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• W1514439400 abstract "Abstract Observations of the solar wind interaction with weakly magnetized bodies in the solar system (Venus, Mars, comets) are used to define guidelines applicable to the region of interaction between the local interstellar plasma and the solar wind. In particular, a configuration based on a supersonic flow past a plasma obstacle is considered. It is argued that anomalous viscous processes may produce a downstream deformation of the heliospheric cavity and the stratification of the interstellar plasma that flows around it. In addition to the interface (heliopause) that bounds the solar wind from the interstellar plasma, and the external bow shock that develops upstream from that boundary, there should be a third transition within the interstellar flow located in the region between them. This additional (intermediate) boundary marks the outermost extent of the region affected by friction processes at the heliopause and divides the postshock interstellar flow into layers of different properties. Downstream from the intermediate transition the plasma should be hotter, more rarifed and move slower than that upstream from it." @default.
• W1514439400 created "2016-06-24" @default.
• W1514439400 creator A5076277610 @default.
• W1514439400 date "1990-01-01" @default.
• W1514439400 modified "2023-09-25" @default.
• W1514439400 title "Signature of a Viscous Interaction at the Heliopause" @default.
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• W1514439400 doi "https://doi.org/10.1016/b978-0-08-040780-7.50052-x" @default.
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