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Kelvin-Helmholtz instability in partially ionized compressible plasmas

The Kelvin-Helmholtz Instability (KHI) has been observed in the solar atmosphere. Ion-neutral collisions may play a relevant role for the growth rate and evolution of the KHI in solar partially ionized plasmas as in, e.g., solar prominences. Here, we investigate the linear phase of the KHI at an int...

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Detalles Bibliográficos
Autores principales:	Soler, R, Diaz, A J, Ballester, J L, Goossens, M
Lenguaje:	eng
Publicado:	2012
Materias:	Astrophysics and Astronomy
Acceso en línea:	https://dx.doi.org/10.1088/0004-637X/749/2/163 http://cds.cern.ch/record/1425732

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