Preferred locations of weak surface field in numerical dynamos with heterogeneous core–mantle boundary heat flux: consequences for the South Atlantic Anomaly

Author:

Terra-Nova Filipe12ORCID,Amit Hagay2,Choblet Gaël2ORCID

Affiliation:

1. Departamento de Geofísica, Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226, Cidade Universitária, 05508-090 São Paulo, Brasil

2. CNRS, Université de Nantes, Nantes Atlantiques Universités, UMR CNRS 6112, Laboratoire de Planétologie et de Géodynamique, 2 rue de la Houssinière, F-44000 Nantes, France

Funder

National Council for Scientific and Technological Development

São Paulo Research Foundation

Publisher

Oxford University Press (OUP)

Subject

Geochemistry and Petrology,Geophysics

Reference79 articles.

1. Can downwelling at the top of the Earth’s core be detected in the geomagnetic secular variation?;Amit;Phys. Earth planet. Inter.,2014

2. Stationary, oscillating or drifting mantle-driven geomagnetic flux patches?;Amit;J. geophys. Res.,2010

3. A simple model for mantle-driven flow at the top of Earth’s core;Amit;Earth Planets Space,2008

4. Mantle-driven geodynamo features - effects of compositional and narrow D” anomalies;Amit;Earth Planet. Inter,2012

5. Towards more realistic core-mantle boundary heat flux patterns: a source of diversity in planetary dynamos;Amit;Prog. Earth planet. Sci.,2015

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