Assessing climate variability and trends in global solar radiation over Saudi Arabia using the CLARA-A3 dataset

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Ahmad E. Samman , Mostafa Morsy , Abdallah Abdaldym , Heshmat Abdel Basset
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引用次数: 0

Abstract

The spatio-temporal distribution of global solar radiation (GSR) is essential for the effective integration of photovoltaic (PV) energy systems. Therefore, this study aims to investigate the long-term trend, variation, fluctuation, and abrupt changes of the GSR over Kingdom of Saudi Arabia (KSA). The observed GSR data from World Radiation Data Center (WRDC) were used to evaluate the gridded 0.25° × 0.25° CLARA-A3 dataset at the available five stations. The GSR data at another 10 stations from the CLARA-A3 dataset covering the different climatic regions in KSA during the period from 1979 to 2023 were extracted to facilitate the analysis and interpretation of GSR. The results showed that, CLARA-A3 produced high accuracy and reliability GSR data over KSA. Also, the monthly GSR ranges from 140 to 240 W/m2 as minimum during winter and from 280 to 340 W/m2 as maximum during summer. The coefficient of variation (CV) gradient, both annual and seasonal, varies from around 0.5 %–6 %, with the highest gradient occurring in the mountainous regions in southwestern KSA. Furthermore, the GSR has a positive Mann-Kendall (MK) trend during spring, followed by winter and annual trends, whereas a negative MK trend is detected during summer. The climatological variability of annual GSR behavior, analyzed using Gaussian and binomial low-pass filters, indicates a positive trend at the majority of stations. Finally, the first positive abrupt change in GSR values at all stations is found in 1999 and 2001, while the negative abrupt change was detected in 1992 at only three stations.
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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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