Chatzopoulou Anthi, Tourpali K, Bais A F, Braesicke P
Laboratory of Atmospheric Physics, Physics Department, Aristotle University of Thessaloniki, Thessaloniki, Greece.
Institute of Meteorology and Climate Research Atmospheric Trace Gases and Remote Sensing, Karlsruhe Institute of Technology, Karlsruhe, Germany.
Photochem Photobiol Sci. 2025 Jan;24(1):113-130. doi: 10.1007/s43630-024-00676-6. Epub 2024 Dec 24.
This paper investigates the evolution of changes in surface ultraviolet (UV) radiation globally, emphasizing the significant impacts of key factors influencing its variability, i.e., total column ozone, aerosols, clouds, and surface reflectivity. Simulations of UV radiation were performed by the UVSPEC radiative transfer model and span from the mid-twentieth century to the end of the twenty-first century. Input data were derived from eleven Earth System Models that participated in the 6th Phase of the Coupled Model Intercomparison Project (CMIP6). The UV Index (UVI) simulations for the late twentieth century indicate an increase in UVI levels relative to the 1950s in the Southern Hemisphere's mid and high latitudes, attributed to ozone depletion, and decreases in southeastern Asia due to increases in aerosols. Projections of changes in UVI for the last decade of the twenty-first century were derived for three Shared Socioeconomic Pathways (SSPs): SSP1-2.6, SSP3-7.0, and SSP5-8.5. Under SSP1-2.6, the scenario with the lowest greenhouse gas (GHG) and aerosol emissions, UVI is projected to increase relative to the 1950s by up to 20% in Europe and North America and to decrease by as much as - 10% over tropical and polar regions. Under SSP3-7.0 and SSP5-8.5, scenarios with higher GHG and aerosol emissions, UVI changes are generally negative globally due to ozone recovery and increases in aerosol optical depth, while localized positive changes are found over Central and South America, Europe, Africa, and the Pacific and Indian Oceans. The changes in the biologically effective solar irradiance for plant growth exhibit similar geographical patterns to UVI with slight differences, due to weaker sensitivity to changes in ozone.
本文研究了全球地表紫外线(UV)辐射变化的演变情况,强调了影响其变率的关键因素,即总臭氧柱、气溶胶、云和气表反射率的重大影响。利用UVSPEC辐射传输模型对紫外线辐射进行了模拟,时间跨度从20世纪中叶到21世纪末。输入数据来自参与耦合模式比较计划第6阶段(CMIP6)的11个地球系统模型。20世纪后期的紫外线指数(UVI)模拟表明,南半球中高纬度地区的UVI水平相对于20世纪50年代有所增加,这归因于臭氧损耗,而东南亚地区由于气溶胶增加而下降。针对三种共享社会经济路径(SSP)得出了21世纪最后十年UVI变化的预测结果:SSP1-2.6、SSP3-7.0和SSP5-8.5。在温室气体(GHG)和气溶胶排放最低的SSP1-2.6情景下,预计欧洲和北美的UVI相对于20世纪50年代将增加高达20%,而热带和极地地区将下降多达-10%。在GHG和气溶胶排放较高的SSP3-7.0和SSP5-8.5情景下,由于臭氧恢复和气溶胶光学厚度增加,全球UVI变化总体为负,而在中美洲、南美洲、欧洲、非洲以及太平洋和印度洋发现了局部正变化。由于对臭氧变化的敏感性较弱,植物生长的生物有效太阳辐照度变化呈现出与UVI相似但略有不同的地理模式。