Novel hybrid kepler optimization algorithm for parameter estimation of photovoltaic modules

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作者
Reda Mohamed
Mohamed Abdel-Basset
Karam M. Sallam
Ibrahim M. Hezam
Ahmad M. Alshamrani
Ibrahim A. Hameed
机构
[1] Zagazig University,Department of Computer Science
[2] University of Sharjah,School of IT and Systems, Faculty of Science and Technology
[3] University of Canberra,Statistics & Operations Research Department, College of Sciences
[4] King Saud University,Department of ICT and Natural Sciences
[5] Norwegian University of Science and Technology (NTNU),undefined
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The parameter identification problem of photovoltaic (PV) models is classified as a complex nonlinear optimization problem that cannot be accurately solved by traditional techniques. Therefore, metaheuristic algorithms have been recently used to solve this problem due to their potential to approximate the optimal solution for several complicated optimization problems. Despite that, the existing metaheuristic algorithms still suffer from sluggish convergence rates and stagnation in local optima when applied to tackle this problem. Therefore, this study presents a new parameter estimation technique, namely HKOA, based on integrating the recently published Kepler optimization algorithm (KOA) with the ranking-based update and exploitation improvement mechanisms to accurately estimate the unknown parameters of the third-, single-, and double-diode models. The former mechanism aims at promoting the KOA’s exploration operator to diminish getting stuck in local optima, while the latter mechanism is used to strengthen its exploitation operator to faster converge to the approximate solution. Both KOA and HKOA are validated using the RTC France solar cell and five PV modules, including Photowatt-PWP201, Ultra 85-P, Ultra 85-P, STP6-120/36, and STM6-40/36, to show their efficiency and stability. In addition, they are extensively compared to several optimization techniques to show their effectiveness. According to the experimental findings, HKOA is a strong alternative method for estimating the unknown parameters of PV models because it can yield substantially different and superior findings for the third-, single-, and double-diode models.
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