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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/3UGCRBU
Repositorysid.inpe.br/plutao/2019/12.03.13.55.11
Last Update2019:12.05.18.58.43 (UTC) administrator
Metadata Repositorysid.inpe.br/plutao/2019/12.03.13.55.12
Metadata Last Update2021:07.28.22.15.05 (UTC) administrator
DOI10.1029/2019JA026889
ISSN2169-9402
Labellattes: 8026732855379621 3 KogaGoSoCaWaLi:2019:DeSoWi
Citation KeyKogaGoSoCaWaLi:2019:DeSoWi
TitleDayside magnetopause reconnection: its dependence on solar wind and magnetosheath conditions
Year2019
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2663 KiB
2. Context
Author1 Koga, Daiki
2 Gonzalez Alarcon, Walter Demétrio
3 Souza, Vitor Moura Cardoso e Silva
4 Cardoso, Flávia Reis
5 Wang, Chi
6 Liu, Zhengkuan
Resume Identifier1
2 8JMKD3MGP5W/3C9JJC4
ORCID1 0000-0002-4590-2601
2 0000-0002-4859-9310
3 0000-0001-7294-7963
4 0000-0001-7239-0894
5 0000-0001-6991-9398
6 0000-0001-8034-5575
Group1
2 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
3 YYY-CGCEA-INPE-MCTIC-GOV-BR
4 DIDGE-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Chinese Academy of Sciences
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 Chinese Academy of Sciences
6 Chinese Academy of Sciences
JournalJournal of Geophysical Research: Space Physics
Volume124
Pages2019JA026889
History (UTC)2019-12-05 18:58:45 :: lattes -> administrator :: 2019
2021-07-28 22:15:05 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractMagnetic reconnection permits topological rearrangements of the interplanetary and magnetospheric magnetic fields and the entry of solar wind mass, energy, and momentum into the magnetosphere. Thus, magnetic reconnection is a key issue to understand space weather. However, it has not been fully understood yet under which interplanetary/magnetosheath conditions magnetic reconnection takes place more effectively at the dayside magnetopause. In the present study 25 dayside magnetopause reconnection events are investigated using the Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellite observations in order to find its dependence on solar wind and magnetosheath conditions. It is found that the reconnection electric field is proportional to the interplanetary electric field and inversely proportional to the solar wind-Alfvén Mach number and that the reconnection outflow speed is proportional to the solar wind Alfvén speed and inversely proportional to the magnetosheath plasma beta. It is also shown that the range of magnetic shear angles for which magnetic reconnection should occur is restricted to large shears as the magnetosheath flow direction becomes more perpendicular to the direction of the local magnetopause normal vector. Since these results refer to fairly typical solar wind-Alfvén Mach number condition, they may not necessarily apply to more extreme cases.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > Dayside magnetopause reconnection:...
Arrangement 2urlib.net > BDMCI > Fonds > Produção anterior à 2021 > YYY-PCI-CGCEA > Dayside magnetopause reconnection:...
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source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W/3UGCRBU
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W/3UGCRBU
Languageen
Target Filekoga_dayside.pdf
User Grouplattes
Visibilityshown
Archiving Policydenypublisher6 allowfinaldraft
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/4467GD8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.15.01.50 3
sid.inpe.br/bibdigital/2013/10.01.22.11 2
sid.inpe.br/bibdigital/2021/02.11.01.58 1
DisseminationWEBSCI
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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