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CME Evolution

Chapter
Part of the Astrophysics and Space Science Library book series (ASSL, volume 376)

Abstract

Here we review the popular mechanisms proposed to describe the evolution of the CME once it has cleared the Sun. These may be categorised into three categories: aerodynamic drag, shock dynamics and magnetohydroydynamics. We review each of these, and discuss the eventual fate of the CME as it merges with corotating structures and other CMEs at large distances from the Sun to form merged interaction regions.

Keywords

Solar Wind Coronal Hole Interplanetary Magnetic Field Flux Rope Solar Wind Speed 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media, LLC 2011

Authors and Affiliations

  1. 1.Space StudiesSouthwest Research InstituteBoulderUSA

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