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Paleomagnetic constraints on an Archean-Paleoproterozoic Superior-Karelia connection: New evidence from Archean Karelia

机译:太古宙古古生界上卡累利阿连接的古地磁约束:太古宙卡累利阿的新证据

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Charno-enderbitic granitoids in the Karelia craton of the Fennoscandian shield have been studied paleomagnetically. The characteristic remanence component has a steep negative inclination and is interpreted to record magnetization at a maximum age of 2684 ± 2 Ma. Consistently stable results were obtained from 12 sites in the Koitere area, corresponding to regions with high positive magnetic anomalies and high remanence intensities. Petrographic studies, coupled with rock magnetic investigations, indicate that the remanence resides in fine SD/PSD magnetite grains formed during Neoarchean clinopyroxene alteration. Cross-cutting vertical/subvertical Paleoproterozoic dolerite dykes suggest that the Koitere granitoids are in their original orientations and were not affected by Svecofennian deformation at ca. 1.9-1.8. Ga. The Koitere granitoids have an opposite polarity compared to the steep positive inclination remanence direction of the previously studied ca. 2.63. Ga Varpaisj?rvi enderbites and granulites. The data from Koitere and Varpaisj?rvi imply that at ca. 2.7-2.6. Ga the Karelia craton was located at high latitudes of 80-60°, whereas previous paleomagnetic data from ca. 2.5. Ga formations in the Vodlozero terrane in NW Russia indicate a near-equatorial position. Comparison of paleomagnetic data from the Koitere and Varpaisj?rvi granulite-grade rocks with rocks of similar age in the Superior craton shows that at ca. 2.7-2.6. Ga the Superior and Karelia cratons were located at high latitudes and in close proximity, although the present data cannot demonstrate that the cratons were amalgamated. However, during the Archean-Paleoproterozoic transition at ca. 2.50. Ga both cratons experienced significant rotation and drifting to near-equatorial paleolatitudes, suggesting that the Superior and Karelia cratons may have been attached at that time.
机译:芬诺斯堪的纳维亚盾的卡累利阿克拉通中的Charno-低位花岗岩。特征剩磁分量具有陡峭的负倾角,并被解释为记录最大年龄2684±2 Ma的磁化强度。从Koitere地区的12个地点获得了稳定的结果,对应于具有高正磁异常和高剩磁强度的区域。岩相学研究以及岩石磁学研究表明,剩磁存在于新古宙纪次氯环比蚀变中形成的精细SD / PSD磁铁矿晶粒中。横切的垂直/亚垂直古元古代白云岩堤坝表明,Koitere花岗岩处于其原始方向,并且不受斯威科芬尼亚变形的影响。 1.9-1.8。与先前研究的ca的陡峭正倾角剩磁方向相比,Koitere花岗岩具有相反的极性。 2.63。 Ga Varpaisj?rvi牙石和花岗石。来自Koitere和Varpaisj?rvi的数据表明,大约在2.7-2.6。 Ga卡累利阿克拉通位于高纬度80-60°,而先前的古磁数据来自ca。 2.5。俄罗斯西北部Vodlozero地层中的Ga层表示接近赤道位置。比较来自上克拉通的Koitere和Varpaisj?rvi粒级岩石与年龄相似的岩石的古磁数据,发现在2.7-2.6。 Ga上级和卡累利阿(Karelia)克拉通位于高纬度且紧邻,尽管目前的数据无法证明克拉通已合并。然而,在大约从太古宙古生代过渡期。 2.50。 Ga的两个克拉通都经历了明显的旋转并漂移到近赤道古纬度,表明当时可能已附着了上克拉通和卡累利阿克拉通。

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