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VOLUME 78 (2003) | ISSUE 2 | PAGE 110
Comment on Mach cones and magnetic forces in Saturn's rings
PACS: 52.27.Lw, 52.35.Fp, 96.30.Wr
Abstract
We clarify the underlying physics of long wavelength dust magnetoacoustic waves and short wavelength (in comparison with the ion gyroradius ρi) dust acoustic waves that are involved in the formation of Mach cones in a magnetized dusty plasma of Saturn's rings.