Abstract
We clarify the underlying physics of long-wavelength dust magnetoacoustic waves and short-wavelength (in comparison with the ion gyroradius ρ i ) dust acoustic waves that are involved in the formation of Mach cones in the magnetized dusty plasma of Saturn’s rings.
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From Pis’ma v Zhurnal Éksperimental’no\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) i Teoretichesko\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Fiziki, Vol. 78, No. 2, 2003, pp. 110–111.
Original English Text Copyright © 2003 by Shukla, Mamun, Bingham.
This article was submitted by the authors in English.