CIR Morphology, Turbulence, Discontinuities, and Energetic Particles

Details CIR Morphology, Turbulence, Discontinuities, and Energetic Particles CIR Morphology, Turbulence, Discontinuities, and Energetic Particles

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ssrv...89..179c&link_type=abstract

Space Science Reviews, v. 89, Issue 1/2, p. 179-220 (1999).

Mathematics

Logic

27

Scientific paper

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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