Download - Talk from EWASS (2013)
Transcript
Three-dimensional evolution of ejected flux ropes from the Sun to 1 AU
Flux rope evolution should be studied in 3D
•
•
•
•
•
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
•
•
•
•
Longitudinal deflection