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Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.14/41491

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Title
Physics of the dusty Hall plasmas
Related
Physics of plasmas, Vol. 13, Issue 12, p.122106-1-122106-6
DOI
10.1063/1.2402148
Publisher
American Institute of Physics
Date
2006
FoR/RFCD Code(s)
020204 Plasma Physics; Fusion Plasmas; Electrical Discharges  020299 Atomic, Molecular, Nuclear, Particle and Plasma Physics not elsewhere classified
Author/Creator
Pandey, B. P
Author/Creator
Vranjes, J
Description
The presence of the immobile charged dust in the plasma modifies the scale over which the Hall effect becomes important. For a positively charged dusty background this scale can become arbitrarily large. It is shown that the emergence of the Hall effect in an immobile charged background is related to the presence of an electric field that operates over the plasma gyration period. The generalized flux, which is a combination of the magnetic and fluid vortex flux, can decay due to the presence of the charge or the density inhomogeneities. The normal mode behavior of such a dusty plasma could be very different for positively and negatively charged grains. Whereas for negatively charged grains the usual magnetohydrodynamic (MHD) modes are present in the system, for positively charged grains, the Alfvén mode may not exist if Znd~ne, where Z is the charge of the dust and nd(ne) are the dust (electron) number densities. In the presence of the inhomogeneities, inertialess dusty plasma is subject to the Hall instability. It is shown that the growth rate of the Hall instability is proportional to the whistler frequency. Since Hall drift is nondissipative in nature, this instability can play important role in redistributing the magnetic energy from the large to small scales.
Description
6 page(s)
Subject Keyword
020204 Plasma Physics; Fusion Plasmas; Electrical Discharges
Subject Keyword
020299 Atomic, Molecular, Nuclear, Particle and Plasma Physics not elsewhere classified
Resource Type
journal article
Organisation
Macquarie University. Dept. of Physics

Identifier
http://hdl.handle.net/1959.14/41491
Identifier
ISSN:1089-7674
Identifier
mq-rm-2006005835
Language
eng
Rights
Copyright 2006 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in Physics of plasmas, Vol. 13, Issue 12, pp.122106-1-122106-6 and may be found at http://link.aip.org/link/?php/13/122106.
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Subject
"Physics of plasmas"
 
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