Latitudinal variation of solar wind corotating stream interaction regions: Ulysses
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J. Phillips | J. Gosling | D. Mccomas | S. Bame | M. Neugebauer | V. Pizzo | B. Goldstein | B. Goldstein | D. McComas
[1] V. Pizzo. Global, quasi‐steady dynamics of the distant solar wind, 1. Origin of north‐south flows in the outer heliosphere , 1994 .
[2] J. Harvey,et al. Ulysses observations of a recurrent high speed solar wind stream and the heliomagnetic streamer belt , 1993 .
[3] J. Phillips,et al. Disappearance of the heliospheric sector structure at Ulysses , 1993 .
[4] V. Pizzo. The evolution of corotating stream fronts near the ecliptic plane in the inner solar system: 2. Three‐dimensional tilted‐dipole fronts , 1991 .
[5] A. Hundhausen,et al. Solar wind structure at large heliocentric distances: An interpretation of Pioneer 10 observations , 1976 .
[6] E. Smith,et al. Observations of interaction regions and corotating shocks between one and five AU - Pioneers 10 and 11. [solar wind streams] , 1976 .
[7] J. Asbridge. Compressions and Rarefactions in the Solar Wind' Vela 3 J. T. GosLInG, A. J. HUN)HAUSEN, AND V. Pzzo , 1972 .
[8] G. Siscoe,et al. An east-west asymmetry in the solar wind velocity. , 1969 .
[9] David J. McComas,et al. The Ulysses solar wind plasma experiment , 1992 .