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Short-Term Solar Irradiance Forecasts Using Sky Images and Radiative Transfer Model

DOI:10.3390/en11051107 期刊:Energies 出版年份:2018 更新时间:2025-09-23 15:21:01
摘要: In this paper, we propose a novel forecast method which addresses the difficulty in short-term solar irradiance forecasting that arises due to rapidly evolving environmental factors over short time periods. This involves the forecasting of Global Horizontal Irradiance (GHI) that combines prediction sky images with a Radiative Transfer Model (RTM). The prediction images (up to 10 min ahead) are produced by a non-local optical flow method, which is used to calculate the cloud motion for each pixel, with consecutive sky images at 1 min intervals. The Direct Normal Irradiance (DNI) and the diffuse radiation intensity field under clear sky and overcast conditions obtained from the RTM are then mapped to the sky images. Through combining the cloud locations on the prediction image with the corresponding instance of image-based DNI and diffuse radiation intensity fields, the GHI can be quantitatively forecasted for time horizons of 1–10 min ahead. The solar forecasts are evaluated in terms of root mean square error (RMSE) and mean absolute error (MAE) in relation to in-situ measurements and compared to the performance of the persistence model. The results of our experiment show that GHI forecasts using the proposed method perform better than the persistence model.
作者: Juan Du,Qilong Min,Penglin Zhang,Jinhui Guo,Jun Yang,Bangsheng Yin
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To develop a novel forecast method for short-term solar irradiance forecasting that addresses the difficulty arising due to rapidly evolving environmental factors over short time periods.

The study demonstrates that combining prediction sky images with a Radiative Transfer Model (RTM) can quantitatively forecast DNI and DHI for time horizons shorter than 10 min. The RMSE and MAE errors of the presented forecast model were less than those of the persistence model, validating the use of prediction images combined with the RTM for short-term forecasting horizons.

1. The proposed method may generate large errors in the presence of optically thin cloud layers due to their blue-tinting effect. 2. All clouds in images containing the same optical depth values as in the RTM may cause a certain number of DHI errors. 3. The wide shadowband of TSI and the distance between TSI and MFRSR could cause prediction errors.

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