PAOFCDN: A novel method for predictive analysis of solar irradiance

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-10-22 DOI:10.1016/j.jastp.2024.106376
Sana Mujeeb
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Abstract

Solar photovoltaic power is the most feasible Renewable Energy Source (RES) for Pakistan, due to ample sunlight availability throughout the year. Since solar photovoltaic power is primarily dependent on solar irradiance, forecasting of solar irradiance is essential for reliable, secure and effective incorporation of solar photovoltaic power in power systems. Considering the importance of solar irradiance forecasting, in this study, predictive analysis of Islamabad’s solar irradiance is performed by using a novel proposed model named as Pelican Algorithm-based Optimized Fully-Connected Deep Network (PAOFCDN). The initial weights of Fully-Connected Deep Network (FCDN) are optimized through an effective optimization technique known as Pelican optimization. The accuracy of the optimized network PAOFCDN is enhanced many fold as compared to the FCDN network trained with randomly initialized weights. The inherent issue of poor generalization in FCDN is also resolved by optimization. The superior performance of PAOFCDN is evident from its comparative evaluation with existing benchmark methods, i.e., Long Short-Term Memory (LSTM), Support Vector Regression (SVR), Least Square Boosting (LSBoost) and standard FCDN. PAOFCDN achieves the least Normalized Root Mean Square Error (NRMSE) of 0.0503 as compared to 0.1179 of LSTM, 0.1256 of FCDN, and 0.2992 of SVR and LSBoost. The proposed model is applied to three real-world solar irradiance datasets having different resolutions of 10-minutes, hourly and daily. This study took the initiative of performing predictions on three datasets having multiple resolutions in perspective of south asia.
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PAOFCDN:预测分析太阳辐照度的新方法
太阳能光伏发电是巴基斯坦最可行的可再生能源 (RES),因为巴基斯坦全年都有充足的日照。由于太阳能光伏发电主要依赖于太阳辐照度,因此要将太阳能光伏发电可靠、安全、有效地纳入电力系统,就必须对太阳辐照度进行预测。考虑到太阳辐照度预测的重要性,在本研究中,通过使用一种名为 "基于鹈鹕算法的优化全连接深度网络(PAOFCDN)"的新模型,对伊斯兰堡的太阳辐照度进行了预测分析。全连接深度网络(FCDN)的初始权重是通过一种名为鹈鹕优化的有效优化技术进行优化的。与使用随机初始化权重训练的 FCDN 网络相比,经过优化的 PAOFCDN 网络的准确性提高了许多倍。FCDN 固有的泛化能力差的问题也通过优化得到了解决。PAOFCDN 与现有基准方法(即长短期记忆 (LSTM)、支持向量回归 (SVR)、最小平方提升 (LSBoost) 和标准 FCDN)的比较评估表明,PAOFCDN 性能优越。与 LSTM 的 0.1179、FCDN 的 0.1256 以及 SVR 和 LSBoost 的 0.2992 相比,PAOFCDN 的归一化均方根误差(NRMSE)最小,为 0.0503。提出的模型被应用于三个真实世界的太阳辐照度数据集,这些数据集的分辨率各不相同,分别为 10 分钟、每小时和每天。本研究以南亚地区为视角,对三个具有不同分辨率的数据集进行了预测。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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