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Two interacting X lines in magnetotail : Evolution of collision between the counterstreaming jets. / Alexandrova, Alexandra; Nakamura, Rumi; Panov, Evgeny V.; Sasunov, Yury L.; Nakamura, Takuma; Vörös, Zoltán; Retinò, Alessandro; Semenov, Vladimir S.

In: Geophysical Research Letters, Vol. 43, No. 15, 16.08.2016, p. 7795-7803.

Research output: Contribution to journal › Article › peer-review

Harvard

Alexandrova, A, Nakamura, R, Panov, EV, Sasunov, YL, Nakamura, T, Vörös, Z, Retinò, A & Semenov, VS 2016, 'Two interacting X lines in magnetotail: Evolution of collision between the counterstreaming jets', Geophysical Research Letters, vol. 43, no. 15, pp. 7795-7803. https://doi.org/10.1002/2016GL069823, https://doi.org/10.1002/2016GL069823

APA

Alexandrova, A., Nakamura, R., Panov, E. V., Sasunov, Y. L., Nakamura, T., Vörös, Z., Retinò, A., & Semenov, V. S. (2016). Two interacting X lines in magnetotail: Evolution of collision between the counterstreaming jets. Geophysical Research Letters, 43(15), 7795-7803. https://doi.org/10.1002/2016GL069823, https://doi.org/10.1002/2016GL069823

Vancouver

Alexandrova A, Nakamura R, Panov EV, Sasunov YL, Nakamura T, Vörös Z et al. Two interacting X lines in magnetotail: Evolution of collision between the counterstreaming jets. Geophysical Research Letters. 2016 Aug 16;43(15):7795-7803. https://doi.org/10.1002/2016GL069823, https://doi.org/10.1002/2016GL069823

Author

Alexandrova, Alexandra ; Nakamura, Rumi ; Panov, Evgeny V. ; Sasunov, Yury L. ; Nakamura, Takuma ; Vörös, Zoltán ; Retinò, Alessandro ; Semenov, Vladimir S. / Two interacting X lines in magnetotail : Evolution of collision between the counterstreaming jets. In: Geophysical Research Letters. 2016 ; Vol. 43, No. 15. pp. 7795-7803.

BibTeX

@article{d6da69a2f3c144998de10af5ace7fab4,
title = "Two interacting X lines in magnetotail: Evolution of collision between the counterstreaming jets",
abstract = "We study the process of collision between the counterstreaming jets flowing out from two reconnection sites in the Earth's magnetotail. The X lines, bracketing the region of jets collision, were passing by two Cluster probes successively in tailward direction. Two probes observed two different stages of the collision process. At the jets collision site, a probe first observed an ion-scale current sheet-like structure, while the other probe observed more compressed one later. The strong wave activities on both ion and electron scales were seen within the compressed layer. Such evolution of the jets collision resulting in the formation of the compressed boundary between the active X lines shows an example of interaction between the X lines during multiple reconnection.",
keywords = "jets collision, magnetic reconnection, multiple reconnection",
author = "Alexandra Alexandrova and Rumi Nakamura and Panov, {Evgeny V.} and Sasunov, {Yury L.} and Takuma Nakamura and Zolt{\'a}n V{\"o}r{\"o}s and Alessandro Retin{\`o} and Semenov, {Vladimir S.}",
note = "Funding Information: The research was supported by the Austrian Science Fund (FWF) grant P23862-N16, A.A. and R.N., and grant P24740-N27, Z.V. V.S.S. was supported by the Russian Foundation for Basic Research (RFBR) grant 16-05-0047016. A.A. acknowledges the Cluster Science Archive for use of data presented and Emmanuel Penou for the ion velocity distribution provided by the CLWeb software. A.A. thanks Olga Alexandrova, Catherine Lacombe, and Patrick Canu for their help in STAFF data. We would like to thank two anonymous reviewers for evaluating the paper. Publisher Copyright: {\textcopyright}2016. American Geophysical Union. All Rights Reserved. Copyright: Copyright 2016 Elsevier B.V., All rights reserved.",
year = "2016",
month = aug,
day = "16",
doi = "10.1002/2016GL069823",
language = "English",
volume = "43",
pages = "7795--7803",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "American Geophysical Union",
number = "15",

}

RIS

TY - JOUR

T1 - Two interacting X lines in magnetotail

T2 - Evolution of collision between the counterstreaming jets

AU - Alexandrova, Alexandra

AU - Nakamura, Rumi

AU - Panov, Evgeny V.

AU - Sasunov, Yury L.

AU - Nakamura, Takuma

AU - Vörös, Zoltán

AU - Retinò, Alessandro

AU - Semenov, Vladimir S.

N1 - Funding Information: The research was supported by the Austrian Science Fund (FWF) grant P23862-N16, A.A. and R.N., and grant P24740-N27, Z.V. V.S.S. was supported by the Russian Foundation for Basic Research (RFBR) grant 16-05-0047016. A.A. acknowledges the Cluster Science Archive for use of data presented and Emmanuel Penou for the ion velocity distribution provided by the CLWeb software. A.A. thanks Olga Alexandrova, Catherine Lacombe, and Patrick Canu for their help in STAFF data. We would like to thank two anonymous reviewers for evaluating the paper. Publisher Copyright: ©2016. American Geophysical Union. All Rights Reserved. Copyright: Copyright 2016 Elsevier B.V., All rights reserved.

PY - 2016/8/16

Y1 - 2016/8/16

N2 - We study the process of collision between the counterstreaming jets flowing out from two reconnection sites in the Earth's magnetotail. The X lines, bracketing the region of jets collision, were passing by two Cluster probes successively in tailward direction. Two probes observed two different stages of the collision process. At the jets collision site, a probe first observed an ion-scale current sheet-like structure, while the other probe observed more compressed one later. The strong wave activities on both ion and electron scales were seen within the compressed layer. Such evolution of the jets collision resulting in the formation of the compressed boundary between the active X lines shows an example of interaction between the X lines during multiple reconnection.

AB - We study the process of collision between the counterstreaming jets flowing out from two reconnection sites in the Earth's magnetotail. The X lines, bracketing the region of jets collision, were passing by two Cluster probes successively in tailward direction. Two probes observed two different stages of the collision process. At the jets collision site, a probe first observed an ion-scale current sheet-like structure, while the other probe observed more compressed one later. The strong wave activities on both ion and electron scales were seen within the compressed layer. Such evolution of the jets collision resulting in the formation of the compressed boundary between the active X lines shows an example of interaction between the X lines during multiple reconnection.

KW - jets collision

KW - magnetic reconnection

KW - multiple reconnection

UR - http://www.scopus.com/inward/record.url?scp=84980390177&partnerID=8YFLogxK

U2 - 10.1002/2016GL069823

DO - 10.1002/2016GL069823

M3 - Article

VL - 43

SP - 7795

EP - 7803

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

IS - 15

ER -

ID: 7628177