Dust-induced instability in a rotating plasma


Autoria(s): MIKHAILOVSKII, A. B.; VLADIMIROV, S. V.; LOMINADZE, J. G.; TSYPIN, V. S.; CHURIKOV, A. P.; EROKHIN, N. N.; Galvao, Ricardo Magnus Osorio
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

18/04/2012

18/04/2012

2008

Resumo

The effect of immobile dust on stability of a magnetized rotating plasma is analyzed. In the presence of dust, a term containing an electric field appears in the one-fluid equation of plasma motion. This electric field leads to an instability of the magnetized rotating plasma called the dust-induced rotational instability (DRI). The DRI is related to the charge imbalance between plasma ions and electrons introduced by the presence of charged dust. In contrast to the well-known magnetorotational instability requiring the decreasing radial profile of the plasma rotation frequency, the DRI can appear for an increasing rotation frequency profile. (c) 2008 American Institute of Physics.

Identificador

PHYSICS OF PLASMAS, v.15, n.1, 2008

1070-664X

http://producao.usp.br/handle/BDPI/15985

10.1063/1.2813188

http://dx.doi.org/10.1063/1.2813188

Idioma(s)

eng

Publicador

AMER INST PHYSICS

Relação

Physics of Plasmas

Direitos

openAccess

Copyright AMER INST PHYSICS

Palavras-Chave #HIGH-Z IMPURITIES #ALFVEN WAVES #PROTOPLANETARY DISKS #PROPAGATION #COAGULATION #GRAINS #Physics, Fluids & Plasmas
Tipo

article

original article

publishedVersion