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Titel Depth to Curie temperature or magnetic sources bottom in the volcanic zone of La Réunion hot spot
VerfasserIn Lydie-Sarah Gailler, Jean-François Lénat, Richard J. Blakely
Konferenz EGU General Assembly 2015
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 17 (2015)
Datensatznummer 250106390
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2015-6060.pdf
 
Zusammenfassung
We present an innovative study to generalize Curie Point Depth (CPD) determinations at the scale of oceanic volcanic islands, an approach heretofore largely focused on continental areas. In order to assert the validity of this technique in oceanic environments, we first test the Tanaka et al. (1999) approach on sets of oceanic ridges anomalies. Assuming that magnetic anomalies are concentrated within the oceanic crust and maybe part of the underlying upper mantle, the Curie depth should become deeper as the oceanic lithosphere becomes older (i.e. thicker). The calculated depths to magnetic bottom are in agreement with this general pattern. Using the growing assumption of a magnetized upper mantle, we consider that the method can be confidently used in the case of La Réunion Island and its surrounding oceanic lithosphere. We use the magnetic anomaly map computed by Gailler and Lénat (2010), completed and extended with the global Earth Magnetic Anomaly Grid (EMAG2) (Maus et al., 2007). The calculated magnetic sources bottom lies at depths between 10 and 29 km and exhibits a complex topography, presumably caused by the combination of various magmatic and tectonic crustal structures. To the first order, the magnetic bottom surface shallows beneath La Réunion and Mauritius Islands, suggesting a thermal effect of the hot spot, and deepens away from La Réunion edifice. At the scale of the Mascarene Basin, several discontinuities in CPD are well correlated with main fracture zones.