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Understanding Interplanetary Coronal Mass Ejection Signatures

Report of Working Group B

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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.

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Authors and Affiliations

  1. Institut für Experimentelle und Angewandte Physik, Extraterrestrische Physik, Christian-Albrechts-Universityät zu Kiel, Kiel, Germany

    R. F. Wimmer-Schweingruber

  2. Center for Space Physics, Boston University, Boston, MA, USA

    N. U. Crooker

  3. The Blackett Laboratory, Imperial College London, London, United Kingdom

    A. Balogh, R. J. Forsyth & T. Horbury

  4. Max-Planck-Institut für Sonnensystemforschung, Lindau, Germany

    V. Bothmer & L. Rodriguez

  5. San Jose State University Foundation, NASA Ames Research Center, Moffett Field, CA, USA

    P. Gazis

  6. Laboratory for Atmospheric and Space Physicsm University of Colorado, Boulder, CO, USA

    J. T. Gosling

  7. International Space Science Institute, Bern, Switzerland

    A. Kilchenmann & R. von Steiger

  8. NASA Goddard Space Flight Center, Greenbelt, MD, USA

    I. G. Richardson

  9. Massachusets Institute of Technology, Cambridge, MA, USA

    J. D. Richardson

  10. Science Applications International Corporation, San Diego, CA, USA

    P. Riley

  11. Physikalisches Institut, Universität Bern, Bern, Switzerland

    P. Wurz

  12. Dept. of Atmosph.,Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI, USA

    T. H. Zurbuchen

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  1. R. F. Wimmer-Schweingruber
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  16. T. H. Zurbuchen
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Correspondence to R. F. Wimmer-Schweingruber.

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Wimmer-Schweingruber, R.F., Crooker, N.U., Balogh, A. et al. Understanding Interplanetary Coronal Mass Ejection Signatures. Space Sci Rev 123, 177–216 (2006). https://doi.org/10.1007/s11214-006-9017-x

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