1. Identity statement | |
Reference Type | Journal Article |
Site | mtc-m21d.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | 8JMKD3MGP3W34T/4B3D8H8 |
Repository | sid.inpe.br/mtc-m21d/2024/04.01.10.58 (restricted access) |
Last Update | 2024:04.01.10.58.22 (UTC) simone |
Metadata Repository | sid.inpe.br/mtc-m21d/2024/04.01.10.58.22 |
Metadata Last Update | 2024:05.15.12.39.03 (UTC) administrator |
DOI | 10.1029/2023GL106282 |
ISSN | 0094-8276 |
Citation Key | WangCSLRLGG:2024:DiDeOn |
Title | Direct Detection of Ongoing Magnetic Reconnection at Mercury's High-Latitude Magnetopause |
Year | 2024 |
Month | Mar. |
Access Date | 2024, May 19 |
Type of Work | journal article |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 8050 KiB |
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2. Context | |
Author | 1 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 Identifier | 1 2 3 4 5 6 7 8 8JMKD3MGP5W/3C9JJC4 |
ORCID | 1 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 |
Group | 1 2 3 4 5 6 7 8 DIHPA-CGCE-INPE-MCTI-GOV-BR |
Affiliation | 1 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 Address | 1 rswan@ustc.edu.cn 2 3 4 5 6 7 8 walter.gonzalez@inpe.br |
Journal | Geophysical Research Letters |
Volume | 51 |
Number | 5 |
Pages | e2023GL106282 |
Secondary Mark | A1_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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | Mercury's magnetosphere magnetic reconnection magnetic flux ropes |
Abstract | An 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Direct Detection of... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | |
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4. Conditions of access and use | |
Language | en |
Target File | Geophysical Research Letters - 2024 - Wang - Direct Detection of Ongoing Magnetic Reconnection at Mercury s High‐Latitude.pdf |
User Group | simone |
Reader Group | administrator simone |
Visibility | shown |
Archiving Policy | denypublisher6 allowfinaldraft |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Mirror Repository | urlib.net/www/2021/06.04.03.40.25 |
Next Higher Units | 8JMKD3MGPCW/46KTFK8 |
Dissemination | WEBSCI; PORTALCAPES; AGU; COMPENDEX; SCOPUS. |
Host Collection | urlib.net/www/2021/06.04.03.40 |
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6. Notes | |
Empty Fields | alternatejournal 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 |
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7. Description control | |
e-Mail (login) | simone |
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