Wan Li , Hujia Zhao , Changshuang Wang , Peng Wang , Dong Han , Chengyu Wang , Wenjing Yuan , Shuanglu Bo
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引用次数: 0
Abstract
Air pollution, particularly fine particulate matter (PM2.5), poses severe environmental and public health challenges. Understanding the complex interactions between PM2.5 concentrations and meteorological factors is crucial for effective air quality management and policy development. However, existing predictive models often struggle to capture the nonlinear and spatiotemporal dependencies of PM2.5 variations, limiting their interpretability and accuracy. To address these gaps, this study developed a machine learning-based model using extensive historical environmental and meteorological data to analyze the nonlinear response of near-surface PM2.5 concentrations to multiple spatiotemporal drivers. A monthly-scale prediction model was established, integrating CMIP6 climate projections under different emission scenarios, projected emission inventories, and multi-source auxiliary data. The findings reveal that PM2.5 concentrations are highest in winter and lowest in summer, with significant seasonal and regional variations from 2015 to 2023. The model demonstrated strong predictive performance, particularly over the North China Plain and Northeast urban agglomerations (R = 0.825), though performance was weaker over the Tibetan Plateau. Key meteorological factors influencing PM2.5 concentrations include specific humidity, 500 hPa wind, and short-wave radiation. Under future climate scenarios, PM2.5 concentrations in South and East China are projected to decline during 2025–2030, while Northern China may experience seasonal increases under low-emission scenarios. Regional climate changes, such as increased precipitation and wind speeds in certain areas, further influence PM2.5 concentration patterns. This study provides a novel, data-driven approach to quantifying the impact of meteorological fluctuations on PM2.5 variations, offering valuable insights for air quality forecasting and policy formulation under different climate scenarios.
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.