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Wallis 1982
Wallis, M.K. (1982). Comet-like interaction of Venus with the solar wind III the atomic oxygen corona. Geophysical Research Letters 9: doi: 10.1029/GL009i004p00427. issn: 0094-8276.

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 0+ 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.

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Journal
Geophysical Research Letters
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American Geophysical Union
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