Nonlinear dust Alfvén modes

Details Nonlinear dust Alfvén modes Nonlinear dust Alfvén modes

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ssrv...68..109v&link_type=abstract

Space Science Reviews, Volume 68, Issue 1-4, pp. 109-114

Astronomy and Astrophysics

Astrophysics

37

Dusty Plasmas, Alfv&Eacute, N Waves, Space Plasmas, Nonlinear Modes

Scientific paper

Nonlinear modes are investigated in magnetized dusty plasmas, where the dust dynamics is modelled by a number of cold, highly negatively charged and very massive fluids, besides ordinary electrons and protons. Several low-frequency motions occur which are typical for the dust components, some of them described by model equations such as the derivative nonlinear Schrödinger equation for electromagnetic waves. One can include equilibrium drifts and even fluctuations in the grain charges. Most of the preceding conclusions are relevant for different kinds of astrophysical and heliospheric plasmas.

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