中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The evolution of geomagnetotail magnetic flux in isolated substorms

文献类型:期刊论文

作者Yang, Y. Y.1,2; Shen, C.3; Rong, Z. J.4,5; Dunlop, M.6,7; Shen, X. H.1,2; Huang, J. P.1,2; Chen, Z. Q.8
刊名JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS
出版日期2017-11-01
卷号164页码:163-171
关键词Geomagnetotail Magnetic Flux Magnetospheric Energy Substorm Energy Isolated Substorm
ISSN号1364-6826
DOI10.1016/j.jastp.2017.08.016
文献子类Article
英文摘要The magnetic field energy stored in geomagnetotail released during a substorm period, cause significant magnetic disturbance of the space environment. The quantitative relationship between the magnetic field energy and the level of substorm activity, however, is still unclear, although many studies have qualitatively revealed the correlation between them. Here, using data from four selected isolated substorm cases, the evolution of the magnetic flux (MF) in the magnetotail observed by Cluster is quantitatively surveyed. The results from the four cases demonstrate that the evolution of magnetotail MF is closely related to the phases of substorm development. For quiet time, the magnetotail is in the ground state with ME being about 0.6 GWb. During the growth phase, however, as the substonn develop the MF keeps increasing, the substorm onset is triggered when the MF has increased up to some threshold. The comparison between the four cases shows that the accumulation of more magnetic field energy corresponds to more released energy, and consistently, the more intense a substorm can be powered. The study also finds that there is an imbalance between the increased and decreased MF amplitude, indicating that the substorm may not be the only way to release the stored magnetotail energy.
WOS关键词POLAR-CAP AREA ; SOLAR-WIND ; BOUNDARY MOTION ; ENERGY BUDGET ; MAGNETOTAIL ; MAGNETOPAUSE ; GROWTH
WOS研究方向Geochemistry & Geophysics ; Meteorology & Atmospheric Sciences
语种英语
WOS记录号WOS:000417671000017
出版者PERGAMON-ELSEVIER SCIENCE LTD
资助机构Institute of Crustal Dynamics, China Earthquake Administration(ZDJ2017-22 ; Institute of Crustal Dynamics, China Earthquake Administration(ZDJ2017-22 ; National Natural Science Foundation of China(41231066 ; National Natural Science Foundation of China(41231066 ; ISSI ; ISSI ; ZDJ2016-19) ; ZDJ2016-19) ; 41204117) ; 41204117) ; Institute of Crustal Dynamics, China Earthquake Administration(ZDJ2017-22 ; Institute of Crustal Dynamics, China Earthquake Administration(ZDJ2017-22 ; National Natural Science Foundation of China(41231066 ; National Natural Science Foundation of China(41231066 ; ISSI ; ISSI ; ZDJ2016-19) ; ZDJ2016-19) ; 41204117) ; 41204117) ; Institute of Crustal Dynamics, China Earthquake Administration(ZDJ2017-22 ; Institute of Crustal Dynamics, China Earthquake Administration(ZDJ2017-22 ; National Natural Science Foundation of China(41231066 ; National Natural Science Foundation of China(41231066 ; ISSI ; ISSI ; ZDJ2016-19) ; ZDJ2016-19) ; 41204117) ; 41204117) ; Institute of Crustal Dynamics, China Earthquake Administration(ZDJ2017-22 ; Institute of Crustal Dynamics, China Earthquake Administration(ZDJ2017-22 ; National Natural Science Foundation of China(41231066 ; National Natural Science Foundation of China(41231066 ; ISSI ; ISSI ; ZDJ2016-19) ; ZDJ2016-19) ; 41204117) ; 41204117)
源URL[http://ir.iggcas.ac.cn/handle/132A11/82270]  
专题中国科学院地质与地球物理研究所
通讯作者Yang, Y. Y.
作者单位1.China Earthquake Adm, Inst Crustal Dynam, Beijing 100085, Peoples R China
2.China Earthquake Adm, Key Lab Crustal Dynam, Beijing 100085, Peoples R China
3.Harbin Inst Technol, Shenzhen 518055, Peoples R China
4.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing 100029, Peoples R China
5.Univ Chinese Acad Sci, Coll Earth Sci, Beijing, Peoples R China
6.Beihang Univ, Sch Astronaut, Space Sci Inst, Beijing 100191, Peoples R China
7.RAL, Chilton OX11 0QX, Oxon, England
8.Chinese Acad Sci, Natl Space Sci Ctr, Beijing 100190, Peoples R China
推荐引用方式
GB/T 7714
Yang, Y. Y.,Shen, C.,Rong, Z. J.,et al. The evolution of geomagnetotail magnetic flux in isolated substorms[J]. JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS,2017,164:163-171.
APA Yang, Y. Y..,Shen, C..,Rong, Z. J..,Dunlop, M..,Shen, X. H..,...&Chen, Z. Q..(2017).The evolution of geomagnetotail magnetic flux in isolated substorms.JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS,164,163-171.
MLA Yang, Y. Y.,et al."The evolution of geomagnetotail magnetic flux in isolated substorms".JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS 164(2017):163-171.

入库方式: OAI收割

来源:地质与地球物理研究所

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