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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4AC7R42
Repositorysid.inpe.br/mtc-m21d/2023/12.11.12.18
Metadata Repositorysid.inpe.br/mtc-m21d/2023/12.11.12.18.14
Metadata Last Update2024:01.02.17.16.56 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyDaiHWSGDLRG:2023:PeSM
TitleA phenomenological model of Strongly-Driven Substorms and Magnetosphere Convection: Perspectives for SMILE
Year2023
Access Date2024, May 19
Secondary TypePRE CI
2. Context
Author1 Dai, Lei
2 Han, Yimin
3 Wang, Chi
4 Shuo, Yao
5 Gonzalez Alarcon, Walter Demétrio
6 Duan, Suping
7 Lavraud, Benoit
8 Ren, Yong
9 Guo, Zhenyuan
Resume Identifier1
2
3
4
5 8JMKD3MGP5W/3C9JJC4
Group1
2
3
4
5 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 Chinese Academy of Sciences (CAS)
2 Chinese Academy of Sciences (CAS)
3 Chinese Academy of Sciences (CAS)
4 Chinese Academy of Sciences (CAS)
5 Instituto Nacional de Pesquisas Espaciais (INPE)
6 Chinese Academy of Sciences (CAS)
7 IRAP
8 Chinese Academy of Sciences (CAS)
9 Chinese Academy of Sciences (CAS)
Author e-Mail Address1
2
3
4
5 walter.gonzalez@inpe.br
Conference NameAGU FAll Meeting
Conference LocationSan Francisco, CA
Date11-15 Dec. 2023
PublisherAGU
Book TitleProceedings
History (UTC)2023-12-11 12:18:14 :: simone -> administrator ::
2024-01-02 17:16:56 :: administrator -> simone :: 2023
3. Content and structure
Is the master or a copy?is the master
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Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractUsing solar-wind-magnetosphere-ionosphere conjunction observations, we investigate the geomagnetic responses to fluctuating IMF Bz from interplanetary Alfven waves. Interplanetary Alfven waves transmit intensified IMF Bz to the magnetosheath, leading to intervals of large magnetic shear angles across the magnetopause and magnetopause reconnection. Such intervals are promptly followed by hundreds of nT increases in AE/AU index within 10-20 min. These observations are confirmed in multiple events in corotating interaction region (CIR)-driven geomagnetic storms. To put the observations into context, we propose a phenomenological model of strongly-driven magnetosphere convection/substorm. The substorm electrojet is linked to the enhanced magnetopause reconnection in the short timescale of re-establishing the ionosphere electric field and the two-cell convection. The ionosphere two-cell convection drives enhanced magnetosphere convection that may lead to substorm expansion. These results provide new insights on the temporal patterns of the solarwindmagnetosphere-ionosphere coupling.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > A phenomenological model...
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User Groupsimone
Visibilityshown
Update Permissionnot transferred
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6. Notes
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