Andean Geology is becoming an English-language journal
This transition will be effective starting July 1, 2026. All submissions but obituaries and comments, and those part of special issues, will be required to be submitted in English
Call for Papers
Special Issue: Advances in Paleontology in Chile: Opportunities and Challenges for a Synthesis
Edited by:
- Marcelo Rivadeneira, CEAZA
- Enrique Bostelmann, Sernageomin
- Martín Chávez-Hoffmeister, CIAHN
- Joseline Manfroi, CIAHN
- Philippe Moisan, Universidad de Atacama
- Karen Moreno, Universidad Austral de Chile
- Sven Nielsen, Universidad Austral de Chile
- Ana Valenzuela-Toro, CIAHN
- Natalia Villavicencio, Universidad de O'Higgins
Submission status: Open between March 1, 2026, and November 30, 2026
Read more (pdf)
About The Authors
Camilo Bustamante
Departamento de Ciencias de la Tierra, Universidad EAFIT, Carrera 49 No. 7 Sur-50, Medellín, Colombia. Colombia
Carlos J. Archanjo
Instituto de Geociências, Universidade de São Paulo, Rua do Lago 562, CEP 05508-080, São Paulo, Brasil. Brazil
Agustin Cardona
Departamento de Procesos y Energía, Facultad de Minas, Universidad Nacional, Carrera 80, 65-223, Medellín, Colombia. Colombia
Marcela Restrepo
Departamento de Ciencias de la Tierra, Universidad EAFIT, Carrera 49 No. 7 Sur-50, Medellín, Colombia. Colombia
Magnetic fabric of the Parashi stock and related dyke swarm, Alta Guajira (Colombia): The Caribbean-South American plates oblique convergence
Camilo Bustamante, Carlos J. Archanjo, Agustin Cardona, Marcela Restrepo
Abstract
Anisotropy of magnetic susceptibility (AMS) and anhysteretic remanence (AAR) were used to evaluate the emplacement history of the Parashi stock and related dyke swarm situated in NW Colombia. The average magnetic susceptibility of 4.5×10-2 SI, in conjunction with low-coercivity components provided by the isothermal remanence and thermomagnetic curves with net Verwey and Curie transitions, indicates that multidomain magnetite records the anisotropy directions. The similar orientation and shape of the AMS and AAR ellipsoids indicate the absence of very fine magnetite with an inverse fabric. The magnetic foliation is the best-defined fabric element in these rocks and outlines a concentric structure, elongated parallel to the NE-SW direction of the pluton. Crystallisation age of the stock and dykes (51-47 Ma), along with pressure of emplacement determination indicate that the stock and the dyke swarm probably formed simultaneously, and they were emplaced in the shallow crust (<10 km). The magnetic fabric agrees with emplacement in a transtensional setting, with the dyke swarm infilling tensional cracks formed during the final stages of pluton crystallisation. This tectonic setting likely records the difficulty of the thick oceanic crust subducting, which would result in general transtension in the overriding continental plate and cessation of arc magmatism in the Eocene.