Properties of Stream Interactions at One AU During 1995 – 2004

A stream interaction region (SIR) forms when a fast solar stream overtakes a slow stream, leading to structure that evolves as an SIR moves away from the Sun. Based on Wind (1995 - 2004) and ACE (1998 - 2004) in situ observations, we have conducted a comprehensive survey of SIRs at one AU, including...

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Veröffentlicht in:	Solar physics 2006-12, Vol.239 (1-2), p.337-392
Hauptverfasser:	Jian, L, Russell, C T, Luhmann, J G, Skoug, R M
Format:	Artikel
Sprache:	eng
Schlagworte:	Magnetic fields Solar physics
Online-Zugang:	Volltext
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