New progress of Double Star-Cluster joint exploration and study

Zhen Xing Liu; Zu Yin Pu; Jin Bin Cao; Chao Shen; Li Lu; Ling Qian Zhang

doi:10.1007/s11431-008-0267-6

New progress of Double Star-Cluster joint exploration and study

Zhen Xing Liu^*
, Zu Yin Pu
, Jin Bin Cao
, Chao Shen
, Li Lu
, Ling Qian Zhang

^*Corresponding author for this work

CAS - National Space Science Center
Peking University

Research output: Contribution to journal › Article › peer-review

2 Scopus citations

Abstract

The magnetic reconnection of magnetosphere and the magnetospheric space storms (including magnetospheric substorm, magnetic storm, magnetospheric particle storm) has long been one of the most challenging subjects in the solar-terrestrial physics. The reconnection mechanism and global triggering process of the magnetospheric space storms are still unclear up to now. Based on the Double Star Program (DSP) and Cluster joint measurements, we have observed the solar wind density hole, the component magnetic field reconnection in the magnetopause, the structures of magnetic storm ring current, global and multi-scale driven and triggering processes of magnetospheric substorm. In this paper we will briefly introduce these results.

Original language	English
Pages (from-to)	1565-1579
Number of pages	15
Journal	Science in China, Series E: Technological Sciences
Volume	51
Issue number	10
DOIs	https://doi.org/10.1007/s11431-008-0267-6
State	Published - Oct 2008
Externally published	Yes

Keywords

Magnetic reconnection
Magnetic storm
Magnetospheric substorm
Solar wind

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10.1007/s11431-008-0267-6

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title = "New progress of Double Star-Cluster joint exploration and study",

abstract = "The magnetic reconnection of magnetosphere and the magnetospheric space storms (including magnetospheric substorm, magnetic storm, magnetospheric particle storm) has long been one of the most challenging subjects in the solar-terrestrial physics. The reconnection mechanism and global triggering process of the magnetospheric space storms are still unclear up to now. Based on the Double Star Program (DSP) and Cluster joint measurements, we have observed the solar wind density hole, the component magnetic field reconnection in the magnetopause, the structures of magnetic storm ring current, global and multi-scale driven and triggering processes of magnetospheric substorm. In this paper we will briefly introduce these results.",

keywords = "Magnetic reconnection, Magnetic storm, Magnetospheric substorm, Solar wind",

author = "Liu, \{Zhen Xing\} and Pu, \{Zu Yin\} and Cao, \{Jin Bin\} and Chao Shen and Li Lu and Zhang, \{Ling Qian\}",

year = "2008",

month = oct,

doi = "10.1007/s11431-008-0267-6",

language = "英语",

volume = "51",

pages = "1565--1579",

journal = "Science in China, Series E: Technological Sciences",

issn = "1006-9321",

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T1 - New progress of Double Star-Cluster joint exploration and study

AU - Liu, Zhen Xing

AU - Pu, Zu Yin

AU - Cao, Jin Bin

AU - Shen, Chao

AU - Lu, Li

AU - Zhang, Ling Qian

PY - 2008/10

Y1 - 2008/10

N2 - The magnetic reconnection of magnetosphere and the magnetospheric space storms (including magnetospheric substorm, magnetic storm, magnetospheric particle storm) has long been one of the most challenging subjects in the solar-terrestrial physics. The reconnection mechanism and global triggering process of the magnetospheric space storms are still unclear up to now. Based on the Double Star Program (DSP) and Cluster joint measurements, we have observed the solar wind density hole, the component magnetic field reconnection in the magnetopause, the structures of magnetic storm ring current, global and multi-scale driven and triggering processes of magnetospheric substorm. In this paper we will briefly introduce these results.

AB - The magnetic reconnection of magnetosphere and the magnetospheric space storms (including magnetospheric substorm, magnetic storm, magnetospheric particle storm) has long been one of the most challenging subjects in the solar-terrestrial physics. The reconnection mechanism and global triggering process of the magnetospheric space storms are still unclear up to now. Based on the Double Star Program (DSP) and Cluster joint measurements, we have observed the solar wind density hole, the component magnetic field reconnection in the magnetopause, the structures of magnetic storm ring current, global and multi-scale driven and triggering processes of magnetospheric substorm. In this paper we will briefly introduce these results.

KW - Magnetic reconnection

KW - Magnetic storm

KW - Magnetospheric substorm

KW - Solar wind

UR - https://www.scopus.com/pages/publications/51849154767

U2 - 10.1007/s11431-008-0267-6

DO - 10.1007/s11431-008-0267-6

M3 - 文章

AN - SCOPUS:51849154767

SN - 1006-9321

VL - 51

SP - 1565

EP - 1579

JO - Science in China, Series E: Technological Sciences

JF - Science in China, Series E: Technological Sciences

IS - 10

ER -

New progress of Double Star-Cluster joint exploration and study

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Keywords

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