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3-D views of the expanding CME: from the Sun to 1AU

Published online by Cambridge University Press:  05 March 2015

Alexis P. Rouillard
Alexis P. Rouillard*
Affiliation:
Université de Toulouse; UPS-OMP; IRAP; Toulouse, France CNRS, IRAP, 9 Av. colonel Roche, BP 44346, F-31028 Toulouse cedex 4, France email: arouillard@irap.omp.eu
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Abstract

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Three-dimensional information on Coronal Mass Ejections (CMEs) can be obtained from a wide range of in-situ measurements and remote-sensing techniques. Extreme ultraviolet (EUV) and white-light imaging sensed from several vantage points can be used to infer the 3-D geometry of the different parts that constitute a CME. High-resolution and high-cadence coronal imaging provides detailed information on the formation and release phase of a magnetic flux rope, the lateral expansion of the CME and the reconfiguration of the corona associated with the effects of pressure variations and reconnection. The evolution of the CME in the interplanetary medium and the connection of its various substructures with in-situ measurements can be obtained from multi-point heliospheric imaging.

Keywords

Solar WindSolar ActivityCoronal Mass EjectionsCorotating Interaction Regions
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 106 - 108
Copyright
Copyright © International Astronomical Union 2015 

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