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The Kelvin–Helmholtz instability at Venus: What is the unstable boundary?

The Kelvin–Helmholtz instability gained scientific attention after observations at Venus by the spacecraft Pioneer Venus Orbiter gave rise to speculations that the instability contributes to the loss of planetary ions through the formation of plasma clouds. Since then, a handful of studies were devo...

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Autores principales: Möstl, Ute V., Erkaev, Nikolay V., Zellinger, Michael, Lammer, Helmut, Gröller, Hannes, Biernat, Helfried K., Korovinskiy, Daniil
Formato: Artigo
Lenguaje:Inglês
Publicado: Academic Press 2011
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Acceso en línea:https://ncbi.nlm.nih.gov/pmc/articles/PMC3280700/
https://ncbi.nlm.nih.gov/pubmed/22347723
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1016/j.icarus.2011.09.012
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