Strange attractors in the Saturn ring system

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Strange attractors in the Saturn ring system

Show simple item record Lalaja, V Nampoori, V P N Pratap, R 2011-12-09T10:37:28Z 2011-12-09T10:37:28Z 1989-02
dc.identifier.issn 0167-9295
dc.identifier.issn Earth, Moon, and Planets , vol. 44, Feb. 1989, p. 105-119.
dc.description.abstract The theory of deterministic chaos is used to study the three rings A, B, and C of Saturn and the French and Cassini divisions in between them. The data set comprises Voyager photopolarimeter measurements. The existence of spatially distributed strange attractors is shown, implying that the system is open, dissipative, nonequilibrium, and non-Markovian in character. en_US
dc.description.sponsorship Cochin University of Science and Technology en_US
dc.language.iso en en_US
dc.publisher Kluwer Academic Publishers en_US
dc.subject Planetary Environments en_US
dc.subject Saturn Rings en_US
dc.subject Strange Attractors en_US
dc.subject Chaos en_US
dc.subject Markov Processes en_US
dc.subject Solar System en_US
dc.subject Spatial Distribution en_US
dc.subject Yoyager Project en_US
dc.title Strange attractors in the Saturn ring system en_US
dc.type Working Paper en_US
dc.contributor.faculty Technology en_US
dc.identifier.url DOI: 10.1007/BF00056311 en_US

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