Space Sci.Rev., 89, 7 - 20, 1999
Abstract:
In a Corotating Interaction Region (CIR) the stream interface is
identified as a relatively sharp density drop, temperature rise, and
flow shear in the 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 solar wind near the Sun, the
evolution of stream interfaces with heliocentric distance in the inner
helioshere, and their relationship.
For preprints of this paper, please contact us.