2005-2035年全球海洋热含量时间序列数据的趋势和变率

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Mehmet Bilgili
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引用次数: 0

摘要

人为温室气体(GHG)排放产生的大约90%的余热被海洋吸收,使海洋热含量(OHC)成为评估气候变化进程的基本指标。对全球和区域两级热含量变化的准确了解,为了解全球变暖的范围及其对海平面上升、天气模式和生态系统的影响提供了宝贵的见解,并有助于完善气候科学的预测。本研究利用季节自回归综合移动平均(SARIMA)方法模拟了主要海洋盆地(全球、南半球、北半球、太平洋、大西洋和印度洋)0-700 m和0-2000 m层的月平均热含量。该研究利用2005年至2023年的数据,提供了2035年的预测。结果表明,SARIMA模型的相关系数(R)在0.8544以上,平均绝对误差(MAE)小于0.932 × 1022 J,均方根误差(RMSE)小于1.222 × 1022 J,趋势精度较高,与实测数据吻合较好。预估到2035年热含量异常的增加突出了持续变暖的趋势,特别是在海洋上层。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Trends and variability in global ocean heat content time series data for the period 2005–2035
Approximately 90 % of the surplus heat generated by anthropogenic greenhouse gas (GHG) emissions is absorbed by the oceans, positioning ocean heat content (OHC) as a fundamental indicator for assessing the progression of climate change. Accurate knowledge of OHC changes at both global and regional levels offers valuable insights into the scope of global warming and its effects on sea-level rise, weather patterns, and ecosystems, and helps refine predictions in climate science. This study models monthly average OHC at 0–700 m and 0–2000 m layers across major ocean basins (Global, Southern Hemisphere, Northern Hemisphere, Pacific, Atlantic, and Indian Oceans) using the Seasonal Autoregressive Integrated Moving Average (SARIMA) method. Utilizing data from 2005 to 2023, the study provides forecasts up to 2035. The results demonstrate that the SARIMA models have correlation coefficients (R) above 0.8544, mean absolute error (MAE) values less than 0.932 × 1022 J, and root mean square error (RMSE) values under 1.222 × 1022 J, indicating highly accurate trends and satisfactory agreement with the observed data. Projected increases in OHC anomalies by 2035 highlight a continued warming trend, particularly in the upper ocean layers.
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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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