Cluster observations of a transient signature in the magnetotail: implications for the mode of reconnection
S. Beyene,C. J. Owen,A. P. Walsh,C. Forsyth,A. N. Fazakerley,S. Kiehas,I. Dandouras,and E. Lucek
S. Beyene
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, RH5 6NT, UK
C. J. Owen
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, RH5 6NT, UK
A. P. Walsh
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, RH5 6NT, UK
C. Forsyth
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, RH5 6NT, UK
A. N. Fazakerley
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, RH5 6NT, UK
S. Kiehas
Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, 8042 Graz, Austria
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, California, USA
I. Dandouras
Institut de Recherche en Astrophysique et Planétologie (IRAP), University of Toulouse, UPS, 9 Ave. du Colonel Roche, B.P. 44346, 31028 Toulouse, France
IRAP, CNRS, B.P. 44346, 31028 Toulouse, France
E. Lucek
Space and Atmospheric Physics, Imperial College London, SW7 2BZ, UK
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