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Astrophys. Space Sci. Trans., 3, 15-20, 2007
www.astrophys-space-sci-trans.net/3/15/2007/ doi:10.5194/astra-3-15-2007 © Author(s) 2007. This work is licensed under the Creative Commons Attribution-NonCommercial-ShareAlike 2.5 License. |
07 Sep 2007
1Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, B–9000 Gent, Belgium
2School of Physics, University of KwaZulu-Natal, Private Bag X54001, Durban 4000, South Africa
3Indian Institute of Geomagnetism, New Panvel (West), Navi Mumbai 410 218, India
Abstract. Necessary conditions are discussed for the possible generation of large solitary acoustic modes in plasmas with one or more ion species which are hotter than some or all of the electron species. The analysis is based on a fluid dynamic approach. It is found that in most of these configurations the existence ranges for the solitary wave velocities are very narrow and close to one of the thermal velocities. In the latter situation, linear Landau damping may prevent the generation of nonlinear structures. The analysis indicates that both inertial and thermal effects for the ions need to be kept in the description, thus rendering an analytical investigation much more intricate.
Citation: Verheest, F., Hellberg, M. A., and Lakhina, G. S.: Necessary conditions for the generation of acoustic solitons in magnetospheric and space plasmas with hot ions, Astrophys. Space Sci. Trans., 3, 15-20, doi:10.5194/astra-3-15-2007, 2007.