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Alexandre Fournier
Researcher at Institut de Physique du Globe de Paris
Publications - 84
Citations - 4380
Alexandre Fournier is an academic researcher from Institut de Physique du Globe de Paris. The author has contributed to research in topics: Earth's magnetic field & Dynamo. The author has an hindex of 31, co-authored 79 publications receiving 3502 citations. Previous affiliations of Alexandre Fournier include Paris Diderot University & Princeton University.
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Journal ArticleDOI
International Geomagnetic Reference Field: the 12th generation
Erwan Thébault,Christopher C. Finlay,Ciaran Beggan,Patrick Alken,Patrick Alken,Julien Aubert,Olivier Barrois,François Bertrand,T. Bondar,A. Boness,Laura Brocco,Elisabeth Canet,Aude Chambodut,Arnaud Chulliat,Arnaud Chulliat,Pierdavide Coïsson,François Civet,Aimin Du,Alexandre Fournier,Isabelle Fratter,Nicolas Gillet,Brian Hamilton,Mohamed Hamoudi,Mohamed Hamoudi,Gauthier Hulot,Thomas Jager,Monika Korte,Weijia Kuang,Xavier Lalanne,Benoit Langlais,Jean-Michel Leger,Vincent Lesur,F. J. Lowes,Susan Macmillan,Mioara Mandea,Chandrasekharan Manoj,Chandrasekharan Manoj,Stefan Maus,Nils Olsen,Valeriy G. Petrov,Victoria Ridley,Martin Rother,Terence J. Sabaka,Diana Saturnino,Reyko Schachtschneider,Olivier Sirol,Andrew Tangborn,Alan Thomson,Lars Tøffner-Clausen,Pierre Vigneron,Ingo Wardinski,Tatiana I. Zvereva +51 more
TL;DR: The 12th generation of the International Geomagnetic Reference Field (IGRF) was adopted in December 2014 by the Working Group V-MOD appointed by the International Association of Geomagnetism and Aeronomy (IAGA) as discussed by the authors.
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Fast torsional waves and strong magnetic field within the Earth’s core
TL;DR: Numerical geodynamo models with studies of geostrophic motions in the Earth’s core that rely on geomagnetic data reconcile, finding a torsional wave recurring every six years from an ensemble inversion of core flow models.
Journal ArticleDOI
AxiSEM: broadband 3-D seismic wavefields in axisymmetric media
Tarje Nissen-Meyer,M. van Driel,Simon Stähler,Kasra Hosseini,Stefanie Hempel,Ludwig Auer,Andrea Colombi,Alexandre Fournier +7 more
TL;DR: In this article, the authors present a methodology to compute 3D global seismic wavefields for realistic earthquake sources in visco-elastic anisotropic media, covering applications across the observable seismic frequency band with moderate computational resources.
Journal ArticleDOI
International Geomagnetic Reference Field: the thirteenth generation
Patrick Alken,Patrick Alken,Erwan Thébault,Ciaran Beggan,Hagay Amit,Julien Aubert,Julien Baerenzung,T. Bondar,William R. Brown,S. Califf,S. Califf,Aude Chambodut,Arnaud Chulliat,Arnaud Chulliat,Grace Cox,Christopher C. Finlay,Alexandre Fournier,Nicolas Gillet,Alexander Grayver,Magnus Danel Hammer,Matthias Holschneider,Loïc Huder,Gauthier Hulot,Thomas Jager,Clemens Kloss,Monika Korte,Weijia Kuang,Alexey Kuvshinov,Benoit Langlais,Jean-Michel Leger,Vincent Lesur,Philip W. Livermore,F. J. Lowes,Susan Macmillan,Werner Magnes,Mioara Mandea,Santiago Marsal,J. Matzka,M. C. Metman,Takuto Minami,Takuto Minami,Achim Morschhauser,J. E. Mound,M. C. Nair,M. C. Nair,Shin'ya Nakano,Nils Olsen,Fco. Javier Pavón-Carrasco,Fco. Javier Pavón-Carrasco,Valeriy G. Petrov,Guillaume Ropp,Martin Rother,Terence J. Sabaka,Sabrina Sanchez,Diana Saturnino,N. R. Schnepf,N. R. Schnepf,Xuhui Shen,Claudia Stolle,Andrew Tangborn,Lars Tøffner-Clausen,Hiroaki Toh,Joan Miquel Torta,J. Varner,J. Varner,Foteini Vervelidou,Pierre Vigneron,Ingo Wardinski,Johannes Wicht,A. Woods,A. Woods,Yanyan Yang,Z. Zeren,Bin Zhou +73 more
TL;DR: The International Geomagnetic Reference Field (IGRF) was adopted by the IGA Division V Working Group (V-MOD) in 2019 as discussed by the authors, which provides the equations defining the IGRF, the spherical harmonic coefficients for this thirteenth generation model, maps of magnetic declination, inclination, and total field intensity for the epoch 2020.0, and maps of their predicted rate of change for the 2020 to 2025.0 time period.
Journal ArticleDOI
Turbulent geodynamo simulations: a leap towards Earth's core
TL;DR: In this paper, a sequence of three convection-driven simulations in a rapidly rotating spherical shell is used to reach realistic turbulent regime in direct numerical simulations of the geodynamo.