Breaking dust-Alfvénic Mach barriers at Saturn

Shukla, P. K. and Mamun, A. A. and Bingham, R. (2003) Breaking dust-Alfvénic Mach barriers at Saturn. Physica Scripta, 68 (4). pp. 293-294. ISSN 0031-8949

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Abstract

A theoretical prediction for the formation of dust-Alfvénic Mach cones in Saturn's rings is made. It is explicitly shown that for typical dusty plasma parameters corresponding to Saturn's dense rings, Mach cones are only formed by dust-Alfvén waves which are found to be more prominent than any other longitudinal waves (e.g., dust-acoustic waves). The dust-Alfvénic Mach cones that we have reported here are expected to be observed in Saturn's rings by CASSINI, arriving at Saturn in 2004.

Creators(s): Shukla, P. K., Mamun, A. A. and Bingham, R. ORCID logoORCID: https://orcid.org/0000-0002-9843-7635;
Item type:Article
ID code:52012
Keywords:Saturn, magnetohydrodynamic waves, rings, dust, acoustic wave propagation, astrophysics, magnetoacoustic effects, plasma density, Plasma physics. Ionized gases, Atomic and Molecular Physics, and Optics, Mathematical Physics, Condensed Matter Physics
Subjects:Science > Physics > Plasma physics. Ionized gases
Department:Faculty of Science > Physics
Depositing user: Pure Administrator
Date deposited:03 Mar 2015 09:25
Last modified:20 Jan 2021 21:53
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URI:https://strathprints.strath.ac.uk/id/eprint/52012
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