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dc.date.accessioned2013-03-12T09:02:05Z
dc.date.available2013-03-12T09:02:05Z
dc.date.issued2006en_US
dc.date.submitted2006-02-01en_US
dc.identifier.citationSkaten, Maren Kristin Møllerup. The Lillehammer Submarine Fan Complex. Masteroppgave, University of Oslo, 2006en_US
dc.identifier.urihttp://hdl.handle.net/10852/12396
dc.description.abstractAbstract The Lillehammer Submarine Fan Complex is a mixed mud/sand rich turbidite fan system. The fan complex was deposited in the Neoproterozoic Hedmark rift basin from west towards east extending at least 50 km from the basin margin. A detailed sedimentary study of outcrops in the Lillehammer area is performed with the aim of analyzing the depositional environment as an analogue for subsurface turbidite systems. Seven sedimentary logs cover a nearly 1000 meter thick stratigraphic section. Seven facies have been organized into seven facies associations, representing architectural elements including basin plain-thin bedded turbidites, basin plain-hemipelagic shale, lobe, lobe-channel, basin floor channel infill, major channel and channel-levee. The Lillehammer Submarine Fan Complex represents two or three fan systems, separated by hemipelagic black shale or thick unit of homogenous shale that may indicate rise in relative sea level. The overall system is progradational and represents an outer and middle to inner fan environment. The main factors controlling the development of the Lillehammer Submarine Fan Complex are thought to be tectonic activity at the basin margin and sediment influx. Comparison of the Lillehammer Submarine Fan Complex with the Upper Cretaceous fans in the Vøring Basin reveals a good geometrical resemblance despite large differences in sandstone petrography and clay matrix content. The petrographic more impure and clay-rich sandstones of the Lillehammer Submarine Fan Complex, as compared with those in the Vøring Basin, is interpreted to be related to differences in provenance and basin structure. Synthetic seismograms were performed for a 400 meter thick logged section to discuss the differences in seismic resolution under 1500 meter of overload and 3500 meter of overload. Only half of the seismic events are shown in the deepest model compared to the shallow model. Reflections associated with most interfaces are recognizable, but difficult to distinguish from each other. The shallow model reveals good seismic resolution of two fans separated by a thick layer of homogenous shale. The same model under a thicker overload does not have the same obvious trends, but is recognizable when you know what to expect.nor
dc.language.isoengen_US
dc.subjectgeofysikk petroleumsgeologi geologi submarin-vifte dypmarin gravitasjonsstrømmer seismisk modeleringen_US
dc.titleThe Lillehammer Submarine Fan Complexen_US
dc.typeMaster thesisen_US
dc.date.updated2006-02-10en_US
dc.creator.authorSkaten, Maren Kristin Møllerupen_US
dc.subject.nsiVDP::450en_US
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&rft.au=Skaten, Maren Kristin Møllerup&rft.title=The Lillehammer Submarine Fan Complex&rft.inst=University of Oslo&rft.date=2006&rft.degree=Masteroppgaveen_US
dc.identifier.urnURN:NBN:no-11725en_US
dc.type.documentMasteroppgaveen_US
dc.identifier.duo35845en_US
dc.contributor.supervisorJohan Petter Nystuen, Leif J. Geliusen_US
dc.identifier.bibsys060250801en_US
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/12396/1/skaten.pdf


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