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Mioara Mandea

Researcher at Centre National D'Etudes Spatiales

Publications -  181
Citations -  7749

Mioara Mandea is an academic researcher from Centre National D'Etudes Spatiales. The author has contributed to research in topics: Earth's magnetic field & Secular variation. The author has an hindex of 41, co-authored 167 publications receiving 6798 citations. Previous affiliations of Mioara Mandea include Institut de Physique du Globe de Paris & Paris Diderot University.

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International Geomagnetic Reference Field: the 12th generation

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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International Geomagnetic Reference Field: the eleventh generation

Abstract: The eleventh generation of the International Geomagnetic Reference Field (IGRF) was adopted in December 2009 by the International Association of Geomagnetism and Aeronomy Working Group V-MOD. It updates the previous IGRF generation with a definitive main field model for epoch 2005.0, a main field model for epoch 2010.0, and a linear predictive secular variation model for 2010.0–2015.0. In this note the equations defining the IGRF model are provided along with the spherical harmonic coefficients for the eleventh generation. Maps of the magnetic declination, inclination and total intensity for epoch 2010.0 and their predicted rates of change for 2010.0–2015.0 are presented. The recent evolution of the South Atlantic Anomaly and magnetic pole positions are also examined.
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Small-scale structure of the geodynamo inferred from Oersted and Magsat satellite data

TL;DR: Data from the currently operating Danish Oersted satellite and from the US Magsat satellite are used to identify and interpret variations in the magnetic field over the past 20 years, down to length scales previously inaccessible.
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CHAOS—a model of the Earth's magnetic field derived from CHAMP, Ørsted, and SAC‐C magnetic satellite data

TL;DR: In this paper, the authors derived a model of the near-Earth magnetic field (up to spherical harmonic degree n = 50 for the static field, and up to n = 18 for the first time derivative) using more than 6.5 yr of high-precision geomagnetic measurements from the three satellites Orsted, CHAMP and SAC-C taken between 1999 March and 2005 December.
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Crustal magnetic field of Mars

TL;DR: In this article, the equivalent source dipole technique is used to model the three components of the Martian lithospheric magnetic field, including the magnetization, magnetic field directions, and magnetization intensity.