{"title":"2005-2035年全球海洋热含量时间序列数据的趋势和变率","authors":"Mehmet Bilgili","doi":"10.1016/j.jastp.2025.106586","DOIUrl":null,"url":null,"abstract":"<div><div>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 × 10<sup>22</sup> J, and root mean square error (RMSE) values under 1.222 × 10<sup>22</sup> 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.</div></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"274 ","pages":"Article 106586"},"PeriodicalIF":1.9000,"publicationDate":"2025-06-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Trends and variability in global ocean heat content time series data for the period 2005–2035\",\"authors\":\"Mehmet Bilgili\",\"doi\":\"10.1016/j.jastp.2025.106586\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>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 × 10<sup>22</sup> J, and root mean square error (RMSE) values under 1.222 × 10<sup>22</sup> 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.</div></div>\",\"PeriodicalId\":15096,\"journal\":{\"name\":\"Journal of Atmospheric and Solar-Terrestrial Physics\",\"volume\":\"274 \",\"pages\":\"Article 106586\"},\"PeriodicalIF\":1.9000,\"publicationDate\":\"2025-06-24\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Atmospheric and Solar-Terrestrial Physics\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S1364682625001701\",\"RegionNum\":4,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682625001701","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
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.
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.