Evidence of guide field magnetic reconnection in flapping current sheets
Based on current sheet flapping motion on 27 August 2018 in the dusk flank magnetotail, as recorded by instruments aboard Magnetospheric Multiscale (MMS) spacecraft, we present the first study of guide field reconnection observed in the flux rope embedded in kink-like flapping current sheets near th...
| Published in: | Earth and Planetary Physics |
|---|---|
| Main Authors: | , , , |
| Format: | Article |
| Language: | English |
| Published: |
Science Press
2024-07-01
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| Subjects: | |
| Online Access: | http://www.eppcgs.org/article/doi/10.26464/epp2024035?pageType=en |
| _version_ | 1850290499841163264 |
|---|---|
| author | YunTian Hou SuPing Duan Lei Dai Chi Wang |
| author_facet | YunTian Hou SuPing Duan Lei Dai Chi Wang |
| author_sort | YunTian Hou |
| collection | DOAJ |
| container_title | Earth and Planetary Physics |
| description | Based on current sheet flapping motion on 27 August 2018 in the dusk flank magnetotail, as recorded by instruments aboard Magnetospheric Multiscale (MMS) spacecraft, we present the first study of guide field reconnection observed in the flux rope embedded in kink-like flapping current sheets near the dusk-side flank of the magnetotail. Unlike more common magnetotail reconnections, which are symmetric, these asymmetric small-scale (λi ~ 650 km) reconnections were found in the highly twisted current sheet when the direction normal to the sheet changes from the Z direction into the Y direction. The unique feature of this unusual reconnection is that the reconnection jets are along the Z direction — different from outflow in the X direction, which is the more usual situation. This vertical reconnection jet is parallel or antiparallel to the up-and-down motion of the tail’s current sheet. The normalized reconnection rate R is estimated to be ~ 0.1. Our results indicate that such asymmetric reconnections can significantly enlarge current sheet flapping, with large oscillation amplitudes. This letter presents direct evidence of guide field reconnection in a highly twisted current sheet, characterized by enlarged current sheet flapping as a consequence of the reconnection outflow. |
| format | Article |
| id | doaj-art-e8a786e1a5c846e5ae5bfb1ddb2e42dc |
| institution | Directory of Open Access Journals |
| issn | 2096-3955 |
| language | English |
| publishDate | 2024-07-01 |
| publisher | Science Press |
| record_format | Article |
| spelling | doaj-art-e8a786e1a5c846e5ae5bfb1ddb2e42dc2025-08-19T23:35:35ZengScience PressEarth and Planetary Physics2096-39552024-07-018465065810.26464/epp2024035RA482-houyuntian-dusuping-FEvidence of guide field magnetic reconnection in flapping current sheetsYunTian Hou0SuPing Duan1Lei Dai2Chi Wang3State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, ChinaState Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, ChinaState Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, ChinaState Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, ChinaBased on current sheet flapping motion on 27 August 2018 in the dusk flank magnetotail, as recorded by instruments aboard Magnetospheric Multiscale (MMS) spacecraft, we present the first study of guide field reconnection observed in the flux rope embedded in kink-like flapping current sheets near the dusk-side flank of the magnetotail. Unlike more common magnetotail reconnections, which are symmetric, these asymmetric small-scale (λi ~ 650 km) reconnections were found in the highly twisted current sheet when the direction normal to the sheet changes from the Z direction into the Y direction. The unique feature of this unusual reconnection is that the reconnection jets are along the Z direction — different from outflow in the X direction, which is the more usual situation. This vertical reconnection jet is parallel or antiparallel to the up-and-down motion of the tail’s current sheet. The normalized reconnection rate R is estimated to be ~ 0.1. Our results indicate that such asymmetric reconnections can significantly enlarge current sheet flapping, with large oscillation amplitudes. This letter presents direct evidence of guide field reconnection in a highly twisted current sheet, characterized by enlarged current sheet flapping as a consequence of the reconnection outflow.http://www.eppcgs.org/article/doi/10.26464/epp2024035?pageType=enmagnetic reconnectionmagnetotailcurrent sheet |
| spellingShingle | YunTian Hou SuPing Duan Lei Dai Chi Wang Evidence of guide field magnetic reconnection in flapping current sheets magnetic reconnection magnetotail current sheet |
| title | Evidence of guide field magnetic reconnection in flapping current sheets |
| title_full | Evidence of guide field magnetic reconnection in flapping current sheets |
| title_fullStr | Evidence of guide field magnetic reconnection in flapping current sheets |
| title_full_unstemmed | Evidence of guide field magnetic reconnection in flapping current sheets |
| title_short | Evidence of guide field magnetic reconnection in flapping current sheets |
| title_sort | evidence of guide field magnetic reconnection in flapping current sheets |
| topic | magnetic reconnection magnetotail current sheet |
| url | http://www.eppcgs.org/article/doi/10.26464/epp2024035?pageType=en |
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