talk from ewass (2013)
TRANSCRIPT
![Page 1: Talk from EWASS (2013)](https://reader033.vdocuments.us/reader033/viewer/2022052701/55d2aa6dbb61ebf23a8b45c8/html5/thumbnails/1.jpg)
Three-dimensional evolution of ejected flux ropes from the Sun to 1 AU
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Flux rope evolution should be studied in 3D
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Flux rope orientation in 3D
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Tracking a flux rope requires several tools
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Flux rope signatures in the lower corona
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Coronagraph observations of flux ropes
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In-situ measurements as a constraint
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Flux rope propagation through MHD solar wind
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Deflection towards equatorial plane
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Rotation towards heliospheric current sheet
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Rotation due to kinematic interaction
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Conclusions
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Longitudinal deflection