A Reconnecting Current Sheet Imaged in a Solar Flare
Magnetic reconnection changes the magnetic field topology and powers explosive events in astrophysical, space, and laboratory plasmas. For flares and coronal mass ejections (CMEs) in the solar atmosphere, the standard model predicts the presence of a reconnecting current sheet, which has been the su...
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| Published in: | Astrophysical journal. Letters Vol. 723; no. 1; pp. L28 - L33 |
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| Main Authors: | , , , , , |
| Format: | Journal Article |
| Language: | English |
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IOP Publishing
01.11.2010
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| ISSN: | 2041-8205, 2041-8213 |
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| Abstract | Magnetic reconnection changes the magnetic field topology and powers explosive events in astrophysical, space, and laboratory plasmas. For flares and coronal mass ejections (CMEs) in the solar atmosphere, the standard model predicts the presence of a reconnecting current sheet, which has been the subject of considerable theoretical and numerical modeling over the last 50 years, yet direct, unambiguous observational verification has been absent. In this Letter, we show a bright sheet structure of global length (>0.25 R ) and macroscopic width ((5-10)X103 km) distinctly above the cusp-shaped flaring loop, imaged during the flare rising phase in EUV. The sheet formed due to the stretch of a transequatorial loop system and was accompanied by various reconnection signatures. This unique event provides a comprehensive view of the reconnection geometry and dynamics in the solar corona. |
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| AbstractList | Magnetic reconnection changes the magnetic field topology and powers explosive events in astrophysical, space, and laboratory plasmas. For flares and coronal mass ejections (CMEs) in the solar atmosphere, the standard model predicts the presence of a reconnecting current sheet, which has been the subject of considerable theoretical and numerical modeling over the last 50 years, yet direct, unambiguous observational verification has been absent. In this Letter, we show a bright sheet structure of global length (>0.25 R {sub sun}) and macroscopic width ((5-10)x10{sup 3} km) distinctly above the cusp-shaped flaring loop, imaged during the flare rising phase in EUV. The sheet formed due to the stretch of a transequatorial loop system and was accompanied by various reconnection signatures. This unique event provides a comprehensive view of the reconnection geometry and dynamics in the solar corona. Magnetic reconnection changes the magnetic field topology and powers explosive events in astrophysical, space, and laboratory plasmas. For flares and coronal mass ejections (CMEs) in the solar atmosphere, the standard model predicts the presence of a reconnecting current sheet, which has been the subject of considerable theoretical and numerical modeling over the last 50 years, yet direct, unambiguous observational verification has been absent. In this Letter, we show a bright sheet structure of global length (>0.25 R ) and macroscopic width ((5-10)X103 km) distinctly above the cusp-shaped flaring loop, imaged during the flare rising phase in EUV. The sheet formed due to the stretch of a transequatorial loop system and was accompanied by various reconnection signatures. This unique event provides a comprehensive view of the reconnection geometry and dynamics in the solar corona. |
| Author | Liu, Rui Stenborg, Guillermo Lee, Jeongwoo Wang, Tongjiang Wang, Haimin Liu, Chang |
| Author_xml | – sequence: 1 fullname: Liu, Rui – sequence: 2 fullname: Lee, Jeongwoo – sequence: 3 fullname: Wang, Tongjiang – sequence: 4 fullname: Stenborg, Guillermo – sequence: 5 fullname: Liu, Chang – sequence: 6 fullname: Wang, Haimin |
| BackLink | https://www.osti.gov/biblio/21452723$$D View this record in Osti.gov |
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| Snippet | Magnetic reconnection changes the magnetic field topology and powers explosive events in astrophysical, space, and laboratory plasmas. For flares and coronal... |
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| SubjectTerms | ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ATMOSPHERES MAGNETIC FIELDS MAGNETIC RECONNECTION MAIN SEQUENCE STARS PHYSICS SIMULATION SOLAR ACTIVITY SOLAR ATMOSPHERE SOLAR CORONA SOLAR FLARES STARS STELLAR ACTIVITY STELLAR ATMOSPHERES STELLAR CORONAE STELLAR FLARES SUN |
| Title | A Reconnecting Current Sheet Imaged in a Solar Flare |
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