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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2003, Volume 77, Issue 10, Pages 644–648
(Mi jetpl2817)
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This article is cited in 25 scientific papers (total in 25 papers)
Dust-Alfvén Mach Cones in Saturn's Dense Rings
A. A. Mamuna, P. K. Shuklaa, R. Binghamb a Institut für Theoretische Physik IV, Ruhr-Universität Bochum
b Rutherford Appletion Laboratory
Abstract:
The formation of Mach cones associated with dust-Alfvén waves in Saturn's dense rings has been theoretically investigated. 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 characteristics of the dust-Alfvén Mach cones that are found to be formed in Saturn's dense rings are also presented. The dusty plasma model, dust-Alfvén waves, and dust-Alfvén Mach cones that we predict in our present letter are expected to be observed in Saturn's dense rings by the imaging and occultation experiments on board the NASA/ESA space mission CASSINI, arriving at Saturn in 2004.
Received: 20.03.2003
Citation:
A. A. Mamun, P. K. Shukla, R. Bingham, “Dust-Alfvén Mach Cones in Saturn's Dense Rings”, Pis'ma v Zh. Èksper. Teoret. Fiz., 77:10 (2003), 644–648; JETP Letters, 77:10 (2003), 541–545
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https://www.mathnet.ru/eng/jetpl2817 https://www.mathnet.ru/eng/jetpl/v77/i10/p644
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Abstract page: | 138 | Full-text PDF : | 47 | References: | 33 |
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