Five Spacecraft Observations of Oppositely Directed Exhaust Jets from a Magnetic Reconnection X-line Extending > 4.3 x 10 6 km in the Solar Wind Gosling.
Studying Solar Wind Magnetic Reconnection Events using Cluster. A.C. Foster 1, C.J. Owen 1, A.N. Fazakerley 1, I. J. Rae 1, C. Forsyth 1, E. Lucek 2, H.
Studying Solar Wind Magnetic Reconnection Events using Cluster.
ICMEs and Magnetic Clouds Session Summary
Studying Solar Wind Magnetic Reconnection Events using the Cluster 4-point Measurement Capability
A multi-island mechanism for particle acceleration during magnetic reconnection in solar flares
