Arnida L. Latifah , Amandha Affa Auliya , Inna Syafarina , Sheila Dewi Ayu Kusumaningtyas
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引用次数: 0
Abstract
Understanding solar radiation variability is essential for efficiently planning and managing solar energy systems. The transmission of solar radiation to the ground is generally affected by a variety of factors. This research deals with the impacts of weather and air pollution on the amount of diffuse solar radiation across two distinct environments, i.e., urban and peatland areas. Two stations in Jakarta, Kemayoran and Jagakarsa represent the urban area, while two stations in South Kalimantan, Pinang Habang and Jambu, represent the peatland area. Three machine learning-based models were used to estimate the amount of diffuse solar radiation related to weather and air pollution, namely Random Forest (RF), K-nearest neighbor (KNN), and Light Gradient Boosting Machine (LGBM). Five experiments were carried out using various combinations of predictor variables, including temperature, air pollutants, and cloud cover. The results of the experiments highlighted the significance of pollutants as predictive factors. All models demonstrated reliable results in capturing the variability of diffuse solar radiation in four stations, revealing that urban areas receive approximately half the amount of diffuse solar radiation compared to peatland areas, despite sharing a similar annual pattern. Among the models, RF model achieved the highest correlation coefficient with actual values, yielding the least error. Among the sites studied, the predictions from peatland areas closely aligned with the reference pattern. Furthermore, this study found that CO is the primary factor in predicting diffuse solar radiation in urban areas. Differently, PM2.5 mostly impact the diffuse solar radiation in rural areas. This research underscores the critical role of air pollutants, particularly CO and PM2.5, in determining solar radiation levels, which in turn affects the efficiency of solar energy systems.
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.