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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Detalles Bibliográficos
Autores principales: Möstl, Ute V., Erkaev, Nikolay V., Zellinger, Michael, Lammer, Helmut, Gröller, Hannes, Biernat, Helfried K., Korovinskiy, Daniil
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Academic Press 2011
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3280700/
https://www.ncbi.nlm.nih.gov/pubmed/22347723
http://dx.doi.org/10.1016/j.icarus.2011.09.012

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3280700/
https://www.ncbi.nlm.nih.gov/pubmed/22347723
http://dx.doi.org/10.1016/j.icarus.2011.09.012

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