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
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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 |
DOI | 10.1029/2023JA031445 |
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. |
入库方式: OAI收割
来源:地质与地球物理研究所
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