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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/4B3D8H8
Repositorysid.inpe.br/mtc-m21d/2024/04.01.10.58   (restricted access)
Last Update2024:04.01.10.58.22 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2024/04.01.10.58.22
Metadata Last Update2024:05.15.12.39.03 (UTC) administrator
DOI10.1029/2023GL106282
ISSN0094-8276
Citation KeyWangCSLRLGG:2024:DiDeOn
TitleDirect Detection of Ongoing Magnetic Reconnection at Mercury's High-Latitude Magnetopause
Year2024
MonthMar.
Access Date2024, May 19
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size8050 KiB
2. Context
Author1 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
Resume Identifier1
2
3
4
5
6
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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
Group1
2
3
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5
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8 DIHPA-CGCE-INPE-MCTI-GOV-BR
Affiliation1 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)
Author e-Mail Address1 rswan@ustc.edu.cn
2
3
4
5
6
7
8 walter.gonzalez@inpe.br
JournalGeophysical Research Letters
Volume51
Number5
Pagese2023GL106282
Secondary MarkA1_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
History (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. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsMercury's magnetosphere
magnetic reconnection
magnetic flux ropes
AbstractAn 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. Conditions of access and use
Languageen
Target FileGeophysical Research Letters - 2024 - Wang - Direct Detection of Ongoing Magnetic Reconnection at Mercury s High‐Latitude.pdf
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