talk from ewass (2013)
Post on 18-Aug-2015
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Three-dimensional evolution of ejected flux ropes from the Sun to 1 AU
Flux rope evolution should be studied in 3D
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Flux rope orientation in 3D
Tracking a flux rope requires several tools
Flux rope signatures in the lower corona
Coronagraph observations of flux ropes
In-situ measurements as a constraint
Flux rope propagation through MHD solar wind
Deflection towards equatorial plane
Rotation towards heliospheric current sheet
Rotation due to kinematic interaction
Conclusions
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Longitudinal deflection
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