Geology

dc.creatorKnipping, J.
dc.creatorBilenker, L.
dc.creatorSimon, A.
dc.creatorReich, M.
dc.creatorBarra, F.
dc.creatorDeditius, A.
dc.creatorLundstrom, Bin-deman, I.
dc.creatorMunizaga, R.
dc.date2020-03-11T20:26:50Z
dc.date2022-07-07T23:45:02Z
dc.date2020-03-11T20:26:50Z
dc.date2022-07-07T23:45:02Z
dc.date2015
dc.date.accessioned2023-08-21T22:42:45Z
dc.date.available2023-08-21T22:42:45Z
dc.identifier15090013
dc.identifier15090013
dc.identifierhttps://hdl.handle.net/10533/238118
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8291410
dc.descriptionKiruna-type iron oxide–apatite (IOA) deposits are an important source of Fe ore, and two radically different processes are being actively investigated for their origin. One hypothesis invokes direct crystallization of immiscible Fe-rich melt that separate
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1130/G36650.1
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleGiant Kiruna-type deposits form by efficient flotation of magmatic magnetite suspensions
dc.titleGeology
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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