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dc.contributor.authorBecker, TMen_US
dc.contributor.authorColwell, JEen_US
dc.contributor.authorEsposito, LWen_US
dc.contributor.authorAttree, NOen_US
dc.contributor.authorMurray, CDen_US
dc.date.accessioned2018-03-29T09:54:42Z
dc.date.accessioned2018-04-03T12:54:19Z
dc.date.available2018-02-02en_US
dc.date.issued2018-05-15en_US
dc.date.submitted2018-03-13T19:23:07.898Z
dc.date.submitted2018-03-29T14:07:45.447Z
dc.identifier.issn0019-1035en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/36171
dc.description.sponsorshipThis material is based upon work supported by the National Aeronautics and Space Administration under grants NNX10AF20G and NNX15AH22G issued through the Cassini Data Analysis Program and through the Cassini Project on a grant issued through JPL to the UVIS investigation. This work was also supported by the NASA Florida Space Grant Consortium. C.M. was supported by the UK Science and Technology Facilities Council (Grant No. ST/M001202/1) and is grateful to them for financial assistance. N.A. is grateful to the UK Science and Technology Facilities Council for the award of a PhD studentship.
dc.format.extent171 - 199en_US
dc.relation.ispartofICARUSen_US
dc.relation.replaceshttp://qmro.qmul.ac.uk/xmlui/handle/123456789/36145
dc.relation.replaces123456789/36145
dc.subjectPlanetary ringsen_US
dc.subjectOccultationsen_US
dc.subjectSaturnen_US
dc.titleCassini UVIS solar occultations by Saturn's F ring and the detection of collision-produced micron-sized dusten_US
dc.typeArticle
dc.rights.holder© 2018 Elsevier Inc.
dc.identifier.doi10.1016/j.icarus.2018.02.006en_US
pubs.author-urlhttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000429082000013&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume306en_US


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