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Reconstruction of the reconnection rate from Cluster measurements: Method improvements. / Ivanova, V.V.; Semenov, V.S.; Penz, T.; Ivanov, I.B.; Sergeev, V.A.; M.F., Heyn; Farrugia, C.J.; Biernat, H.K.; Nakamura, R.; Baumjohann, W.

в: Journal of Geophysical Research, Том 112, 2007.

Результаты исследований: Научные публикации в периодических изданияхстатья

Harvard

Ivanova, VV, Semenov, VS, Penz, T, Ivanov, IB, Sergeev, VA, M.F., H, Farrugia, CJ, Biernat, HK, Nakamura, R & Baumjohann, W 2007, 'Reconstruction of the reconnection rate from Cluster measurements: Method improvements', Journal of Geophysical Research, Том. 112. https://doi.org/10.1029/2006JA012183

APA

Ivanova, V. V., Semenov, V. S., Penz, T., Ivanov, I. B., Sergeev, V. A., M.F., H., Farrugia, C. J., Biernat, H. K., Nakamura, R., & Baumjohann, W. (2007). Reconstruction of the reconnection rate from Cluster measurements: Method improvements. Journal of Geophysical Research, 112. https://doi.org/10.1029/2006JA012183

Vancouver

Author

Ivanova, V.V. ; Semenov, V.S. ; Penz, T. ; Ivanov, I.B. ; Sergeev, V.A. ; M.F., Heyn ; Farrugia, C.J. ; Biernat, H.K. ; Nakamura, R. ; Baumjohann, W. / Reconstruction of the reconnection rate from Cluster measurements: Method improvements. в: Journal of Geophysical Research. 2007 ; Том 112.

BibTeX

@article{8e940b0a929c4478ad4a7e84d2105dac,
title = "Reconstruction of the reconnection rate from Cluster measurements: Method improvements",
abstract = "[1] A remote-sensing method for reconstructing the reconnection rate and the location of X-line from single-spacecraft observations developed recently is extended to a compressible plasma and an asymmetric magnetic field configuration. The method is based on the two-dimensional analytical model of time-dependent Petschek-type magnetic reconnection. The reconstruction technique is applied to a nightside flux transfer event recorded by Cluster spacecraft in the near-Earth magnetotail on 26 September 2005. The reconnection rate is found to be 3.7-4.8 mV/m; the reconnection distance is around 9-11 Re in the tail. Copyright 2007 by the American Geophysical Union.",
author = "V.V. Ivanova and V.S. Semenov and T. Penz and I.B. Ivanov and V.A. Sergeev and Heyn M.F. and C.J. Farrugia and H.K. Biernat and R. Nakamura and W. Baumjohann",
year = "2007",
doi = "10.1029/2006JA012183",
language = "English",
volume = "112",
journal = "Journal of Geophysical Research: Biogeosciences",
issn = "0148-0227",
publisher = "American Geophysical Union",

}

RIS

TY - JOUR

T1 - Reconstruction of the reconnection rate from Cluster measurements: Method improvements

AU - Ivanova, V.V.

AU - Semenov, V.S.

AU - Penz, T.

AU - Ivanov, I.B.

AU - Sergeev, V.A.

AU - M.F., Heyn

AU - Farrugia, C.J.

AU - Biernat, H.K.

AU - Nakamura, R.

AU - Baumjohann, W.

PY - 2007

Y1 - 2007

N2 - [1] A remote-sensing method for reconstructing the reconnection rate and the location of X-line from single-spacecraft observations developed recently is extended to a compressible plasma and an asymmetric magnetic field configuration. The method is based on the two-dimensional analytical model of time-dependent Petschek-type magnetic reconnection. The reconstruction technique is applied to a nightside flux transfer event recorded by Cluster spacecraft in the near-Earth magnetotail on 26 September 2005. The reconnection rate is found to be 3.7-4.8 mV/m; the reconnection distance is around 9-11 Re in the tail. Copyright 2007 by the American Geophysical Union.

AB - [1] A remote-sensing method for reconstructing the reconnection rate and the location of X-line from single-spacecraft observations developed recently is extended to a compressible plasma and an asymmetric magnetic field configuration. The method is based on the two-dimensional analytical model of time-dependent Petschek-type magnetic reconnection. The reconstruction technique is applied to a nightside flux transfer event recorded by Cluster spacecraft in the near-Earth magnetotail on 26 September 2005. The reconnection rate is found to be 3.7-4.8 mV/m; the reconnection distance is around 9-11 Re in the tail. Copyright 2007 by the American Geophysical Union.

U2 - 10.1029/2006JA012183

DO - 10.1029/2006JA012183

M3 - Article

VL - 112

JO - Journal of Geophysical Research: Biogeosciences

JF - Journal of Geophysical Research: Biogeosciences

SN - 0148-0227

ER -

ID: 5018308