Abstract

This study focuses on the use of cloud motion vectors (CMV) and fast radiative transfer models (FRTM) in the prospect of forecasting downwelling surface solar irradiation (DSSI). Using near-real-time cloud optical thickness (COT) data derived from multispectral images from the spinning enhanced visible and infrared imager (SEVIRI) onboard the Meteosat second generation (MSG) satellite, we introduce a novel short-term forecasting system (3 h ahead) that is capable of calculating solar energy in large-scale (1.5 million-pixel area covering Europe and North Africa) and in high spatial (5 km over nadir) and temporal resolution (15 min intervals). For the operational implementation of such a big data computing architecture (20 million simulations in less than a minute), we exploit a synergy of high-performance computing and deterministic image processing technologies (dense optical flow estimation). The impact of clouds forecasting uncertainty on DSSI was quantified in terms of cloud modification factor (CMF), for all-sky and clear sky conditions, for more generalized results. The forecast accuracy was evaluated against the real COT and CMF images under different cloud movement patterns, and the correlation was found to range from 0.9 to 0.5 for 15 min and 3 h ahead, respectively. The CMV forecast variability revealed an overall DSSI uncertainty in the range 18–34% under consecutive alternations of cloud presence, highlighting the ability of the proposed system to follow the cloud movement in opposition to the baseline persistent forecasting, which considers the effects of topocentric sun path on DSSI but keeps the clouds in “fixed” positions, and which presented an overall uncertainty of 30–43%. The proposed system aims to support the distributed solar plant energy production management, as well as electricity handling entities and smart grid operations.

Highlights

  • Over the last decades, the main goal for worldwide sustainable development and mitigation policies for climate change is the turn to renewables against coal energy production

  • cloud modification factor (CMF) corresponds to cloud optical thickness (COT) values from 0 to 3 since larger values, in reality, make the downwelling surface solar irradiation (DSSI)

  • We made some comparisons between Farnebäck [32] (FRB) and the TVL motion flow approaches so as to identify the optimum conditions where both are able to provide much better results from the PRS method, where we keep clouds stationary, and all the other parameters change dynamically

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Summary

Introduction

The main goal for worldwide sustainable development and mitigation policies for climate change is the turn to renewables against coal energy production. According to the recent five-year forecasts report of the International Energy Agency (IEA) [1], until 2024, renewable energy production is designated to increase by 50%, with solar PV capacity leading this increment by more than half of this increase globally (~60%). Accurate knowledge of solar resources with their temporal and spatial variability is a prerequisite for every solar energy technology and for the integration of solar energy exploitation systems in every country’s share of annual electricity generation [2]. Based on the solar radiation attenuation potential, the key atmospheric parameter governing the amount of solar irradiance reaching the earth’s surface is cloud coverage, and the challenge for solar resources forecasting is the prediction of the future position and optical properties of clouds, which shows great spatial and temporal variability.

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