中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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
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
DOI10.1029/2021GL097340
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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