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• W1668638048 abstract "Observations between 1 and 5 AU by Pioneers 10 and 11 have led to the identification of large numbers of interplanetary shocks. Both forward and reverse shocks, which begin to develop beyond 1.5 AU and which frequently appear as shock pairs, are found to accompany solar wind streams. The number of forward shocks continues to increase out to at least 5 AU. Reverse shocks are seen less often than forward shocks and, in some instances, disappear at larger distances. There is evidence that the shocks are corotating in the solar frame, as anticipated theoretically. The evolution of solar wind streams beyond 1 AU is profoundly affected by the shocks. A thick interaction region, with large enhancements in density, temperature, field strength and fluctuation level, forms in the region originally characterized by a positive velocity gradient. The solar wind and magnetic field properties adjacent to, and within, the interaction regions have been studied to determine their qualitative behavior and characteristic changes with distance. Several interplanetary shocks generated by solar flares have also been identified and analyzed." @default.
• W1668638048 created "2016-06-24" @default.
• W1668638048 creator A5049299108 @default.
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• W1668638048 date "1977-01-01" @default.
• W1668638048 modified "2023-10-03" @default.
• W1668638048 title "Pioneer 10, 11 observations of evolving solar wind streams and shocks beyond 1 AU" @default.
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• W1668638048 doi "https://doi.org/10.1007/978-90-277-0860-1_11" @default.
• W1668638048 hasPublicationYear "1977" @default.
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