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ICMEs in the Inner Heliosphere: Origin, Evolution and Propagation Effects |
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| Authors: | R J Forsyth V Bothmer C Cid N U Crooker T S Horbury K Kecskemety B Klecker J A Linker D Odstrcil M J Reiner I G Richardson J Rodriguez-Pacheco J M Schmidt R F Wimmer-Schweingruber |
| Institution: | 1. The Blackett Laboratory, Imperial College London, London, UK 2. Institute for Astrophysics, University of G?ttingen, G?ttingen, Germany 3. Alcalá Space Research Group, Dpto. Fí sica, Univ. de Alcalá, Madrid, Spain 4. Center for Space Physics, Boston University, Boston, Massachusetts, USA 5. KFKI Research Institute for Particle and Nuclear Physics, Budapest, Hungary 6. MPI für Extraterrestrische Physik, Garching, Germany 7. SAIC, San Diego, CA, USA 8. NOAA Space Environment Center, Boulder, CO, USA 9. The Catholic University of America and NASA/GSFC, Greenbelt, MD, USA 10. NASA Goddard Space Flight Center, Greenbelt, MD, USA 11. International University Bremen, Bremen, Germany 12. Institut für Experimentelle und Angewandte Physik, Extraterrestrische Physik, Christian-Albrechts-Universit?t zu Kiel, Kiel, Germany |
| Abstract: | This report assesses the current status of research relating the origin at the Sun, the evolution through the inner heliosphere and the effects on the inner heliosphere of the interplanetary counterparts of coronal mass ejections (ICMEs). The signatures of ICMEs measured by in-situ spacecraft are determined both by the physical processes associated with their origin in the low corona, as observed by space-borne coronagraphs, and by the physical processes occurring as the ICMEs propagate out through the inner heliosphere, interacting with the ambient solar wind. The solar and in-situ observations are discussed as are efforts to model the evolution of ICMEs from the Sun out to 1 AU. |
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