Titlebook: Corotating Interaction Regions; Proceedings of an IS A. Balogh,J. T. Gosling,H. Kunow Conference proceedings 1999 Springer Science+Business

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Solar Origin and Interplanetary Evolution of Stream Interfacese solar wind, and is now generally believed to mark the boundary between solar wind which was originally slow when it left the Sun and solar wind which was originally fast. This paper summarises some important facts and open questions about the origin and nature of the boundary between fast and slow

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Formation and Evolution of Corotating Interaction Regions and Their Three Dimensional Structureifferent speeds to become radially aligned. Compressive interaction regions are produced where high-speed wind runs into slower plasma ahead. When the flow pattern emanating from the Sun is roughly time-stationary these compression regions form spirals in the solar equatorial plane that corotate wit

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