中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A Possible Unified Picture for the Connected Recurrent Magnetic Dipolarization, Quasi-Periodic ENA Enhancement, SKR Low-Frequency Extension and Narrowband Emission at Saturn

文献类型:期刊论文

作者Xu, Y.2,3; Yao, Z. H.1,2,3; Ye, S. -Y.4; Badman, S. V.6; Dialynas, K.7; Sergis, N.7,8; Ray, L. C.6; Guo, R. L.9; Pan, D. X.5; Dunn, W. R.
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
出版日期2023-09-01
卷号128期号:9页码:11
关键词ENA dipolarization SKR narrow band emission partial ring current
ISSN号2169-9380
DOI10.1029/2023JA031445
英文摘要Magnetic Dipolarization, a hallmark indicator of the formation of field-aligned currents, plays a crucial role in the energy dissipative processes that occur within planetary magnetospheres. Saturn's magnetic dipolarization was found to recur after one planetary rotation, suggesting a potential correlation with the corotating current systems. The observation of enhanced Energetic Neutral Atoms (ENA) within Saturn's inner magnetosphere serves as a diagnostic tool, revealing the existence of a rotating, dynamic Partial Ring Current (PRC) system. By utilizing multiple datasets from Cassini, this study advances the understanding of the interrelationship between ENA emission and magnetic dipolarization. Our results suggest the possibility of a coupling between the PRC system revealed by the ENA emission and magnetic dipolarization. Furthermore, a temporal correlation was found between the ENA emissions and two distinct radio emissions. This study discusses potential causal relationships among these phenomena and first time proposes a global unified physical picture.
WOS关键词RADIO EMISSIONS ; TERRESTRIAL ; MAGNETOSPHERE ; RADIATION ; EARTH ; RECONNECTION ; MODEL ; MIMI
资助项目This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con[IGGCAS-201904] ; National Natural Science Foundation of China[NAS5 97271] ; Key Research Program of the Institute of Geology and Geophysics, CAS[NNX07AJ69~G] ; Key Research Program of the Institute of Geology and Geophysics, CAS[NNN06AA01C] ; Key Research Program of the Institute of Geology and Geophysics, CAS[ST/V000748/1] ; NASA[ST/M005534/1] ; STFC ; [42074211]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001057900000001
出版者AMER GEOPHYSICAL UNION
资助机构This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; NASA ; NASA ; NASA ; NASA ; STFC ; STFC ; STFC ; STFC ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; NASA ; NASA ; NASA ; NASA ; STFC ; STFC ; STFC ; STFC ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; NASA ; NASA ; NASA ; NASA ; STFC ; STFC ; STFC ; STFC ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; This work was supported by National Natural Science Foundation of China Grants 42074211, Key Research Program of the Institute of Geology and Geophysics, CAS, Grant IGGCAS-201904. The work at the Academy of Athens was supported at JHU/APL by NASA under con ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; Key Research Program of the Institute of Geology and Geophysics, CAS ; NASA ; NASA ; NASA ; NASA ; STFC ; STFC ; STFC ; STFC
源URL[http://ir.iggcas.ac.cn/handle/132A11/111441]  
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Yao, Z. H.
作者单位1.UCL Mullard Space Sci Lab, Dorking, England
2.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
3.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China
4.Southern Univ Sci & Technol SUSTech, Dept Earth & Space Sci, Shenzhen, Peoples R China
5.China Univ Geosci Beijing, Sch Geophys & Informat Technol, Beijing, Peoples R China
6.Univ Lancaster, Dept Phys, Lancaster, England
7.Acad Athens, Off Space Res & Technol, Athens, Greece
8.Inst Space Applicat & Remote Sensing, Natl Observ Athens, Athens, Greece
9.Shandong Univ, Inst Space Sci, Sch Space Sci & Phys, Lab Opt Astron & Solar Terr Environm, Weihai, Peoples R China
10.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
推荐引用方式
GB/T 7714
Xu, Y.,Yao, Z. H.,Ye, S. -Y.,et al. A Possible Unified Picture for the Connected Recurrent Magnetic Dipolarization, Quasi-Periodic ENA Enhancement, SKR Low-Frequency Extension and Narrowband Emission at Saturn[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2023,128(9):11.
APA Xu, Y..,Yao, Z. H..,Ye, S. -Y..,Badman, S. V..,Dialynas, K..,...&Wei, Y..(2023).A Possible Unified Picture for the Connected Recurrent Magnetic Dipolarization, Quasi-Periodic ENA Enhancement, SKR Low-Frequency Extension and Narrowband Emission at Saturn.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,128(9),11.
MLA Xu, Y.,et al."A Possible Unified Picture for the Connected Recurrent Magnetic Dipolarization, Quasi-Periodic ENA Enhancement, SKR Low-Frequency Extension and Narrowband Emission at Saturn".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 128.9(2023):11.

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来源:地质与地球物理研究所

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