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Substorm Current Wedge Revisited. / Kepko, L.; McPherron, R. L.; Amm, O.; Apatenkov, S.; Baumjohann, W.; Birn, J.; Lester, M.; Nakamura, R.; Pulkkinen, T. I.; Sergeev, V.

In: Space Science Reviews, Vol. 190, No. 1-4, 2015, p. 1-46.

Research output: Contribution to journalReview articlepeer-review

Harvard

Kepko, L, McPherron, RL, Amm, O, Apatenkov, S, Baumjohann, W, Birn, J, Lester, M, Nakamura, R, Pulkkinen, TI & Sergeev, V 2015, 'Substorm Current Wedge Revisited', Space Science Reviews, vol. 190, no. 1-4, pp. 1-46. https://doi.org/10.1007/s11214-014-0124-9, https://doi.org/10.1007/s11214-014-0124-9

APA

Kepko, L., McPherron, R. L., Amm, O., Apatenkov, S., Baumjohann, W., Birn, J., Lester, M., Nakamura, R., Pulkkinen, T. I., & Sergeev, V. (2015). Substorm Current Wedge Revisited. Space Science Reviews, 190(1-4), 1-46. https://doi.org/10.1007/s11214-014-0124-9, https://doi.org/10.1007/s11214-014-0124-9

Vancouver

Kepko L, McPherron RL, Amm O, Apatenkov S, Baumjohann W, Birn J et al. Substorm Current Wedge Revisited. Space Science Reviews. 2015;190(1-4):1-46. https://doi.org/10.1007/s11214-014-0124-9, https://doi.org/10.1007/s11214-014-0124-9

Author

Kepko, L. ; McPherron, R. L. ; Amm, O. ; Apatenkov, S. ; Baumjohann, W. ; Birn, J. ; Lester, M. ; Nakamura, R. ; Pulkkinen, T. I. ; Sergeev, V. / Substorm Current Wedge Revisited. In: Space Science Reviews. 2015 ; Vol. 190, No. 1-4. pp. 1-46.

BibTeX

@article{44cdb65ca6da457483caddf5a68e9530,
title = "Substorm Current Wedge Revisited",
abstract = "Almost 40 years ago the concept of the substorm current wedge was developed to explain the magnetic signatures observed on the ground and in geosynchronous orbit during substorm expansion. In the ensuing decades new observations, including radar and low-altitude spacecraft, MHD simulations, and theoretical considerations have tremendously advanced our understanding of this system. The AMPTE/IRM, THEMIS and Cluster missions have added considerable observational knowledge, especially on the important role of fast flows in producing the stresses that generate the substorm current wedge. Recent detailed, multi-spacecraft, multi-instrument observations both in the magnetosphere and in the ionosphere have brought a wealth of new information about the details of the temporal evolution and structure of the current system. While the large-scale picture remains valid, the new details call for revision and an update of the original view. In this paper we briefly review the historical development of the substorm current",
author = "L. Kepko and McPherron, {R. L.} and O. Amm and S. Apatenkov and W. Baumjohann and J. Birn and M. Lester and R. Nakamura and Pulkkinen, {T. I.} and V. Sergeev",
year = "2015",
doi = "10.1007/s11214-014-0124-9",
language = "English",
volume = "190",
pages = "1--46",
journal = "Space Science Reviews",
issn = "0038-6308",
publisher = "Springer Nature",
number = "1-4",

}

RIS

TY - JOUR

T1 - Substorm Current Wedge Revisited

AU - Kepko, L.

AU - McPherron, R. L.

AU - Amm, O.

AU - Apatenkov, S.

AU - Baumjohann, W.

AU - Birn, J.

AU - Lester, M.

AU - Nakamura, R.

AU - Pulkkinen, T. I.

AU - Sergeev, V.

PY - 2015

Y1 - 2015

N2 - Almost 40 years ago the concept of the substorm current wedge was developed to explain the magnetic signatures observed on the ground and in geosynchronous orbit during substorm expansion. In the ensuing decades new observations, including radar and low-altitude spacecraft, MHD simulations, and theoretical considerations have tremendously advanced our understanding of this system. The AMPTE/IRM, THEMIS and Cluster missions have added considerable observational knowledge, especially on the important role of fast flows in producing the stresses that generate the substorm current wedge. Recent detailed, multi-spacecraft, multi-instrument observations both in the magnetosphere and in the ionosphere have brought a wealth of new information about the details of the temporal evolution and structure of the current system. While the large-scale picture remains valid, the new details call for revision and an update of the original view. In this paper we briefly review the historical development of the substorm current

AB - Almost 40 years ago the concept of the substorm current wedge was developed to explain the magnetic signatures observed on the ground and in geosynchronous orbit during substorm expansion. In the ensuing decades new observations, including radar and low-altitude spacecraft, MHD simulations, and theoretical considerations have tremendously advanced our understanding of this system. The AMPTE/IRM, THEMIS and Cluster missions have added considerable observational knowledge, especially on the important role of fast flows in producing the stresses that generate the substorm current wedge. Recent detailed, multi-spacecraft, multi-instrument observations both in the magnetosphere and in the ionosphere have brought a wealth of new information about the details of the temporal evolution and structure of the current system. While the large-scale picture remains valid, the new details call for revision and an update of the original view. In this paper we briefly review the historical development of the substorm current

U2 - 10.1007/s11214-014-0124-9

DO - 10.1007/s11214-014-0124-9

M3 - Review article

VL - 190

SP - 1

EP - 46

JO - Space Science Reviews

JF - Space Science Reviews

SN - 0038-6308

IS - 1-4

ER -

ID: 4038154