georefid:2006-021128SEDIS Publication Catalogueana.macario@awi.dehttp://sedis.iodp.org/pub-catalogue/informationpointOfContact2011-06-23T00:00:00Zhttp://sedis.iodp.org/pub-catalogue/index.php?id=2006-021128<gco:CharacterString>Kinematics of the Campanian-Maastrichtian island arcs in northeastern Asia in light of drilling results on the Emperor Seamounts</gco:CharacterString>2005-01-01publicationgeorefid:2006-021128Shapiro, M. N.Russian Academy of Sciences, Institute of Physics of the Earth, Moscow, Russian FederationauthorMAIK Nauka/Interperiodica Publishing, Birmingham, AL, United StatespublisherdocumentHardcopyGeotectonics39 (5)408-415The southward drift of the Hawaiian hotspot established by drilling on the Emperor Seamounts was not significant enough to suggest that the northern Emperor Seamounts and the Cretaceous island-arc sequences in the Olyutor-Kamchatka region were located at similar paleomagnetic latitudes. Furthermore, the obvious differences in the Late Cretaceous sedimentation on the Emperor Seamounts and in Kamchatka paleoarcs are caused not only by differences in their paleolatitudes. Therefore, the drilling results provide no serious grounds to revise the concept of substantial northern drift of the Cretaceous island arcs.completedSolid-earth geophysicsStratigraphyAsiabiostratigraphyboreholesCampanianCommonwealth of Independent StatesCretaceousEast Pacific Ocean IslandsEmperor SeamountsHawaiihot spotsInvertebrataisland arcsKamchatka PeninsulaLeg 145Leg 197MaestrichtianMesozoicmicrofossilsNorth PacificNorthwest PacificOcean Drilling ProgramOceaniaPacific Oceanpaleogeographypaleolatitudepaleomagnetismplate tectonicsPolynesiaProtistaRadiolariaRussian FederationRussian Pacific regionSenonianUnited StatesUpper CretaceousWest Pacificurn:org.iodp:exp:145urnlargerWorkCitationcampaignurn:org.iodp:exp:197urnlargerWorkCitationcampaignEnglishgeoscientificInformation-180.0000-140.000020.000050.0000