author_facet Pu, Z. Y.
Raeder, J.
Zhong, J.
Bogdanova, Y. V.
Dunlop, M.
Xiao, C. J.
Wang, X. G.
Fazakerley, A.
Pu, Z. Y.
Raeder, J.
Zhong, J.
Bogdanova, Y. V.
Dunlop, M.
Xiao, C. J.
Wang, X. G.
Fazakerley, A.
author Pu, Z. Y.
Raeder, J.
Zhong, J.
Bogdanova, Y. V.
Dunlop, M.
Xiao, C. J.
Wang, X. G.
Fazakerley, A.
spellingShingle Pu, Z. Y.
Raeder, J.
Zhong, J.
Bogdanova, Y. V.
Dunlop, M.
Xiao, C. J.
Wang, X. G.
Fazakerley, A.
Geophysical Research Letters
Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
General Earth and Planetary Sciences
Geophysics
author_sort pu, z. y.
spelling Pu, Z. Y. Raeder, J. Zhong, J. Bogdanova, Y. V. Dunlop, M. Xiao, C. J. Wang, X. G. Fazakerley, A. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1002/grl.50714 <jats:title>Abstract</jats:title><jats:p>Flux transfer events (FTEs) are magnetic flux ropes formed at planetary magnetopauses (MPs). Although evidence suggests that FTEs form through time‐dependent magnetic reconnection, details of that process and 3D structure of the flux ropes remain largely unclear. This letter presents Double Star/TC‐1 data of an FTE occurred on 7 April 2004 which show that the FTE was separated by two X‐lines moving south‐dawnward. In particular, the electron energy‐pitch angle distribution implies that the FTE was composed of flux ropes of all four possible magnetic topologies, indicating that the field lines must have reconnected multiple times. This is an intrinsic property of FTEs formed by 3D multiple X‐line reconnection distinguished from quasi 2D FTE models. This knowledge of FTE magnetic topologies helps to improve our understanding of solar wind‐ magnetosphere coupling at the MP.</jats:p> Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause Geophysical Research Letters
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recordtype ai
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series Geophysical Research Letters
source_id 49
title Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_unstemmed Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_full Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_fullStr Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_full_unstemmed Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_short Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_sort magnetic topologies of an in vivo fte observed by double star/tc‐1 at earth's magnetopause
topic General Earth and Planetary Sciences
Geophysics
url http://dx.doi.org/10.1002/grl.50714
publishDate 2013
physical 3502-3506
description <jats:title>Abstract</jats:title><jats:p>Flux transfer events (FTEs) are magnetic flux ropes formed at planetary magnetopauses (MPs). Although evidence suggests that FTEs form through time‐dependent magnetic reconnection, details of that process and 3D structure of the flux ropes remain largely unclear. This letter presents Double Star/TC‐1 data of an FTE occurred on 7 April 2004 which show that the FTE was separated by two X‐lines moving south‐dawnward. In particular, the electron energy‐pitch angle distribution implies that the FTE was composed of flux ropes of all four possible magnetic topologies, indicating that the field lines must have reconnected multiple times. This is an intrinsic property of FTEs formed by 3D multiple X‐line reconnection distinguished from quasi 2D FTE models. This knowledge of FTE magnetic topologies helps to improve our understanding of solar wind‐ magnetosphere coupling at the MP.</jats:p>
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author Pu, Z. Y., Raeder, J., Zhong, J., Bogdanova, Y. V., Dunlop, M., Xiao, C. J., Wang, X. G., Fazakerley, A.
author_facet Pu, Z. Y., Raeder, J., Zhong, J., Bogdanova, Y. V., Dunlop, M., Xiao, C. J., Wang, X. G., Fazakerley, A., Pu, Z. Y., Raeder, J., Zhong, J., Bogdanova, Y. V., Dunlop, M., Xiao, C. J., Wang, X. G., Fazakerley, A.
author_sort pu, z. y.
container_issue 14
container_start_page 3502
container_title Geophysical Research Letters
container_volume 40
description <jats:title>Abstract</jats:title><jats:p>Flux transfer events (FTEs) are magnetic flux ropes formed at planetary magnetopauses (MPs). Although evidence suggests that FTEs form through time‐dependent magnetic reconnection, details of that process and 3D structure of the flux ropes remain largely unclear. This letter presents Double Star/TC‐1 data of an FTE occurred on 7 April 2004 which show that the FTE was separated by two X‐lines moving south‐dawnward. In particular, the electron energy‐pitch angle distribution implies that the FTE was composed of flux ropes of all four possible magnetic topologies, indicating that the field lines must have reconnected multiple times. This is an intrinsic property of FTEs formed by 3D multiple X‐line reconnection distinguished from quasi 2D FTE models. This knowledge of FTE magnetic topologies helps to improve our understanding of solar wind‐ magnetosphere coupling at the MP.</jats:p>
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id ai-49-aHR0cDovL2R4LmRvaS5vcmcvMTAuMTAwMi9ncmwuNTA3MTQ
imprint American Geophysical Union (AGU), 2013
imprint_str_mv American Geophysical Union (AGU), 2013
institution DE-D275, DE-Bn3, DE-Brt1, DE-Zwi2, DE-D161, DE-Gla1, DE-Zi4, DE-15, DE-Pl11, DE-Rs1, DE-105, DE-14, DE-Ch1, DE-L229
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mega_collection American Geophysical Union (AGU) (CrossRef)
physical 3502-3506
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publisher American Geophysical Union (AGU)
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series Geophysical Research Letters
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spelling Pu, Z. Y. Raeder, J. Zhong, J. Bogdanova, Y. V. Dunlop, M. Xiao, C. J. Wang, X. G. Fazakerley, A. 0094-8276 1944-8007 American Geophysical Union (AGU) General Earth and Planetary Sciences Geophysics http://dx.doi.org/10.1002/grl.50714 <jats:title>Abstract</jats:title><jats:p>Flux transfer events (FTEs) are magnetic flux ropes formed at planetary magnetopauses (MPs). Although evidence suggests that FTEs form through time‐dependent magnetic reconnection, details of that process and 3D structure of the flux ropes remain largely unclear. This letter presents Double Star/TC‐1 data of an FTE occurred on 7 April 2004 which show that the FTE was separated by two X‐lines moving south‐dawnward. In particular, the electron energy‐pitch angle distribution implies that the FTE was composed of flux ropes of all four possible magnetic topologies, indicating that the field lines must have reconnected multiple times. This is an intrinsic property of FTEs formed by 3D multiple X‐line reconnection distinguished from quasi 2D FTE models. This knowledge of FTE magnetic topologies helps to improve our understanding of solar wind‐ magnetosphere coupling at the MP.</jats:p> Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause Geophysical Research Letters
spellingShingle Pu, Z. Y., Raeder, J., Zhong, J., Bogdanova, Y. V., Dunlop, M., Xiao, C. J., Wang, X. G., Fazakerley, A., Geophysical Research Letters, Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause, General Earth and Planetary Sciences, Geophysics
title Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_full Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_fullStr Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_full_unstemmed Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_short Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
title_sort magnetic topologies of an in vivo fte observed by double star/tc‐1 at earth's magnetopause
title_unstemmed Magnetic topologies of an in vivo FTE observed by Double Star/TC‐1 at Earth's magnetopause
topic General Earth and Planetary Sciences, Geophysics
url http://dx.doi.org/10.1002/grl.50714