skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Kinetic Alfven wave instability in a Lorentzian dusty magnetoplasma

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.3491336· OSTI ID:21421306
;  [1];  [2];  [3]
  1. Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, A-8042 Graz, Austria and Institute of Physics, University of Graz, Universitaetplatz 5, A-8010 Graz (Austria)
  2. Institute of Computational Modelling, 660036 Krasnoyarsk, Russia and Siberian Federal University, 660041 Krasnoyarsk (Russian Federation)
  3. Virtual Vehicle Competence Center (vif), Inffeldgasse 21a, 8010 Graz (Austria)

This study presents a theoretical approach to analyze the influence of kappa distributed streaming ions and magnetized electrons on the plasma wave propagation in the presence of dust by employing two-potential theory. In particular, analytical expressions under certain conditions are derived for various modes of propagation comprising of kinetic Alfven wave streaming instability, two stream instability, and dust acoustic and whistler waves. A dispersion relation for kinetic Alfven-like streaming instability has been derived. The effects of dust particles and Lorentzian index on the growth rates and the threshold streaming velocity for the excitation of the instability are examined. The streaming velocity is observed to be destabilizing for slow motion and stabilizing for fast streaming motions. It is also observed that the presence of magnetic field and superthermal particles hinders the growth rate of instability. Possible applications to various space and astrophysical situations are discussed.

OSTI ID:
21421306
Journal Information:
Physics of Plasmas, Vol. 17, Issue 10; Other Information: DOI: 10.1063/1.3491336; (c) 2010 American Institute of Physics; ISSN 1070-664X
Country of Publication:
United States
Language:
English