IGGCAS OpenIR  > 地球与行星物理院重点实验室
Electron Mirror-mode Structure: Magnetospheric Multiscale Observations
Yao, S. T.1,2; Shi, Q. Q.1; Yao, Z. H.2; Guo, R. L.4; Zong, Q. G.5; Wang, X. G.6; Degeling, A. W.1; Rae, I. J.3; Russell, C. T.7; Tian, A. M.1; Zhang, H.8,9; Hu, H. Q.10; Liu, J.2; Liu, H.5; Li, B.11; Giles, B. L.12
2019-08-20
Source PublicationASTROPHYSICAL JOURNAL LETTERS
ISSN2041-8205
Volume881Issue:2Pages:6
AbstractThe small-scale mirror mode excited by electron dynamics is a fundamental physical process, attracting research interest in space, laboratory, and astrophysical plasma physics over the past half century. However, the investigations of this process were mostly limited to theories and numerical simulations, with no direct observational evidence for their existence. In this study we present clear observations of electron mirror-mode using Magnetospheric Multiscale data at unprecedented high temporal cadence. These structures are train-like, compressible, nonpropagating, and satisfy the theoretical excitation and electron trapping conditions. They were observed near the Earth's foreshock and its downstream turbulence during the corotating interaction region events, which could be involved with the interaction between solar wind and Earth.
DOI10.3847/2041-8213/ab3398
Funding OrganizationNational Natural Science Foundation of China ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF ; PRODEX program ; Belgian Federal Science Policy Office ; National Natural Science Foundation of China ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF ; PRODEX program ; Belgian Federal Science Policy Office ; National Natural Science Foundation of China ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF ; PRODEX program ; Belgian Federal Science Policy Office ; National Natural Science Foundation of China ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF ; PRODEX program ; Belgian Federal Science Policy Office
WOS KeywordFIELD-SWELLING INSTABILITY ; SCALE MAGNETIC HOLES ; MMS OBSERVATIONS ; PLASMA ; MAGNETOSHEATH ; DYNAMICS ; WAVES ; MECHANISM ; CLUSTER
Language英语
Funding ProjectNational Natural Science Foundation of China[41774153] ; National Natural Science Foundation of China[41574157] ; National Natural Science Foundation of China[41674165] ; National Natural Science Foundation of China[41431072] ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF[AGS-1352669] ; PRODEX program ; Belgian Federal Science Policy Office
Funding OrganizationNational Natural Science Foundation of China ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF ; PRODEX program ; Belgian Federal Science Policy Office ; National Natural Science Foundation of China ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF ; PRODEX program ; Belgian Federal Science Policy Office ; National Natural Science Foundation of China ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF ; PRODEX program ; Belgian Federal Science Policy Office ; National Natural Science Foundation of China ; Specialized Research Fund for State Key Laboratories ; International Space Science Institute (ISSI) ; NSF ; PRODEX program ; Belgian Federal Science Policy Office
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000481995700005
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.iggcas.ac.cn/handle/132A11/92979
Collection地球与行星物理院重点实验室
Corresponding AuthorShi, Q. Q.
Affiliation1.Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Inst Space Sci, Weihai 264209, Peoples R China
2.Chinese Acad Sci, State Key Lab Space Weather, Natl Space Sci Ctr, Beijing 100190, Peoples R China
3.Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium
4.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing 100029, Peoples R China
5.Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
6.Harbin Inst Technol, Dept Phys, Harbin 150001, Heilongjiang, Peoples R China
7.Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA USA
8.Univ Alaska Fairbanks, Phys Dept, Fairbanks, AK USA
9.Univ Alaska Fairbanks, Inst Geophys, Fairbanks, AK 99775 USA
10.Polar Res Inst China, SOA Key Lab Polar Sci, Shanghai, Peoples R China
11.Wuhan Univ, Chinese Antarctic Ctr Surveying & Mapping, Wuhan 430079, Hubei, Peoples R China
12.NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
Recommended Citation
GB/T 7714
Yao, S. T.,Shi, Q. Q.,Yao, Z. H.,et al. Electron Mirror-mode Structure: Magnetospheric Multiscale Observations[J]. ASTROPHYSICAL JOURNAL LETTERS,2019,881(2):6.
APA Yao, S. T..,Shi, Q. Q..,Yao, Z. H..,Guo, R. L..,Zong, Q. G..,...&Giles, B. L..(2019).Electron Mirror-mode Structure: Magnetospheric Multiscale Observations.ASTROPHYSICAL JOURNAL LETTERS,881(2),6.
MLA Yao, S. T.,et al."Electron Mirror-mode Structure: Magnetospheric Multiscale Observations".ASTROPHYSICAL JOURNAL LETTERS 881.2(2019):6.
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