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Talk from EWASS (2013)
1.
Three-dimensional evolution of
ejected flux ropes from the Sun to 1 AU
2.
3.
Flux rope evolution
should be studied in 3D • • • • •
4.
Flux rope orientation
in 3D
5.
Tracking a flux
rope requires several tools
6.
Flux rope signatures
in the lower corona
7.
Coronagraph observations of
flux ropes
8.
In-situ measurements as
a constraint
9.
Flux rope propagation
through MHD solar wind
10.
Deflection towards equatorial
plane
11.
Rotation towards heliospheric
current sheet
12.
Rotation due to
kinematic interaction
13.
Conclusions • • • •
14.
Longitudinal deflection
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