์ด ๋งŽ์•„์งˆ์ˆ˜๋ก ์ •ํ™•๋„๊ฐ€ ๊ฐ์†Œํ–ˆ๋‹ค. 2016๋…„ ์ž๋ฃŒ๋กœ ํ›ˆ๋ จํ•œ ๋ชจ๋ธ์„ 2017๋…„ ์ž๋ฃŒ์— ์ ์šฉํ•˜์—ฌ ๊ฒ€์ฆ์„ ์ˆ˜ํ–‰ํ•œ ๊ฒฐ๊ณผ, ํ›ˆ๋ จ์˜ ์ •ํ™•๋„์™€ ๊ฒ€์ฆ์˜ ์ •ํ™•๋„๊ฐ€ ๋น„์Šทํ•˜๊ฒŒ ๋‚˜ํƒ€๋‚˜ ๋ชจ๋ธ์˜ ์‹œ๊ฐ„์  ๋ณดํŽธ์„ฑ์„ ํ™•์ธํ•  ์ˆ˜ ์žˆ์—ˆ๋‹ค. ๋ณธ ์—ฐ๊ตฌ์—์„œ ์ ์šฉํ•œ ๊ถŒ์—ญ๋ณ„ ํ›ˆ๋ จ ๋ชจ๋ธ์€ ๊ถŒ์—ญ๋ณ„๋กœ ํ›ˆ๋ จํ•˜์ง€ ์•Š์€ ์ „๊ตญ์  ๋ชจ๋ธ์— ๋น„ํ•ด ์˜ค์ฐจ๋ฅผ 2% ์ •๋„ ๊ฐ์†Œ์‹œํ‚ฌ ์ˆ˜ ์žˆ์—ˆ์œผ๋ฉฐ, ์•™์ƒ๋ธ” ๊ธฐ๋ฐ˜์˜ ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ ์—ญ์‹œ ๋‹จ์ผ ๋ชจ๋ธ๋ณด๋‹ค ์˜ค์ฐจ๋ฅผ 2% ์ •๋„ ๊ฐ์†Œ์‹œํ‚ด์œผ๋กœ์จ ์ •ํ™•๋„๋ฅผ ํ–ฅ์ƒ์‹œํ‚ค๋Š” ํšจ๊ณผ๊ฐ€ ์žˆ์—ˆ๋‹ค. ์ด๋ ‡๊ฒŒ ๊ตฌ์ถ•ํ•œ ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ์„ ์ ์šฉํ•˜์—ฌ 94๊ฐœ์˜ ๊ธฐ์ƒ์ฒญ ์ข…๊ด€๊ธฐ์ƒ๊ด€์ธก ์ง€์ ์— ๋Œ€ํ•ด 2017๋…„ ํ•œ ํ•ด ๋™์•ˆ์˜ ์‹œ๊ฐ„๋ณ„ ์ผ์‚ฌ๋Ÿ‰์„ ์‚ฐ์ถœํ•˜์˜€๊ณ , ์ด๋ฅผ ํ†ตํ•ด ๊ฐ ์ง€์ ์˜ ์—ฐํ‰๊ท  ์ผ์‚ฌ๋Ÿ‰๊ณผ ์›”ํ‰๊ท  ์ผ์‚ฌ๋Ÿ‰๋„ ์‚ฐ์ถœํ•˜์˜€๋‹ค. ์›”ํ‰๊ท  ์ผ์‚ฌ๋Ÿ‰ ์‚ฐ์ถœ๊ฒฐ๊ณผ๋ฅผ ์‚ดํŽด๋ณด๋ฉด ์ผ๋ฐ˜์ ์œผ๋กœ 1์›”๋ถ€ํ„ฐ 5, 6์›”๊นŒ์ง€ ์ผ์‚ฌ๋Ÿ‰์ด ์ ์ฐจ ์ฆ๊ฐ€ํ•˜๋‹ค๊ฐ€ 7, 8์›”์— ๊ธ‰๊ฒฉํžˆ ๊ฐ์†Œํ•˜๋Š” ๊ฒฝํ–ฅ์„ ๋ณด์˜€๋Š”๋ฐ, ์ด๋Š” ์—ฌ๋ฆ„์ฒ ์—๋Š” ์žฅ๋งˆ์™€ ํƒœํ’ ๋“ฑ์˜ ์˜ํ–ฅ์œผ๋กœ ์ผ์‚ฌ๋Ÿ‰์ด ๊ฐ์†Œํ•˜๊ธฐ ๋•Œ๋ฌธ์œผ๋กœ ๋ณด์ธ๋‹ค. ๋ณธ ์—ฐ๊ตฌ์˜ ๊ถŒ์—ญ๋ณ„ ์ผ์‚ฌ๋Ÿ‰ ๋ชจ๋ธ์„ ์ ์šฉํ•˜๋ฉด ์ผ์‚ฌ๋Ÿ‰ ๊ด€์ธก๊ฐ’์€ ์—†๋”๋ผ๋„ ์‹ค์‹œ๊ฐ„์œผ๋กœ ๊ธฐ์ƒ์ž๋ฃŒ ํš๋“์ด ๊ฐ€๋Šฅํ•œ ์ง€์ ์— ๋Œ€ํ•ด ์‹ค์‹œ๊ฐ„ ์ผ์‚ฌ๋Ÿ‰์„ ์ถ”์ •ํ•  ์ˆ˜ ์žˆ๋‹ค. ์ด๋ฅผ ํ†ตํ•ด ๊ธฐ์กด์˜ ์ผ์‚ฌ๋Ÿ‰ ๊ด€์ธก๋ง๋ณด๋‹ค ์ •๋ฐ€ํ•˜๊ณ  ์ •ํ™•ํ•˜๊ฒŒ ์ผ์‚ฌ๋Ÿ‰์„ ์ถ”์ •ํ•  ์ˆ˜ ์žˆ์„ ๊ฒƒ์œผ๋กœ ๊ธฐ๋Œ€๋œ๋‹ค.1. ์„œ๋ก  1 1.1. ์—ฐ๊ตฌ๋ฐฐ๊ฒฝ 1 1.2. ํƒœ์–‘๋ณต์‚ฌ์™€ ์ผ์‚ฌ๋Ÿ‰ 4 1.2.1. ํƒœ์–‘ ๋ณต์‚ฌ ์ŠคํŽ™ํŠธ๋Ÿผ 4 1.2.2. ๋Œ€๊ธฐ์— ์˜ํ•œ ํƒœ์–‘๋ณต์‚ฌ์˜ ๋ฐ˜์‚ฌ, ํก์ˆ˜, ์‚ฐ๋ž€ 5 1.3. ์ธ๊ณต์‹ ๊ฒฝ๋ง์˜ ์›๋ฆฌ์™€ ์‘์šฉ 8 1.3.1. ์ธ๊ณต์‹ ๊ฒฝ๋ง์˜ ๊ฐœ๋… 8 1.3.2. ๋‹ค์ค‘๊ณ„์ธต์‹ ๊ฒฝ๋ง 11 2. ์—ฐ๊ตฌ์ง€์—ญ ๋ฐ ๋ฐ์ดํ„ฐ 14 2.1. ๊ธฐ์ƒ๊ด€์ธก์ž๋ฃŒ 14 2.2. ์œ„์„ฑ์˜์ƒ ์ž๋ฃŒ 14 3. ๊ถŒ์—ญ๋ณ„ ์ธ๊ณต์‹ ๊ฒฝ๋ง ํ›ˆ๋ จ 17 3.1. ์ผ์‚ฌ๋Ÿ‰ ๊ถŒ์—ญ๋ถ„๋ฅ˜ 17 3.1.1. ๊ตฌ๋ฆ„์ง€์ˆ˜ ์‚ฐ์ถœ 17 3.1.2. ์ฃผ์„ฑ๋ถ„ ๋ถ„์„์„ ํ†ตํ•œ ์ฐจ์› ์ถ•์†Œ 21 3.1.3. K-ํ‰๊ท  ๊ตฐ์ง‘ํ™” 23 3.1.4. K-ํ‰๊ท  ๊ตฐ์ง‘ํ™”์˜ ์ตœ์ ๊ตฐ์ง‘ ๊ฐœ์ˆ˜ ์„ค์ • 23 3.1.5. ๊ถŒ์—ญ๋ณ„ ๋ถ„๋ฅ˜ ๊ฒฐ๊ณผ 26 3.2. ์ž…๋ ฅ๋ฐ์ดํ„ฐ ์„ ํƒ 30 3.2.1. ์ƒํ˜ธ ์ •๋ณด๋Ÿ‰ ํŠน์ง• ์ถ”์ถœ 30 3.2.2. ๋ณ€์ˆ˜ ์„ ํƒ ๊ฒฐ๊ณผ 33 3.3. ์ธ๊ณต์‹ ๊ฒฝ๋ง ํ›ˆ๋ จ 37 4. ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ์˜ ๊ฒ€์ฆ๊ณผ ๋น„๊ต 40 4.1. ์ •ํ™•๋„๋ฅผ ๋‚˜ํƒ€๋‚ด๋Š” ์ธ์ž 40 4.2. ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ์˜ ์ง€์ ๋ณ„ ๊ฒ€์ฆ ๊ฒฐ๊ณผ 41 4.3. ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ์˜ ๊ธฐ์ƒ์กฐ๊ฑด๋ณ„ ๊ฒ€์ฆ ๊ฒฐ๊ณผ 46 4.4. ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ์˜ ์—ฐ๋„๋ณ„ ๊ฒ€์ฆ ๊ฒฐ๊ณผ 55 4.5. ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ์˜ ์›”๋ณ„ ๊ฒ€์ฆ ๊ฒฐ๊ณผ 59 4.6. ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ์˜ ์‹œ๊ฐ„๋ณ„ ๊ฒ€์ฆ ๊ฒฐ๊ณผ 60 4.7. ๊ถŒ์—ญ๋ณ„ ํ›ˆ๋ จ ๋ชจ๋ธ๊ณผ ์ „๊ตญ์  ํ›ˆ๋ จ ๋ชจ๋ธ์˜ ๋น„๊ต 62 4.8. ์•™์ƒ๋ธ” ๋ชจ๋ธ๊ณผ ๋‹จ์ผ ๋ชจ๋ธ์˜ ๋น„๊ต 66 5. ์ธ๊ณต์‹ ๊ฒฝ๋ง ๋ชจ๋ธ์˜ ์ ์šฉ๊ณผ ์ผ์‚ฌ๋Ÿ‰ ์ถ”์ • 70 6. ๊ฒฐ๋ก  79 ์ฐธ๊ณ ๋ฌธํ—Œ 81 Abstract 89Maste

    Renewable Energy Resource Assessment and Forecasting

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    In recent years, several projects and studies have been launched towards the development and use of new methodologies, in order to assess, monitor, and support clean forms of energy. Accurate estimation of the available energy potential is of primary importance, but is not always easy to achieve. The present Special Issue on โ€˜Renewable Energy Resource Assessment and Forecastingโ€™ aims to provide a holistic approach to the above issues, by presenting multidisciplinary methodologies and tools that are able to support research projects and meet todayโ€™s technical, socio-economic, and decision-making needs. In particular, research papers, reviews, and case studies on the following subjects are presented: wind, wave and solar energy; biofuels; resource assessment of combined renewable energy forms; numerical models for renewable energy forecasting; integrated forecasted systems; energy for buildings; sustainable development; resource analysis tools and statistical models; extreme value analysis and forecasting for renewable energy resources

    Atmospheric effects on land classification using satellites and their correction.

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    Haze occurs almost every year in Malaysia and is caused by smoke which originates from forest fire in Indonesia. It causes visibility to drop, therefore affecting the data acquired for this area using optical sensor such as that on board Landsat - the remote sensing satellite that have provided the longest continuous record of Earth's surface. The work presented in this thesis is meant to develop a better understanding of atmospheric effects on land classification using satellite data and method of removing them. To do so, the two main atmospheric effects dealt with here are cloud and haze. Detection of cloud and its shadow are carried out using MODIS algorithms due to allowing optimal use of its rich bands. The analysis is applied to Landsat data, in which shows a high agreement with other methods. The thesis then concerns on determining the most suitable classification scheme to be used. Maximum Likelihood (ML) is found to be a preferable classification scheme due to its simplicity, objectivity and ability to classify land covers with acceptable accuracy. The effects of haze are subsequently modelled and simulated as a summation of a weighted signal component and a weighted pure haze component. By doing so, the spectral and statistical properties of the land classes can be systematically investigated, in which showing that haze modifies the class spectral signatures, consequently causing the classification accuracy to decline. Based on the haze model, a method of removing haze from satellite data was developed and tested using both simulated and real datasets. The results show that the removal method is able clean up haze and improve classification accuracy, yet a highly non-uniform haze may hamper its performance
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