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- W2443084920 abstract "Mars and Venus have no global magnetic field. The solar wind interacts directly with their ionospheres and atmospheres, inducing magnetospheres by a pileup of the interplanetary magnetic field. The first measurements of the ultra-low-frequency activity on Mars were made by the Phobos-2 spacecraft. This chapter investigates the wave observations recently supplied by the Mars Global Surveyor, Venus Express, and Mars Express. Coherent wave structures are a typical feature of the Martian magnetosheath. It is likely that the periodic compressional waves generated upstream of the bow shock are transported to the magnetosheath. At Venus, there has often been observed a penetration of the field oscillations downward to the ionosphere. Periodic oscillations of the escaping oxygen ions were typically observed in the Martian tail by MEX. It seems reasonable to suggest that the observed oscillations take their origin in the foreshock/magnetosheath and then propagate to the ionosphere and further to the tail." @default.
- W2443084920 created "2016-06-24" @default.
- W2443084920 creator A5001724387 @default.
- W2443084920 creator A5063411788 @default.
- W2443084920 date "2016-02-12" @default.
- W2443084920 modified "2023-10-14" @default.
- W2443084920 title "Ultra‐Low‐Frequency Waves at Venus and Mars" @default.
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- W2443084920 doi "https://doi.org/10.1002/9781119055006.ch20" @default.
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