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Understanding Interplanetary Coronal Mass Ejection Signatures |
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| Authors: | R F Wimmer-Schweingruber N U Crooker A Balogh V Bothmer R J Forsyth P Gazis J T Gosling T Horbury A Kilchenmann I G Richardson J D Richardson P Riley L Rodriguez R von Steiger P Wurz T H Zurbuchen |
| Institution: | 1. Institut für Experimentelle und Angewandte Physik, Extraterrestrische Physik, Christian-Albrechts-University?t zu Kiel, Kiel, Germany 2. Center for Space Physics, Boston University, Boston, MA, USA 3. The Blackett Laboratory, Imperial College London, London, United Kingdom 4. Max-Planck-Institut für Sonnensystemforschung, Lindau, Germany 5. San Jose State University Foundation, NASA Ames Research Center, Moffett Field, CA, USA 6. Laboratory for Atmospheric and Space Physicsm University of Colorado, Boulder, CO, USA 7. International Space Science Institute, Bern, Switzerland 8. NASA Goddard Space Flight Center, Greenbelt, MD, USA 9. Massachusets Institute of Technology, Cambridge, MA, USA 10. Science Applications International Corporation, San Diego, CA, USA 11. Physikalisches Institut, Universit?t Bern, Bern, Switzerland 12. Dept. of Atmosph.,Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI, USA |
| Abstract: | While interplanetary coronal mass ejections (ICMEs) are understood to be the heliospheric counterparts of CMEs, with signatures undeniably linked to the CME process, the variability of these signatures and questions about mapping to observed CME features raise issues that remain on the cutting edge of ICME research. These issues are discussed in the context of traditional understanding, and recent results using innovative analysis techniques are reviewed. |
| Keywords: | coronal mass ejections interplanetary physics solar wind |
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