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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3788
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dc.contributor.authorVasundhara, R-
dc.contributor.authorBhattacharyya, J. C-
dc.contributor.authorSanthanam, P-
dc.contributor.authorPande, A. K-
dc.contributor.authorMohan, V-
dc.contributor.authorMahra, H-
dc.date.accessioned2008-09-22T16:29:57Z-
dc.date.available2008-09-22T16:29:57Z-
dc.date.issued1984-12-
dc.identifier.citationNature, Vol. 312, No. 5995, pp. 621 - 623en
dc.identifier.issn0028-0836-
dc.identifier.urihttp://hdl.handle.net/2248/3788-
dc.descriptionRestricted Access-
dc.description.abstractThe region of the magnetosphere of Saturn around 14 radii and 19 radii has been of special interest since the detection of anomalous dips in the low-energy plasma ion-density in these regions by the Voyager 1, Voyager 2 and Pioneer 11 spacecrafts. The authors have observed the occultation of the star SAO158913 from two stations in India following predictions by Mink. This star showed symmetric dips in the light curves on 24 March 1984 (immersion event) and on 25 March 1984 (emersion event), suggesting the possible presence of particulate matter.en
dc.language.isoenen
dc.publisherNature Publishing Groupen
dc.relation.urihttp://dx.doi.org/10.1038/312621a0en
dc.subjectSaturn's Magnetosphereen
dc.subjectEnergy Plasma Ion-Densityen
dc.subjectPioneer 11 Spacecraftsen
dc.subjectOccultation of the Staren
dc.subjectLight Curvesen
dc.titlePossible Detection of a Ring System in Saturn's Magnetosphereen
dc.typeArticleen
Appears in Collections:IIAP Publications
J.C.Bhattacharyya (1982 - 1990)

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