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CIR Morphology, Turbulence, Discontinuities, and Energetic Particles |
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| Authors: | N.U. Crooker J.T. Gosling V. Bothmer R.J. Forsyth P.R. Gazis A. Hewish T.S. Horbury D.S. Intriligator J.R. Jokipii J. Kóta A.J. Lazarus M.A. Lee E. Lucek E. Marsch A. Posner I.G. Richardson E.C. Roelof J.M. Schmidt G.L. Siscoe B.T. Tsurutani R.F. Wimmer-Schweingruber |
| Affiliation: | 1. Center for Space Physics, Boston University, Boston, Massachusetts, USA 2. Los Alamos National Laboratory, Los Alamos, New Mexico, USA 3. Extraterrestrische Physik, Universit?t Kiel, Kiel, Germany 4. The Blackett Laboratory, Imperial College, London, United Kingdom 5. San Jose State University Foundation, NASA Ames Research Center, Moffett Field, California, USA 6. Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom 7. Queen Mary and Westfield College, London, United Kingdom 8. Carmel Research Center, Santa Monica, California, USA 9. Depts. of Planetary Sciences and Astronomy, University of Arizona, Tucson, Arizona, USA 10. Center for Space Research, Massachusetts Institute of Technology, Cambridge, Mass., USA 11. Space Science Center, University of New Hampshire, Durham, New Hampshire, USA 12. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany 13. NASA Goddard Space Flight Center, Greenbelt, Maryland, USA 14. Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, USA 15. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA 16. Physikalisches Institut der Universit?t Bern, Bern, Switzerland |
| 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. This revised version was published online in August 2006 with corrections to the Cover Date. |
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