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- W2124459716 abstract "Suprathermal atomic oxygen constituting an extensive exospheric corona give rise to new heavy ions within the solar plasma flowing around Venus. Because their gyro-radii are large compared with transverse scales, the O+ ions do not simply effect a drag due to ‘mass loading’ of the flow. Some precipitate into the ionosphere and provide a novel ion source. Also, the back-reaction on the flow not only decelerates it, but also deviates it laterally and essentially asymmetrically about the planet." @default.
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- W2124459716 date "1982-04-01" @default.
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- W2124459716 title "Comet-like interaction of Venus with the solar wind III the atomic oxygen corona" @default.
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- W2124459716 doi "https://doi.org/10.1029/gl009i004p00427" @default.
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