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Observation of repeated intense near-Earth reconnection on closed field lines with Cluster, Double Star, and other spacecraft. / Sergeev, V.; Semenov, V.; Kubyshkina, M.; Ivanova, V.; Baumjohann, W.; Nakamura, R.; Penz, T.; Runov, A.; Zhang, T. L.; Glassmeier, K. H.; Angelopoulos, V.; Frey, H.; Sauvaud, J. A.; Daly, P.; Cao, J. B.; Singer, H.; Lucek, E.

в: Geophysical Research Letters, Том 34, № 2, L02103, 28.01.2007.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Sergeev, V, Semenov, V, Kubyshkina, M, Ivanova, V, Baumjohann, W, Nakamura, R, Penz, T, Runov, A, Zhang, TL, Glassmeier, KH, Angelopoulos, V, Frey, H, Sauvaud, JA, Daly, P, Cao, JB, Singer, H & Lucek, E 2007, 'Observation of repeated intense near-Earth reconnection on closed field lines with Cluster, Double Star, and other spacecraft', Geophysical Research Letters, Том. 34, № 2, L02103. https://doi.org/10.1029/2006GL028452

APA

Sergeev, V., Semenov, V., Kubyshkina, M., Ivanova, V., Baumjohann, W., Nakamura, R., Penz, T., Runov, A., Zhang, T. L., Glassmeier, K. H., Angelopoulos, V., Frey, H., Sauvaud, J. A., Daly, P., Cao, J. B., Singer, H., & Lucek, E. (2007). Observation of repeated intense near-Earth reconnection on closed field lines with Cluster, Double Star, and other spacecraft. Geophysical Research Letters, 34(2), [L02103]. https://doi.org/10.1029/2006GL028452

Vancouver

Sergeev V, Semenov V, Kubyshkina M, Ivanova V, Baumjohann W, Nakamura R и пр. Observation of repeated intense near-Earth reconnection on closed field lines with Cluster, Double Star, and other spacecraft. Geophysical Research Letters. 2007 Янв. 28;34(2). L02103. https://doi.org/10.1029/2006GL028452

Author

Sergeev, V. ; Semenov, V. ; Kubyshkina, M. ; Ivanova, V. ; Baumjohann, W. ; Nakamura, R. ; Penz, T. ; Runov, A. ; Zhang, T. L. ; Glassmeier, K. H. ; Angelopoulos, V. ; Frey, H. ; Sauvaud, J. A. ; Daly, P. ; Cao, J. B. ; Singer, H. ; Lucek, E. / Observation of repeated intense near-Earth reconnection on closed field lines with Cluster, Double Star, and other spacecraft. в: Geophysical Research Letters. 2007 ; Том 34, № 2.

BibTeX

@article{077c4d7ebe734031b7f629ee0baa7e3e,
title = "Observation of repeated intense near-Earth reconnection on closed field lines with Cluster, Double Star, and other spacecraft",
abstract = "We report strong repeated magnetic reconnection pulses that occurred deep inside closed plasma sheet flux tubes at r ≤ 14Re. They have been observed with a fortuitous spacecraft constellation during three consecutive turbulent magnetic dipolarizations, accompanied by localized auroral brightenings near the equatorward edge of a wide auroral oval. The reconnection separatrix was mapped to ∼64° CGLat in the ionosphere, where a very energetic and narrow energy-dispersed ion injection with unusually steep dispersion slope was observed. Reconstruction of the reconnection rate from magnetic waveforms at Cluster provided a reconnection pulse duration (∼1 min) and peak strength (ER ∼ 8 mV/m) consistent with direct observations in the reconnection outflow region. The magnetic activity was rather weak, although the concurrent solar wind flow pressure was above the norm. We suggest that near-Earth reconnection events may be a phenomenon more frequent than generally thought. We also confirm that reconnection and the growth of strong turbulence in the near tail are strongly coupled together in near-Earth reconnection events.",
author = "V. Sergeev and V. Semenov and M. Kubyshkina and V. Ivanova and W. Baumjohann and R. Nakamura and T. Penz and A. Runov and Zhang, {T. L.} and Glassmeier, {K. H.} and V. Angelopoulos and H. Frey and Sauvaud, {J. A.} and P. Daly and Cao, {J. B.} and H. Singer and E. Lucek",
year = "2007",
month = jan,
day = "28",
doi = "10.1029/2006GL028452",
language = "English",
volume = "34",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "American Geophysical Union",
number = "2",

}

RIS

TY - JOUR

T1 - Observation of repeated intense near-Earth reconnection on closed field lines with Cluster, Double Star, and other spacecraft

AU - Sergeev, V.

AU - Semenov, V.

AU - Kubyshkina, M.

AU - Ivanova, V.

AU - Baumjohann, W.

AU - Nakamura, R.

AU - Penz, T.

AU - Runov, A.

AU - Zhang, T. L.

AU - Glassmeier, K. H.

AU - Angelopoulos, V.

AU - Frey, H.

AU - Sauvaud, J. A.

AU - Daly, P.

AU - Cao, J. B.

AU - Singer, H.

AU - Lucek, E.

PY - 2007/1/28

Y1 - 2007/1/28

N2 - We report strong repeated magnetic reconnection pulses that occurred deep inside closed plasma sheet flux tubes at r ≤ 14Re. They have been observed with a fortuitous spacecraft constellation during three consecutive turbulent magnetic dipolarizations, accompanied by localized auroral brightenings near the equatorward edge of a wide auroral oval. The reconnection separatrix was mapped to ∼64° CGLat in the ionosphere, where a very energetic and narrow energy-dispersed ion injection with unusually steep dispersion slope was observed. Reconstruction of the reconnection rate from magnetic waveforms at Cluster provided a reconnection pulse duration (∼1 min) and peak strength (ER ∼ 8 mV/m) consistent with direct observations in the reconnection outflow region. The magnetic activity was rather weak, although the concurrent solar wind flow pressure was above the norm. We suggest that near-Earth reconnection events may be a phenomenon more frequent than generally thought. We also confirm that reconnection and the growth of strong turbulence in the near tail are strongly coupled together in near-Earth reconnection events.

AB - We report strong repeated magnetic reconnection pulses that occurred deep inside closed plasma sheet flux tubes at r ≤ 14Re. They have been observed with a fortuitous spacecraft constellation during three consecutive turbulent magnetic dipolarizations, accompanied by localized auroral brightenings near the equatorward edge of a wide auroral oval. The reconnection separatrix was mapped to ∼64° CGLat in the ionosphere, where a very energetic and narrow energy-dispersed ion injection with unusually steep dispersion slope was observed. Reconstruction of the reconnection rate from magnetic waveforms at Cluster provided a reconnection pulse duration (∼1 min) and peak strength (ER ∼ 8 mV/m) consistent with direct observations in the reconnection outflow region. The magnetic activity was rather weak, although the concurrent solar wind flow pressure was above the norm. We suggest that near-Earth reconnection events may be a phenomenon more frequent than generally thought. We also confirm that reconnection and the growth of strong turbulence in the near tail are strongly coupled together in near-Earth reconnection events.

UR - http://www.scopus.com/inward/record.url?scp=34548027504&partnerID=8YFLogxK

U2 - 10.1029/2006GL028452

DO - 10.1029/2006GL028452

M3 - Article

AN - SCOPUS:34548027504

VL - 34

JO - Geophysical Research Letters

JF - Geophysical Research Letters

SN - 0094-8276

IS - 2

M1 - L02103

ER -

ID: 18137491