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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34T/4B3D8H8
Repositóriosid.inpe.br/mtc-m21d/2024/04.01.10.58   (acesso restrito)
Última Atualização2024:04.01.10.58.22 (UTC) simone
Repositório de Metadadossid.inpe.br/mtc-m21d/2024/04.01.10.58.22
Última Atualização dos Metadados2024:05.15.12.39.03 (UTC) administrator
DOI10.1029/2023GL106282
ISSN0094-8276
Chave de CitaçãoWangCSLRLGG:2024:DiDeOn
TítuloDirect Detection of Ongoing Magnetic Reconnection at Mercury's High-Latitude Magnetopause
Ano2024
MêsMar.
Data de Acesso30 jun. 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho8050 KiB
2. Contextualização
Autor1 Wang, Rongsheng
2 Cheng, Zihang
3 Slavin, James A.
4 Lu, Quanming
5 Raines, Jim
6 Lu, San
7 Guo, Jin
8 Gonzalez Alarcon, Walter Demetrio
Identificador de Curriculo1
2
3
4
5
6
7
8 8JMKD3MGP5W/3C9JJC4
ORCID1 0000-0002-9511-7660
2 0000-0009-8743-3266
3 0000-0002-9206-724X
4 0000-0003-3041-2682
5 0000-0001-5956-9523
6 0000-0003-2248-5072
7 0000-0002-9950-1029
8 0000-0002-4859-9310
Grupo1
2
3
4
5
6
7
8 DIHPA-CGCE-INPE-MCTI-GOV-BR
Afiliação1 Deep Space Exploration Laboratory
2 University of Science and Technology of China
3 University of Michigan
4 Deep Space Exploration Laboratory
5 University of Michigan
6 Deep Space Exploration Laboratory
7 University of Science and Technology of China
8 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1 rswan@ustc.edu.cn
2
3
4
5
6
7
8 walter.gonzalez@inpe.br
RevistaGeophysical Research Letters
Volume51
Número5
Páginase2023GL106282
Nota SecundáriaA1_INTERDISCIPLINAR A1_GEOGRAFIA A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A1_ENGENHARIAS_I A1_CIÊNCIAS_AMBIENTAIS A1_CIÊNCIAS_AGRÁRIAS_I A1_BIODIVERSIDADE A2_QUÍMICA A2_ENGENHARIAS_IV A2_ENGENHARIAS_II A2_CIÊNCIAS_BIOLÓGICAS_I B1_ASTRONOMIA_/_FÍSICA B2_ENSINO
Histórico (UTC)2024-04-01 10:58:22 :: simone -> administrator ::
2024-04-01 10:58:25 :: administrator -> simone :: 2024
2024-04-01 10:59:35 :: simone -> administrator :: 2024
2024-05-15 12:39:03 :: administrator -> simone :: 2024
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-ChaveMercury's magnetosphere
magnetic reconnection
magnetic flux ropes
ResumoAn ongoing magnetic reconnection event was detected in the Mercury's high latitude magnetopause during a northward interplanetary magnetic field. The reconnection X-line region was revealed in the Mercury's magnetopause based on the encountered flux ropes ejected away from this region both planetward and tailward. A series of magnetic flux ropes, known as flux transfer event shower were observed tailward of this X-line region. These flux ropes were probably expanding and deflected as they were ejected away tailward from the X-line region. Large-amplitude variations in all three components of the magnetic field and a few small-scale flux ropes were observed inside the X-line region, which could be the seed of the flux rope shower at the magnetopause. The observations suggest that magnetic reconnection is highly dynamic and persistent in Mercury's magnetosphere. Magnetic reconnection has been regarded as the most important process for dynamics of the Mercury's magnetosphere and for the interaction between the solar wind and the Mercury's magnetosphere also. Although magnetic flux ropes and flux transfer events (FTEs) resulting from magnetic reconnection have been extensively observed in the Mercury's magnetosphere, the key region of magnetic reconnection, namely the X-line region, has never been reported so far by the spacecraft. Here, we present the first evidence of the reconnection X-line region in the Mercury's magnetosphere. A few small-scale magnetic flux ropes are observed inside the reconnection X-line region, which could be the seed of the observed magnetic FTE shower. Furthermore, the evolution of these flux ropes is addressed also based on the spacecraft observations. A reconnection X-line region is first observed in the Mercury's magnetopause during the northward interplanetary magnetic field The small-scale magnetic flux ropes in the X-line region could be the seed of the flux transfer event shower The flux ropes probably expand and is deflected after they are ejected away from the X-line region.
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4. Condições de acesso e uso
Idiomaen
Arquivo AlvoGeophysical Research Letters - 2024 - Wang - Direct Detection of Ongoing Magnetic Reconnection at Mercury s High‐Latitude.pdf
Grupo de Usuáriossimone
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Política de Arquivamentodenypublisher6 allowfinaldraft
Permissão de Leituradeny from all and allow from 150.163
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5. Fontes relacionadas
Repositório Espelhourlib.net/www/2021/06.04.03.40.25
Unidades Imediatamente Superiores8JMKD3MGPCW/46KTFK8
DivulgaçãoWEBSCI; PORTALCAPES; AGU; COMPENDEX; SCOPUS.
Acervo Hospedeirourlib.net/www/2021/06.04.03.40
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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