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Evolution of interplanetary coronal mass ejections and magnetic clouds in the heliosphere

Published online by Cambridge University Press:  06 January 2014

Pascal Démoulin
Pascal Démoulin*
Affiliation:
Observatoire de Paris, LESIA, UMR 8109 (CNRS), F-92195 Meudon Principal Cedex, France email: Pascal.Demoulin@obspm.fr
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Abstract

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Interplanetary Coronal Mass Ejections (ICMEs), and more specifically Magnetic Clouds (MCs), are detected with in situ plasma and magnetic measurements. They are the continuation of the CMEs observed with imagers closer to the Sun. A review of their properties is presented with a focus on their magnetic configuration and its evolution. Many recent observations, both in situ and with imagers, point to a key role of flux ropes, a conclusion which is also supported by present coronal eruptive models. Then, is a flux rope generically present in an ICME? How to quantify its 3D physical properties when it is detected locally as a MC? Is it a simple flux rope? How does it evolve in the solar wind? This paper reviews our present answers and limited understanding to these questions.

Keywords

magnetic fields(magnetohydrodynamics:) MHDSun: coronal mass ejections (CMEs)Sun: magnetic fieldsinterplanetary medium
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 245 - 254
Copyright
Copyright © International Astronomical Union 2013 

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