Simulating the Solar Wind-Magnetosphere Interaction During the Matuyama-Brunhes Paleomagnetic Reversal
文献类型:期刊论文
作者 | Gong, Fan1,2; Yu, Yiqun1,2; Cao, Jinbin1,2; Wei, Yong3; Gao, Jiawei3; Li, Hui4; Zhang, Binzheng5; Ridley, Aaron6 |
刊名 | GEOPHYSICAL RESEARCH LETTERS
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出版日期 | 2022-02-16 |
卷号 | 49期号:3页码:10 |
关键词 | solar wind-magnetosphere Interaction paleomagnetic reversal |
ISSN号 | 0094-8276 |
DOI | 10.1029/2021GL097340 |
英文摘要 | During a paleomagnetic reversal, Earth's geomagnetic field is about 10% of today's magnitude and its topology is far more complex than dipolar. Revealing the solar wind energy transmission during the reversal is of importance for understanding the historic space environment. Using a global magnetohydrodynamic model implemented with a data-reconstructed time-dependent paleomagnetic field, this study simulates the solar wind-magnetosphere interactions during the last Matuyama-Brunhes reversal that occurred about 780,000 years ago. As the magnetosphere shrinks in the midst of the reversal, the stand-off distance of the subsolar magnetopause approaches as close as 3 Re. Moreover, multiple magnetic reconnection sites emerge due to the irregular geomagnetic configuration, opening up many channels on the magnetopause surface for the solar wind to directly access. The power transmission efficiency through the magnetopause increases to 18%. |
WOS关键词 | FIELD ; MAGNETOPAUSE ; ENERGY ; MASS ; EVOLUTION ; GEODYNAMO ; SPHERE ; STORM |
资助项目 | NSFC[41821003] ; NSFC[41974192] ; B-type Strategic Priority Program of the Chinese Academy of Sciences[XDB41000000] ; China's National Space Administration (CNSA)[D020103] ; China's National Space Administration (CNSA)[D020105] |
WOS研究方向 | Geology |
语种 | 英语 |
WOS记录号 | WOS:000759485200057 |
出版者 | AMER GEOPHYSICAL UNION |
资助机构 | NSFC ; NSFC ; NSFC ; NSFC ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; NSFC ; NSFC ; NSFC ; NSFC ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; NSFC ; NSFC ; NSFC ; NSFC ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; NSFC ; NSFC ; NSFC ; NSFC ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) ; China's National Space Administration (CNSA) |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/104947] ![]() |
专题 | 地质与地球物理研究所_中国科学院地球与行星物理重点实验室 |
通讯作者 | Yu, Yiqun; Cao, Jinbin; Wei, Yong |
作者单位 | 1.Beihang Univ, Sch Space & Environm, Beijing, Peoples R China 2.Minist Ind & Informat Technol, Key Lab Space Environm Monitoring & Informat Proc, Beijing, Peoples R China 3.Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China 4.Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China 5.Univ Hong Kong, Dept Earth Sci, Hong Kong, Peoples R China 6.Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA |
推荐引用方式 GB/T 7714 | Gong, Fan,Yu, Yiqun,Cao, Jinbin,et al. Simulating the Solar Wind-Magnetosphere Interaction During the Matuyama-Brunhes Paleomagnetic Reversal[J]. GEOPHYSICAL RESEARCH LETTERS,2022,49(3):10. |
APA | Gong, Fan.,Yu, Yiqun.,Cao, Jinbin.,Wei, Yong.,Gao, Jiawei.,...&Ridley, Aaron.(2022).Simulating the Solar Wind-Magnetosphere Interaction During the Matuyama-Brunhes Paleomagnetic Reversal.GEOPHYSICAL RESEARCH LETTERS,49(3),10. |
MLA | Gong, Fan,et al."Simulating the Solar Wind-Magnetosphere Interaction During the Matuyama-Brunhes Paleomagnetic Reversal".GEOPHYSICAL RESEARCH LETTERS 49.3(2022):10. |
入库方式: OAI收割
来源:地质与地球物理研究所
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