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dc.contributor.authorBjørlykke, Knut
dc.coverage.spatial19161 Løten
dc.coverage.spatial20173 Julussa
dc.coverage.spatial19173 Åsmarka
dc.coverage.spatial19172 Rena
dc.coverage.spatialELVERUM
dc.coverage.spatialHAMAR
dc.coverage.spatialÅMOT
dc.date.accessioned2020-08-26T13:01:44Z
dc.date.available2020-08-26T13:01:44Z
dc.date.issued1966
dc.identifier.urihttps://hdl.handle.net/11250/2674835
dc.description.abstractSediments of the Sparagmite group (Eocambrian\/latest Precambrian) have been mapped at a scale of 1:50 000 in the Rena district, 180 km north of Oslo. This district is located along the southern margin of the Sparagmite basin which is down-faulted in the crystalline Precambrian basement. The sediments are made up by a series of conglomeratic arkoses interlayered with shales and limestones. Toward the top of the Sparagmite group the arkoses grade into a quartzite which is overlain by a thin conglomeratic layer of granules which forms the base of fossiliferous Cambrian (Holmian series). The evidence for an Eocambrian glaciation existing in the Moelv tillite is discussed in the light of grain size and fabric analyses. Model analyses and flamephotometric determinations of sodium and potassium content in the sandstones show decreasing sodium\/potassium and plagioclase\/microcline ratio as the total feldspar content decreases towards the upper formation in the Sparagmite group. Spectrographic boron analyses suggest marine conditions during the deposition of the Sparagmite group, even if the analytical error of these analyses is rather high.
dc.language.isoeng
dc.relation.ispartofseriesNGU (238)
dc.rightsNavngivelse 4.0 Internasjonal
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no
dc.subjectKARTLEGGING
dc.subjectPETROLOGI
dc.subjectSPARAGMITT
dc.subjectSEDIMENTÆR BERGART
dc.subjectTEKTONIKK
dc.titleSedimentary petrology of the Sparagmites of the Rena district, S. Norway.
dc.typeJournal article
dc.description.localcode35216
dc.source.pagenumber5-54


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