Dust-acoustic Mach cones in magnetized electron-dust plasmas of Saturn

Details Dust-acoustic Mach cones in magnetized electron-dust plasmas of Saturn Dust-acoustic Mach cones in magnetized electron-dust plasmas of Saturn

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004georl..3106808m&link_type=abstract

Geophysical Research Letters, Volume 31, Issue 6, CiteID L06808

Physics

Plasma Physics

1

Planetology: Solar System Objects: Saturn, Space Plasma Physics: Charged Particle Motion And Acceleration, Space Plasma Physics: Kinetic And Mhd Theory, Space Plasma Physics: Wave/Particle Interactions, Space Plasma Physics: General Or Miscellaneous

Scientific paper

We discuss the possibility of the Mach cone formation involving the modified dust-acoustic waves in a dusty magnetoplasma composed of electrons and positively charged dust grains. It is shown that the modified dust-acoustic waves, whose wavelength is of the order of (or shorter than) the electron gyroradius, are one of the viable candidates for the formation of Mach cones in Saturn's dusty rings.

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