Generalized theory for dust-acoustic Mach cones in Saturn's rings

Details Generalized theory for dust-acoustic Mach cones in Saturn's rings Generalized theory for dust-acoustic Mach cones in Saturn's rings

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003phla..315..258s&link_type=abstract

Physics Letters A, Volume 315, Issue 3-4, p. 258-261.

Physics

13

Scientific paper

A generalized theory for dust-acoustic Mach cones in a magnetized dusty plasma has been introduced. The roles of ion gyroradius ρi and short wavelength (in comparison with ρi) dust-acoustic waves (DAWs) in the formation of Mach cones in a magnetized dusty plasma of Saturn's rings are examined. It is shown that the effects of ion gyroradius, magnetic field strength at the equatorial plane, ion temperature, dust size, and dust charge play significant roles in the formation of Mach cones by short wavelength DAWs in Saturn's rings.

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