Indications of twist in the Epsilon rings of Uranus

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DC Field	Value	Language
dc.contributor.author	Vasundhara, R	-
dc.contributor.author	Bhattacharyya, J. C	-
dc.date.accessioned	2013-09-16T16:07:05Z	-
dc.date.available	2013-09-16T16:07:05Z	-
dc.date.issued	1982	-
dc.identifier.citation	Brahic, A., ed., Planetary rings, International Astronomical Union Colloque No. 75, pp. 193 - 195	en
dc.identifier.uri	http://hdl.handle.net/2248/6353	-
dc.description	Open Access	en
dc.description.abstract	The possibility of the Uranus epsilon ring having a structure consisting of a twisted bundle of narrow lanes of condensed material similar to that of Saturn's F ring was examined by cross correlation of a pair of light curves for the same event from neighboring sections of the ring. The result supports the hypothesis.	en
dc.language.iso	en	en
dc.publisher	Centre national D Etudes Spatiales	en
dc.relation.ispartofseries	International Astronomical Union Colloque;75	-
dc.relation.uri	http://labs.adsabs.harvard.edu/ui/abs/1984plri.coll..193V	en
dc.rights	© Centre national D Etudes Spatiales	en
dc.subject	Orbits	en
dc.subject	Twisting	en
dc.subject	Uranus ring	en
dc.subject	Cross correlation	en
dc.subject	Light curves	en
dc.subject	Saturn rings	en
dc.title	Indications of twist in the Epsilon rings of Uranus	en
dc.type	Article	en
Appears in Collections:	IIAP Publications J.C.Bhattacharyya (1982 - 1990)

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