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• W2117776755 abstract "Solar wind speeds and magnetic field data from the Pioneer Venus Orbiter (0.7 AU) and IMP 8 (1 AU) have been compared to infer the latitudinal structure of the solar wind in the inner heliosphere between 1984 and 1987. The solar wind in the inner heliosphere was found to exhibit an unusual structure during the last solar minimum (1986-1987). High-speed streams were excluded from the vicinity of the solar equator, and the solar wind at low heliographic latitudes (less than 3 deg) was characterized by low-speed solar wind with irregular fluctuations in velocity. At higher latitudes the solar wind had a conventional stream structure with two high-speed streams per solar rotation. While the velocities of these high-speed streams did not appear to vary significantly with latitude, the latitudinal gradients at the equatorward boundaries of high-speed streams were high." @default.
• W2117776755 created "2016-06-24" @default.
• W2117776755 creator A5082161480 @default.
• W2117776755 date "1993-01-01" @default.
• W2117776755 modified "2023-09-24" @default.
• W2117776755 title "Pioneer Venus and IMP 8 observations of the latitude dependence of the solar wind" @default.
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• W2117776755 doi "https://doi.org/10.1029/92ja03000" @default.
• W2117776755 hasPublicationYear "1993" @default.
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