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Timing and location of phenomena during auroral breakup : A case study. / Yahnin, A. G.; Sergeev, V. A.; Kubyshkina, M. V.; Pulkkinen, T. I.; Liou, K.; Meng, C. I.; Angelopoulos, V.; Borodkova, N. L.; Mukai, T.; Kokubun, S.

In: Advances in Space Research, Vol. 30, No. 7, 2002, p. 1775-1778.

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

Harvard

Yahnin, AG, Sergeev, VA, Kubyshkina, MV, Pulkkinen, TI, Liou, K, Meng, CI, Angelopoulos, V, Borodkova, NL, Mukai, T & Kokubun, S 2002, 'Timing and location of phenomena during auroral breakup: A case study', Advances in Space Research, vol. 30, no. 7, pp. 1775-1778. https://doi.org/10.1016/S0273-1177(02)00447-7

APA

Yahnin, A. G., Sergeev, V. A., Kubyshkina, M. V., Pulkkinen, T. I., Liou, K., Meng, C. I., Angelopoulos, V., Borodkova, N. L., Mukai, T., & Kokubun, S. (2002). Timing and location of phenomena during auroral breakup: A case study. Advances in Space Research, 30(7), 1775-1778. https://doi.org/10.1016/S0273-1177(02)00447-7

Vancouver

Yahnin AG, Sergeev VA, Kubyshkina MV, Pulkkinen TI, Liou K, Meng CI et al. Timing and location of phenomena during auroral breakup: A case study. Advances in Space Research. 2002;30(7):1775-1778. https://doi.org/10.1016/S0273-1177(02)00447-7

Author

Yahnin, A. G. ; Sergeev, V. A. ; Kubyshkina, M. V. ; Pulkkinen, T. I. ; Liou, K. ; Meng, C. I. ; Angelopoulos, V. ; Borodkova, N. L. ; Mukai, T. ; Kokubun, S. / Timing and location of phenomena during auroral breakup : A case study. In: Advances in Space Research. 2002 ; Vol. 30, No. 7. pp. 1775-1778.

BibTeX

@article{5c19f64a361e4f5a8d62b460ef91f2ac,
title = "Timing and location of phenomena during auroral breakup: A case study",
abstract = "We performed a multi-instrument ground-based and satellite study of substorm-related phenomena during auroral breakup. Our study is limited to the short (a few minutes) time interval around the breakup onset. A mapping made on the basis of event-oriented magnetospheric model places the pre-breakup arc into the near-Earth region (r approximate to 10 R-E) where thin and intense current sheet develops. Disruption of the current sheet was observed in the same region. The plasmoid was observed in the mid-tail. Backtracing the plasmoid onset time and location confirmed that reconnection related to the substorm. onset could operate in the near-Earth thin current sheet. These observations are in agreement with the idea that the reconnection and current disruption signatures, as well as auroral breakup are different manifestations of the one process. (C) 2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved.",
keywords = "SUBSTORMS, DYNAMICS, FLOWS, MODEL, EVENT",
author = "Yahnin, {A. G.} and Sergeev, {V. A.} and Kubyshkina, {M. V.} and Pulkkinen, {T. I.} and K. Liou and Meng, {C. I.} and V. Angelopoulos and Borodkova, {N. L.} and T. Mukai and S. Kokubun",
year = "2002",
doi = "10.1016/S0273-1177(02)00447-7",
language = "Английский",
volume = "30",
pages = "1775--1778",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "7",
note = "null ; Conference date: 05-02-2001 Through 10-02-2001",

}

RIS

TY - JOUR

T1 - Timing and location of phenomena during auroral breakup

AU - Yahnin, A. G.

AU - Sergeev, V. A.

AU - Kubyshkina, M. V.

AU - Pulkkinen, T. I.

AU - Liou, K.

AU - Meng, C. I.

AU - Angelopoulos, V.

AU - Borodkova, N. L.

AU - Mukai, T.

AU - Kokubun, S.

PY - 2002

Y1 - 2002

N2 - We performed a multi-instrument ground-based and satellite study of substorm-related phenomena during auroral breakup. Our study is limited to the short (a few minutes) time interval around the breakup onset. A mapping made on the basis of event-oriented magnetospheric model places the pre-breakup arc into the near-Earth region (r approximate to 10 R-E) where thin and intense current sheet develops. Disruption of the current sheet was observed in the same region. The plasmoid was observed in the mid-tail. Backtracing the plasmoid onset time and location confirmed that reconnection related to the substorm. onset could operate in the near-Earth thin current sheet. These observations are in agreement with the idea that the reconnection and current disruption signatures, as well as auroral breakup are different manifestations of the one process. (C) 2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved.

AB - We performed a multi-instrument ground-based and satellite study of substorm-related phenomena during auroral breakup. Our study is limited to the short (a few minutes) time interval around the breakup onset. A mapping made on the basis of event-oriented magnetospheric model places the pre-breakup arc into the near-Earth region (r approximate to 10 R-E) where thin and intense current sheet develops. Disruption of the current sheet was observed in the same region. The plasmoid was observed in the mid-tail. Backtracing the plasmoid onset time and location confirmed that reconnection related to the substorm. onset could operate in the near-Earth thin current sheet. These observations are in agreement with the idea that the reconnection and current disruption signatures, as well as auroral breakup are different manifestations of the one process. (C) 2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved.

KW - SUBSTORMS

KW - DYNAMICS

KW - FLOWS

KW - MODEL

KW - EVENT

UR - http://www.scopus.com/inward/record.url?scp=6444244297&partnerID=8YFLogxK

U2 - 10.1016/S0273-1177(02)00447-7

DO - 10.1016/S0273-1177(02)00447-7

M3 - статья

AN - SCOPUS:6444244297

VL - 30

SP - 1775

EP - 1778

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 7

Y2 - 5 February 2001 through 10 February 2001

ER -

ID: 18138426