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DOI10.1016/j.tecto.2020.228386
Paleogeographic and tectonic evolution of the Pampia Terrane in the Cambrian: New paleomagnetic constraints
Franceschinis P.R.; Rapalini A.E.; Escayola M.P.; Rodríguez Piceda C.
发表日期2020
ISSN00401951
卷号779
英文摘要Paleomagnetic, magnetic fabric and rock magnetic studies were carried out in the late Middle to early Late Cambrian Campanario Formation exposed in NW Argentina. The study also presents preliminary results from the Early Cambrian metasediments of the Puncoviscana Formation and from Mojotoro intrusive. A new paleomagnetic pole, C2, was computed for the Campanario Formation (23.6°N, 346.5°E, A95, 7.0°, N: 11 sites) from the localities of Tilcara (T), Terma de Reyes (R) and El Perchel (EP), including previous data from Santa Victoria Oeste (M), in northernmost Argentina. A positive fold test was obtained for Tilcara locality while a positive regional tilt test was obtained for mean site directions for the four localities. This pole can be considered as the representative pole position for the Pampia terrane for the late Middle to Late Cambrian. Previous paleomagnetic data for the same formation from the Iruya-Matancillas locality show an in situ clockwise rotation of about 30° around a vertical axis when compared with the mean Pampia pole. The same is observed when comparing the early Ordovician pole for the Santa Rosita Formation at those localities with the recently obtained coeval pole of the La Pedrera Formation, indicating that local tectonic rotations, affected that area. These results suggest that previous paleomagnetic interpretations for these Late Cambrian and Early Ordovician rocks in the region as recording displacement of the Pampia terrane in Cambrian times are probably incorrect. Additionally, two virtual geomagnetic poles were computed for the Puncoviscana Formation (TP1: 34.5°N, 52.3°E, A95: 5.0°, n: 22 specimens and TP2: 38.3°N, 33.6°E, A95: 5.7°, n: 14 specimens) and one for the Mojotoro Intrusive (MO: 9.1°N, 345.6°E, A95: 16.4°, n: 11 specimens). These and previous Early Cambrian paleomagnetic data from the Pampia terrane differ from Gondwana coeval reference directions in inclination and/or declination, lacking a simple pattern. © 2020 Elsevier B.V.
关键词Campanario FormationGondwanaPampia TerranePuncoviscana Formation
英文关键词Geomagnetism; Lithology; Campanario Formation; Clockwise rotation; Gondwana; Paleomagnetic data; Paleomagnetic poles; Pampia Terrane; Puncoviscana Formation; Tectonic evolution; Tectonics; Rosita
语种英语
来源期刊Tectonophysics
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/207753
作者单位Universidad de Buenos Aires, Laboratorio de Paleomagnetismo Daniel A. Valencio, Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires (IGEBA), Departamento de Ciencias Geológicas, Facultad de Ciencias Exactas y Naturales, Argentina; CONICET, Argentina; ICPA-Universidad Nacional de Tierra del FuegoAntártida e Islas del Atlántico Sur, Argentina; Institut für Geowissenschaften, Universität Potsdam, Potsdam, Germany; GFZ – German Research Center for Geosciences, Potsdam, Germany
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GB/T 7714
Franceschinis P.R.,Rapalini A.E.,Escayola M.P.,et al. Paleogeographic and tectonic evolution of the Pampia Terrane in the Cambrian: New paleomagnetic constraints[J],2020,779.
APA Franceschinis P.R.,Rapalini A.E.,Escayola M.P.,&Rodríguez Piceda C..(2020).Paleogeographic and tectonic evolution of the Pampia Terrane in the Cambrian: New paleomagnetic constraints.Tectonophysics,779.
MLA Franceschinis P.R.,et al."Paleogeographic and tectonic evolution of the Pampia Terrane in the Cambrian: New paleomagnetic constraints".Tectonophysics 779(2020).
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