Inferring the Magnetotail reconnection model from its magnetic products. Authors: S. Beyene 1 , C.J. Owen 1 , A.P. Walsh 1 , A.N. Fazakerley 1 , E. Lucek 2 , I. Dandouras 3 1 Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, RH5 6NT, UK
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Inferring the Magnetotail reconnection model from its magnetic products
Authors: S. Beyene1, C.J. Owen1, A.P. Walsh1, A.N. Fazakerley1, E. Lucek2, I. Dandouras3
1Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, RH5 6NT, UK
2Space and Atmospheric Physics, Imperial College London, SW7 2BZ, UK3Centre d’Etude Spatiale des Rayonnements, Toulouse, France
Multiple X-Line Reconnection
Time Dependant Reconnection
"from Kiehas et al., 2009"
The Cluster data was searched to find a magnetic structure (in the tail) to analyse in the hopes of inferring the reconnection model.
Orbit Plot Relative to C3
Possible Interpretations: Flux Rope
Possible Interpretations: Flux Bulge
Possible Interpretations: Wave