A Radial Standing Pc5-6 Wave and Its Energy Coupling With Field Line Resonance Within the Dusk-Sector Magnetosphere
文献类型:期刊论文
作者 | Zhou, Yi-Jia6,9; He, Fei6,9; Zhang, Xiao-Xin7; Archer, Martin O.5; Lin, Yu4; Ma, Han6,9; Tian, An-Min2; Yao, Zhong-Hua6,9; Wei, Yong6,9; Ni, Binbin1 |
刊名 | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS |
出版日期 | 2023-10-01 |
卷号 | 128期号:10页码:12 |
ISSN号 | 2169-9380 |
关键词 | ultra-low frequency (ULF) wave standing wave field line resonance (FLR) Magnetosheath Fluctuation |
DOI | 10.1029/2023JA031835 |
英文摘要 | Global ultra-low frequency (ULF) oscillations are believed to play a significant role in the mass, energy, and momentum transport within the Earth's magnetosphere. In this letter, we observe a similar to 1.2 mHz radial standing wave in the dusk-sector magnetosphere accompanied by the field line resonance (FLR) on 16 July 2017. The frequency estimation from the simple box model also confirms the radial standing wave. The essential characteristics of FLR are concurrently identified at the dusk-sector magnetosphere and the conjugated ground location. Further, the radial standing wave dissipates energy into upper atmosphere to enhance the local aurora by coupling itself to the FLR. The magnetospheric dominant 1.2/1.1 mHz ULF waves plausibly correspond well with the discrete similar to 1 mHz magnetosheath ion dynamic pressure/velocity oscillation, suggesting this radial standing wave and FLR in the flank magnetosphere may be triggered by the solar-wind and/or magnetosheath dynamic pressure/velocity fluctuations. Just like thumping the strings, the Earth's magnetic field line can also be disturbed by the external impulses or internal instability, generating the rich ultra-low frequency (ULF) oscillations with period of 1-1,000 s. They are believed to play a significant role in the mass, energy, and momentum transport within the Earth's magnetosphere. But the question of how an external driving mechanism can produce field line disturbances deep inside the magnetosphere is a topic of much debate. One classical global mode resonance model suggests that the magnetospheric space sometimes acts as a huge closed or semi-closed cavity, where the ULF waves form the radial standing wave structure. So far, the observational evidence of radial standing waves with period of above 8 min accompanied by the field line disturbance in the flank magnetosphere is sparse. In this letter, we report a radial standing wave with period of similar to 14 min within dusk-sector magnetosphere accompanied by the field line disturbance phenomenon by multiple-satellite observations. The radial standing wave energy sinks down to upper atmosphere to light the local aurora by coupling itself to the field line resonance. We conclude the radial standing wave may be caused by the solar-wind and/or magnetosheath dynamic pressure/velocity fluctuations. A radial standing Pc5-6 ultra-low frequency wave is identified within the dusk-sector magnetosphereRadial standing wave dissipates energy into upper atmosphere by coupling itself to the field line resonanceSolar-wind and/or magnetosheath dynamic pressure/velocity fluctuations possibly trigger this radial standing wave |
WOS关键词 | PERIOD MAGNETIC PULSATIONS ; ULF PULSATIONS ; EXCITATION ; OSCILLATIONS ; MAGNETOPAUSE ; DRIVEN ; CAVITY ; MODES ; INSTABILITY ; INSTRUMENT |
资助项目 | This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the[42222408] ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the[41931073] ; National Natural Science Foundation of China[2021YFA0718600] ; National Key Ramp;D Program of China[Y2021027] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences[IGGCAS-201904] ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences[EP/T01735X/1] ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship[NAS5-02099] ; NASA |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | AMER GEOPHYSICAL UNION |
WOS记录号 | WOS:001075772200001 |
资助机构 | This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; NASA ; NASA ; NASA ; NASA ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; NASA ; NASA ; NASA ; NASA ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; NASA ; NASA ; NASA ; NASA ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; This work was supported by the National Natural Science Foundation of China (42222408, 41931073), the National Key Ramp;D Program of China (2021YFA0718600), the Youth Innovation Promotion Association of the Chinese Academy of Sciences (No. Y2021027), the ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; National Key Ramp;D Program of China ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology amp; Geophysics, Chinese Academy of Sciences ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; UKRI (STFC/EPSRC) Stephen Hawking Fellowship ; NASA ; NASA ; NASA ; NASA |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/110812] |
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 | He, Fei |
作者单位 | 1.Wuhan Univ, Sch Elect Informat, Dept Space Phys, Wuhan, Peoples R China 2.Shandong Univ, Sch Space Sci & Phys, Weihai, Peoples R China 3.Beihang Univ, Sch Space & Environm, Beijing, Peoples R China 4.Auburn Univ, Phys Dept, Auburn, AL USA 5.Imperial Coll London, Dept Phys, Space & Atmospher Phys Grp, London, England 6.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China 7.China Meteorol Adm, Natl Ctr Space Weather, Key Lab Space Weather, Beijing, Peoples R China 8.Peking Univ, Inst Space Phys & Appl Technol, Beijing, Peoples R China 9.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | Zhou, Yi-Jia,He, Fei,Zhang, Xiao-Xin,et al. A Radial Standing Pc5-6 Wave and Its Energy Coupling With Field Line Resonance Within the Dusk-Sector Magnetosphere[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2023,128(10):12. |
APA | Zhou, Yi-Jia.,He, Fei.,Zhang, Xiao-Xin.,Archer, Martin O..,Lin, Yu.,...&Pu, Zu-Yin.(2023).A Radial Standing Pc5-6 Wave and Its Energy Coupling With Field Line Resonance Within the Dusk-Sector Magnetosphere.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,128(10),12. |
MLA | Zhou, Yi-Jia,et al."A Radial Standing Pc5-6 Wave and Its Energy Coupling With Field Line Resonance Within the Dusk-Sector Magnetosphere".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 128.10(2023):12. |
入库方式: OAI收割
来源:地质与地球物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。