Temporal and spatial response of Holocene temperature to solar activity
文献类型:期刊论文
作者 | Lu, Wei4,5; Zhao, Xinhua2,3,5; Feng, Xueshang5; Xiang NB(向南彬)1; Du, Zhanle2; Zhang, Wanting4,5 |
刊名 | QUATERNARY INTERNATIONAL |
出版日期 | 2022-03-10 |
卷号 | 613页码:39-45 |
ISSN号 | 1040-6182 |
关键词 | Solar activity Holocene temperature Solar-terrestrial relationship |
DOI | 10.1016/j.quaint.2021.09.006 |
产权排序 | 第5完成单位 |
文献子类 | Article |
英文摘要 | Based on the latest database, we analyze the characteristics of the changing trends of sunspot number (SSN) and temperatures of the global mean surface (GMST) as well as six latitude bands during the Holocene, aiming to explore the long-term responses of the Holocene temperatures to solar activity. We adopt two methods, i.e., the 300-year moving average and the singular spectrum analysis to obtain the long-term trends of signals. We find that the average changes in the amplitude of temperatures in the Northern Hemisphere (NH) (3.65 degrees C) was greater than that in the Southern Hemisphere (SH) (1.28 degrees C) during the entire Holocene. There was one peak of temperatures (at 6500 BP) and two peaks of solar activity (at 4500 BP and 2000 BP) during our study interval. Spatially, the temperatures in the NH were more sensitive to solar forcing than those in the SH, especially in the latitude bands of 0 degrees-30 degrees N and 60 degrees N-90 degrees N. Moreover, the latitude band 0 degrees-30 degrees N had the strongest correlation with solar activity (C.C. = 0.38 for the 300-year moving average and C.C. = 0.55 for the singular spectrum analysis, p < 0.01), while the latitude band 60 degrees S-90 degrees S had the weakest correlation with solar activity (not significant in the statistical sense). Regarding the time response, solar forcing nearly did not affect the terrestrial temperatures in the early Holocene (8700 BP-6500 BP). While positive correlations started to be strong since 4500 BP and became stronger during 2000 BP-100 BP. All in all, the terrestrial temperatures were consistent with solar activity in the long-term trend during the Holocene, especially in the NH. Although many mysteries in historical climate reconstructions remain un-resolved, evaluating the impact of solar force on terrestrial temperature is crucial to reconstruct and predict terrestrial climate. Much deeper specific research on solarterrestrial mechanisms deserves to be put on the agenda. |
学科主题 | 天文学 ; 太阳与太阳系 |
URL标识 | 查看原文 |
出版地 | THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND |
WOS关键词 | CLIMATE ; CYCLE ; OSCILLATION ; SIGNALS |
资助项目 | Strategic Priority Research Program of Chinese Academy of SciencesChinese Academy of Sciences[XDB 41000000] ; NSFCNational Natural Science Foundation of China (NSFC)[41531073] ; NSFCNational Natural Science Foundation of China (NSFC)[41731067] ; NSFCNational Natural Science Foundation of China (NSFC)[41861164026] ; NSFCNational Natural Science Foundation of China (NSFC)[41874202] ; NSFCNational Natural Science Foundation of China (NSFC)[41474153] ; Youth Innovation Promotion Association of Chinese Academy of Sciences[2016133] ; collaborating research program (CRP) of CAS Key Laboratory of Solar Activity NAO ; Pandeng Program of National Space Science Center, Chinese Academy of Sciences |
WOS研究方向 | Physical Geography ; Geology |
语种 | 英语 |
出版者 | PERGAMON-ELSEVIER SCIENCE LTD |
WOS记录号 | WOS:000740487200004 |
资助机构 | Strategic Priority Research Program of Chinese Academy of SciencesChinese Academy of Sciences[XDB 41000000] ; NSFCNational Natural Science Foundation of China (NSFC)[41531073, 41731067, 41861164026, 41874202, 41474153] ; Youth Innovation Promotion Association of Chinese Academy of Sciences[2016133] ; collaborating research program (CRP) of CAS Key Laboratory of Solar Activity NAO ; Pandeng Program of National Space Science Center, Chinese Academy of Sciences |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/24777] |
专题 | 云南天文台_抚仙湖太阳观测站 |
通讯作者 | Zhao, Xinhua |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, 650011, China 2.CAS Key Laboratory of Solar Activity, National Astronomical Observatories, Beijing, 100101, China; 3.Yading Space Weather Science Center, Daocheng, Ganzi, Sichuan, 627750, China; 4.University of Chinese Academy of Sciences, Beijing, 100049, China; 5.State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China; |
推荐引用方式 GB/T 7714 | Lu, Wei,Zhao, Xinhua,Feng, Xueshang,et al. Temporal and spatial response of Holocene temperature to solar activity[J]. QUATERNARY INTERNATIONAL,2022,613:39-45. |
APA | Lu, Wei,Zhao, Xinhua,Feng, Xueshang,Xiang NB,Du, Zhanle,&Zhang, Wanting.(2022).Temporal and spatial response of Holocene temperature to solar activity.QUATERNARY INTERNATIONAL,613,39-45. |
MLA | Lu, Wei,et al."Temporal and spatial response of Holocene temperature to solar activity".QUATERNARY INTERNATIONAL 613(2022):39-45. |
入库方式: OAI收割
来源:云南天文台
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