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.
|Original language||English (US)|
|Number of pages||42|
|Journal||Space Science Reviews|
|State||Published - Dec 1 1999|
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science