Abstract
A generalized theory for dust-acoustic Mach cones in a magnetized dusty plasma has been introduced. The roles of ion gyroradius ρ i and short wavelength (in comparison with ρ i ) 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.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
