Kelvin-Helmholtz versus Hall magnetoshear instability in astrophysical flows

We study the stability of shear flows in a fully ionized plasma. Kelvin-Helmholtz is a well-known macroscopic and ideal shear-driven instability. In sufficiently low-density plasmas, also the microscopic Hall magnetoshear instability can take place. We performed three-dimensional simulations of the...

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Detalles Bibliográficos
Autores principales: Gómez, D.O., Bejarano, C., Mininni, P.D.
Formato: JOUR
Materias:
Magnetohydrodynamics
Magnetoplasma
Plasma stability
Shear flow
Astrophysical flows
Comparative studies
Ion-cyclotron frequency
Ionized plasmas
Kelvin-Helmholtz
Kelvin-helmholtz instabilities
Low-density plasmas
Three dimensional simulations
Plasma diagnostics
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_15393755_v89_n5_p_Gomez
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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