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A Global Picture of CMEs in the Inner Heliosphere

  • N. Gopalswamy
Part of the Astrophysics and Space Science Library book series (ASSL, volume 317)

Abstract

This is an overview of Coronal mass ejections (CMEs) in the heliosphere with an observational bias towards remote sensing by coronagraphs. Particular emphasis will be placed on the results from the Solar and Heliospheric Observatory (SOHO) mission which has produced high quality CME data uniform and continuos over the longest stretch ever. After summarizing the morphological, physical, and statistical properties of CMEs, a discussion on the phenomena associated with them is presented. These are the various manifestations of CMEs observed at different wavelengths and the accompanying phenomena such as shocks and solar energetic particles that provide information to build a complete picture of CMEs. Implications of CMEs for the evolution of the global solar magnetic field are presented. CMEs in the heliosphere are then discussed including out-of-the-ecliptic observations from Ulysses and the possibility of a 22-year cycle of cosmic ray modulation by CMEs. After outlining some of the outstanding questions, a summary of the chapter is provided.

Keywords

Solar Wind Coronal Mass Ejection Magnetic Cloud Flux Rope Halo CMEs 
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 Dordrecht 2004

Authors and Affiliations

  • N. Gopalswamy
    • 1
  1. 1.Laboratory for Extraterrestrial PhysicsNASA/GSFCGreenbeltUSA

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