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CIR Morphology, Turbulence, Discontinuities, and Energetic Particles

Report of Working Group 2

  • Conference paper
Corotating Interaction Regions

Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 7))

Abstract

Corotating interaction regions (CIRs) in the middle heliosphere have distinct morphological features and associated patterns of turbulence and energetic particles. This report summarizes current understanding of those features and patterns, discusses how they can vary from case to case and with distance from the Sun and possible causes of those variations, presents an analytical model of the morphological features found in earlier qualitative models and numerical simulations, and identifies aspects of the features and patterns that have yet to be resolved.

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Author notes

  1. T. S. Horbury

    Present address: Queen Mary and Westfield College, London, UK

Authors and Affiliations

  1. Center for Space Physics, Boston University, Boston, Massachusetts, USA

    N. U. Crooker & G. L. Siscoe

  2. Los Alamos National Laboratory, Los Alamos, New Mexico, USA

    J. T. Gosling

  3. Extraterrestrische Physik, Universität Kiel, Kiel, Germany

    V. Bothmer & A. Posner

  4. The Blackett Laboratory, Imperial College, London, UK

    R. J. Forsyth, T. S. Horbury, E. Lucek & J. M. Schmidt

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

    P. R. Gazis

  6. Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, UK

    A. Hewish

  7. Carmel Research Center, Santa Monica, California, USA

    D. S. Intriligator

  8. Depts. of Planetary Sciences and Astronomy, University of Arizona, Tucson, Arizona, USA

    J. R. Jokipii & J. Kóta

  9. Center for Space Research, Massachusetts Institute of Technology, Cambridge, Mass., USA

    A. J. Lazarus

  10. Space Science Center, University of New Hampshire, Durham, New Hampshire, USA

    M. A. Lee

  11. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany

    E. Marsch

  12. NASA Goddard Space Flight Center, Greenbelt, Maryland, USA

    I. G. Richardson

  13. Dept. of Astronomy, University of Maryland, College Park, Maryland, USA

    I. G. Richardson

  14. Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, USA

    E. C. Roelof

  15. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA

    B. T. Tsurutani

  16. Physikalisches Institut der Universität Bern, Bern, Switzerland

    R. F. Wimmer-Schweingruber

Authors
  1. N. U. Crooker
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  2. J. T. Gosling
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  3. V. Bothmer
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  4. R. J. Forsyth
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  5. P. R. Gazis
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  6. A. Hewish
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  7. T. S. Horbury
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  8. D. S. Intriligator
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  9. J. R. Jokipii
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  10. J. Kóta
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  11. A. J. Lazarus
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  12. M. A. Lee
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  13. E. Lucek
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  14. E. Marsch
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  15. A. Posner
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  16. I. G. Richardson
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  17. E. C. Roelof
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  18. J. M. Schmidt
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  19. G. L. Siscoe
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  20. B. T. Tsurutani
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  21. R. F. Wimmer-Schweingruber
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Editor information

Editors and Affiliations

  1. The Blackett Laboratory, Imperial College, SW7 2BZ, London, UK

    A. Balogh

  2. Los Alamos National Laboratory, MS D466, NM, 87545, Los Alamos, USA

    J. T. Gosling

  3. Lunar and Planetary Laboratory, University of Arizona, 85721, Tucson, AZ, USA

    J. R. Jokipii

  4. International Space Science Institute, CH-3012, Bern, Switzerland

    R. Kallenbach

  5. Extraterrestrische Physik, Institut für Experimentelle und Angewandte Physik, Universität Kiel, D-24118, Kiel, Germany

    H. Kunow

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Crooker, N.U. et al. (1999). CIR Morphology, Turbulence, Discontinuities, and Energetic Particles. In: Balogh, A., Gosling, J.T., Jokipii, J.R., Kallenbach, R., Kunow, H. (eds) Corotating Interaction Regions. Space Sciences Series of ISSI, vol 7. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1179-1_12

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  • DOI: https://doi.org/10.1007/978-94-017-1179-1_12

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5367-1

  • Online ISBN: 978-94-017-1179-1

  • eBook Packages: Springer Book Archive

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