Articles | Volume 23, issue 2
https://doi.org/10.5194/angeo-23-461-2005
© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-23-461-2005
© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Cluster multispacecraft observations at the high-latitude duskside magnetopause: implications for continuous and component magnetic reconnection
A. Retinò
Swedish Institute of Space Physics, Uppsala, Sweden
M. B. Bavassano Cattaneo
IFSI-CNR, Roma, Italy
M. F. Marcucci
IFSI-CNR, Roma, Italy
A. Vaivads
Swedish Institute of Space Physics, Uppsala, Sweden
M. André
Swedish Institute of Space Physics, Uppsala, Sweden
Y. Khotyaintsev
Swedish Institute of Space Physics, Uppsala, Sweden
T. Phan
University of California, Berkeley, USA
G. Pallocchia
IFSI-CNR, Roma, Italy
H. Rème
CESR, Toulouse, France
E. Möbius
University of New Hampshire, Durham, USA
B. Klecker
MPE, Garching, Germany
C. W. Carlson
University of California, Berkeley, USA
M. McCarthy
University of Washington, Seattle, USA
A. Korth
MPS, Lindau, Germany
R. Lundin
Swedish Institute of Space Physics, Kiruna, Sweden
A. Balogh
Imperial College, London, UK
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Cited
36 citations as recorded by crossref.
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- Retreat and reformation of X‐line during quasi‐continuous tailward‐of‐the‐cusp reconnection under northward IMF H. Hasegawa et al. 10.1029/2008GL034767
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Latest update: 23 Nov 2024