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8. A New Model of the Crustal Magnetic Field of Mars Using MGS and MAVEN

Author

Langlais, Benoit, Thébault, Erwan, Houliez, Aymeric, Purucker, Michael E, and Lillis, Robert J

Subjects
Lunar And Planetary Science And Exploration
Abstract

While devoid of an active magnetic dynamo field today, Mars possesses a remanent magnetic field that may reach several thousand nanoteslas locally. The exact origin and the events that have shaped the crustal magnetization remain largely enigmatic. Three magnetic field data sets from two spacecraft collected over 13 cumulative years have sampled the Martian magnetic field over a range of altitudes from 90 up to 6,000 km: (a) Mars Global Surveyor (MGS) magnetometer (1997–2006), (b) MGS Electron Reflectometer (1999–2006), and (c) Mars Atmosphere and Volatile EvolutioN (MAVEN) magnetometer (2014 to today). In this paper we combine these complementary data sets for the first time to build a new model of the Martian internal magnetic field. This new model improves upon previous ones in several aspects: comprehensive data coverage, refined data selection scheme, modified modeling scheme, discrete-to-continuous transformation of the model, and increased model resolution. The new model has a spatial resolution of ∼160 km at the surface, corresponding to spherical harmonic degree 134. It shows small scales and well-defined features, which can now be associated with geological signatures.

Published
2019
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15. International Geomagnetic Reference Field: the 12th generation

Author

Thébault, Erwan, Finlay, Christopher C, Beggan, Ciarán D, Alken, Patrick, Aubert, Julien, Barrois, Olivier, Bertrand, Francois, Bondar, Tatiana, Boness, Axel, Brocco, Laura, Canet, Elisabeth, Chambodut, Aude, Chulliat, Arnaud, Coïsson, Pierdavide, Civet, François, Du, Aimin, Fournier, Alexandre, Fratter, Isabelle, Gillet, Nicolas, Hamilton, Brian, Hamoudi, Mohamed, Hulot, Gauthier, Jager, Thomas, Korte, Monika, Kuang, Weijia, Lalanne, Xavier, Langlais, Benoit, Léger, Jean-Michel, Lesur, Vincent, Lowes, Frank J, Macmillan, Susan, Mandea, Mioara, Manoj, Chandrasekharan, Maus, Stefan, Olsen, Nils, Petrov, Valeriy, Ridley, Victoria, Rother, Martin, Sabaka, Terence J, Saturnino, Diana, Schachtschneider, Reyko, Sirol, Olivier, Tangborn, Andrew, Thomson, Alan, Tøffner-Clausen, Lars, Vigneron, Pierre, Wardinski, Ingo, and Zvereva, Tatiana

Published
2015
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18. An Empirical Method for the Optimal Setting of the Potential Fields Inverse Problem.

Author

Sampietro, Daniele, Capponi, Martina, Thébault, Erwan, and Gailler, Lydie

Subjects
INVERSE problems, GRAVITY anomalies, EMPIRICAL research, GEOPHYSICAL prospecting, MAGNETIC anomalies
Abstract

The use of potential field methods for geophysical exploration purposes is nowadays quite common: these techniques consent to retrieve geological knowledge over extended regions and can give complementary information where other invasive or expensive techniques, such as seismic acquisitions, fail (e.g., in the recovery of geometries of geological horizons beneath a thick salt layer). Recent dedicated satellite gravity and magnetic missions, such as GRACE, GOCE and SWARM together with the exploitation of offshore satellite altimetry and airborne/shipborne surveys, have paved the way to the realization of a variety of global models, characterized by spatial resolutions of about 4 km (both for gravity anomaly and lithosphere magnetic anomalies) and high accuracy (about 3-5$3\text{-}5$ mGal and 20 nT). These models are a valuable source of information to study the geological evolution and characterization of the lithosphere structure, especially at a regional scale. In the present work, some preliminary technical aspects related to the use of these models to perform three‐dimensional inversion are discussed, thus defining an empirical but rigorous procedure to set up gravity and magnetic inversion. In particular, we address the questions whether the classical planar approximation is acceptable for regional inversions or if a spherical one is required. We also provide guidance for choosing the best gravity functional (e.g., gravity anomalies or second radial derivative of the anomalous potential) and the optimal sizing of the three‐dimensional volume area to be modelled depending on the specific target investigated. The application of the proposed methods to the Mediterranean case study is also presented. [ABSTRACT FROM AUTHOR]

Published
2023
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20. A lithospheric magnetic field model to spherical harmonic degree 1300

Author

Thébault, Erwan, Hulot, Gauthier, THEBAULT, ERWAN, Laboratoire Magmas et Volcans (LMV), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement et la société-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Observatoire de Physique du Globe de Clermont-Ferrand (OPGC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Institut de Physique du Globe de Paris (IPGP (UMR_7154)), and Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)

Subjects
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph], [SDU.STU.GP] Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]
Abstract

International audience

Published
2022

21. A Spherical Harmonic Model of Earth's Lithospheric Magnetic Field up to Degree 1050

Author

Thébault, Erwan, Hulot, Gauthier, Langlais, Benoit, THEBAULT, ERWAN, Laboratoire Magmas et Volcans (LMV-ENSMSE), École des Mines de Saint-Étienne (Mines Saint-Étienne MSE), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-SPIN-Centre National de la Recherche Scientifique (CNRS)-Laboratoire Magmas et Volcans (LMV), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement et la société-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Observatoire de Physique du Globe de Clermont-Ferrand (OPGC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement et la société-Université Clermont Auvergne (UCA)-Observatoire de Physique du Globe de Clermont-Ferrand (OPGC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Institut de Physique du Globe de Paris (IPGP (UMR_7154)), Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Planétologie et Géosciences [UMR_C 6112] (LPG), Université d'Angers (UA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST), Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie, and Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)

Subjects
[SDU] Sciences of the Universe [physics], [SDU]Sciences of the Universe [physics]
Abstract

International audience

Published
2022

22. The Swarm Satellite Constellation Application and Research Facility (SCARF) and Swarm data products

Author

Olsen, Nils, Friis-Christensen, Eigil, Floberghagen, Rune, Alken, Patrick, Beggan, Ciaran D., Chulliat, Arnaud, Doornbos, Eelco, da Encarnação, João Teixeira, Hamilton, Brian, Hulot, Gauthier, van den IJssel, Jose, Kuvshinov, Alexey, Lesur, Vincent, Lühr, Hermann, Macmillan, Susan, Maus, Stefan, Noja, Max, Olsen, Poul Erik H., Park, Jaeheung, Plank, Gernot, Püthe, Christoph, Rauberg, Jan, Ritter, Patricia, Rother, Martin, Sabaka, Terence J., Schachtschneider, Reyko, Sirol, Olivier, Stolle, Claudia, Thébault, Erwan, Thomson, Alan W. P., Tøffner-Clausen, Lars, Velímský, Jakub, Vigneron, Pierre, and Visser, Pieter N.

Published
2013
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24. NanoMagSat, a 16U nanosatellite constellation high-precision magnetic project to initiate permanent low-cost monitoring of the Earth’s magnetic field and ionospheric environment

Author

HULOT, Gauthier, Leger, Jean-Michel, CLAUSEN, Lasse B. N., DECONINCK, Florian, Coïsson, Pierdavide, Vigneron, Pierre, Alken, Patrick, Chulliat, Arnaud, FINLAY, Christopher C., GRAYVER, Alexander, KUVSCHINOV, Alexey, Olsen, Nils, THÉBAULT, Erwan, Bertrand, Francois, Jager, Thomas, HÄFNER, Tobias, Institut de Physique du Globe de Paris (IPGP), Institut national des sciences de l'Univers (INSU - CNRS)-IPG PARIS-Université de La Réunion (UR)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Département Systèmes (DSYS), Commissariat à l'énergie atomique et aux énergies alternatives - Laboratoire d'Electronique et de Technologie de l'Information (CEA-LETI), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), University of Oslo (UiO), Solar Terrestrial Physics Division [Didcot], Space Science and Technology Department [Didcot] (RAL Space), STFC Rutherford Appleton Laboratory (RAL), Science and Technology Facilities Council (STFC)-Science and Technology Facilities Council (STFC)-STFC Rutherford Appleton Laboratory (RAL), Science and Technology Facilities Council (STFC)-Science and Technology Facilities Council (STFC), University of Colorado [Boulder], National Oceanic and Atmospheric Administration (NOAA), Technical University of Denmark [Lyngby] (DTU), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique du Globe de Paris (IPGP (UMR_7154)), Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Danmarks Tekniske Universitet = Technical University of Denmark (DTU)

Subjects
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph], [SDU.STU]Sciences of the Universe [physics]/Earth Sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
Abstract

International audience; The geomagnetic field has been continuously monitored from low-Earth orbit (LEO) since 1999, complementing ground-based observatory data by providing calibrated scalar and vector measurements with global coverage. The successful three-satellite ESA Swarm constellation is expected to remain in operation up to at least 2025. Further monitoring the field from space with high-precision absolute magnetometry beyond that date is of critical importance for improving our understanding of dynamics of the multiple components of this field, as well as that of the ionospheric environment. Here, we will report on the latest status of the NanoMagSat project, which aims to deploy and operate a new constellation concept of three identical 16U nanosatellites, using two inclined (approximately 60°) and one polar LEO, as well as an innovative payload including an advanced Miniaturized Absolute scalar and self-calibrated vector Magnetometer (MAM) combined with a set of precise star trackers (STR), a compact High-frequency Field Magnetometer (HFM, sharing subsystems with the MAM), a multi-needle Langmuir Probe (m-NLP) and dual frequency GNSS receivers. The data to be produced will at least include 1 Hz absolutely calibrated and oriented magnetic vector field (using the MAM and STR), 2 kHz very low noise magnetic scalar (using the MAM) and vector (using the HFM) field, 2 kHz local electron density (using the m-NLP) as well as precise timing, location and TEC products. In addition to briefly presenting the nanosatellite and constellation concepts, as well as the evolving programmatic status of the mission (which already underwent a consolidation study funded by the ESA Scout programme), this presentation will illustrate through a number of E2E simulations the ability of NanoMagSat to complement and improve on many of the science goals of the Swarm mission at a much lower cost, and to bring innovative science capabilities for ionospheric investigations. NanoMagSat could form the basis of a permanent collaborative constellation of nanosatellites for low-cost long-term monitoring of the geomagnetic field and ionospheric environment from space.

Published
2021

26. Archeointensity-based dating method: Examples from France and the Near-East

Author

Genevey, A., Gallet, Yves, Thébault, Erwan, Livermore, Philip, Fournier, Alexandre, and Genevey, Agnès

Subjects
[SDU] Sciences of the Universe [physics], [SHS] Humanities and Social Sciences
Abstract

While directional variations in the geomagnetic field are now widely used in archaeological practice in France to date fired structures found in situ after their abandonment, such as ceramic kilns or domestic ovens, the dating method based on geomagnetic field intensity variations is still under development. The reference intensity variation curve in France remained very fragmentary until very recently, thus limiting the possible applications towards dating. However, over the past decade, the acquisition of a large number of new archaeointensity data has considerably refine our knowledge of these fluctuations from the early Middle Ages to the present day (~1500 years). Large and rapid fluctuations have been revealed. In particular, the period of the early Middle Ages is framed by a rapid increase in intensity in the 6th century and a rapid decrease in the 10th century. These two time intervals therefore seem particularly favorable for the use of archaeointensity for dating purposes. To illustrate this potential, we present the archaeointensity study of two Medieval ceramic productions, from workshops located in Bourges (Cher) and in Chaudry (Oise). In our laboratory, other archeointensity studies have focused on the Near East with a large set of new data acquired in Syria for the Bronze period, between c. 3000 and c. 1000 BC, allowing the construction of a regional average intensity variation curve. This curve also offers new chronological constraints, which will be illustrated by several examples of archaeological contexts.

Published
2021

32. NanoMagSat, a 16U nanosatellite constellation high-precision magnetic project to initiate permanent low-cost monitoring of the Earth’s magnetic field and ionospheric environment

Author

Hulot, Gauthier, primary, Léger, Jean-Michel, additional, Clausen, Lasse B. N., additional, Deconinck, Florian, additional, Coïsson, Pierdavide, additional, Vigneron, Pierre, additional, Alken, Patrick, additional, Chulliat, Arnaud, additional, Finlay, Christopher C., additional, Grayver, Alexander, additional, Kuvschinov, Alexey, additional, Olsen, Nils, additional, Thébault, Erwan, additional, Jager, Thomas, additional, Bertrand, François, additional, and Häfner, Tobias, additional

Published
2021
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33. The Global Lithospheric Magnetic Field

Author

Lesur, Vincent, Thébault, Erwan, German Research Centre for Geosciences - Helmholtz-Centre Potsdam (GFZ), Institut de Physique du Globe de Paris (IPGP), and Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-IPG PARIS-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2019

37. In situ and remote characterization of the external field temporal variations at Mars

Author

Langlais, Benoit, Civet, François, Thébault, Erwan, Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology, [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph], [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2017

40. Electrical conductivity of the Earth's mantle from the first Swarm magnetic field measurements

Author

Civet, Francois, Thébault, Erwan, Verhoeven, Olivier, Langlais, Benoit, Saturnino, Diana, Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), and Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[SDU]Sciences of the Universe [physics], [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph], [SDU.STU]Sciences of the Universe [physics]/Earth Sciences, ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2015

42. Contribution à la modélisation et à l'interprétation du champ magnétique terrestre d'origine lithosphérique

Author

Thébault, Erwan, Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris Diderot (Paris 7) Sorbonne Paris Cité, and Vincent Courtillot

Subjects
geomagnetism, spherical harmonics, champ crustal, [SDU.STU]Sciences of the Universe [physics]/Earth Sciences, géomagnétisme, regional modelling, modélisation
Published
2014

44. Making a Better Magnetic Map

Author

Catalán, Manuel, primary, Dyment, Jérôme, additional, Choi, Yujin, additional, Hamoudi, Mohamed, additional, Lesur, Vincent, additional, Thébault, Erwan, additional, de Santis, Angelo, additional, Ishihara, Takemi, additional, Korhonen, Juha, additional, Litvinova, Tamara, additional, Luis, Joaquim, additional, Meyer, Brian, additional, Milligan, Peter, additional, Nakanishi, Masao, additional, Okuma, Shigeo, additional, Pilkington, Mark, additional, Purucker, Michael, additional, Ravat, Dhananjay, additional, Gaina, Carmen, additional, Maus, Stefan, additional, Quesnel, Yoann, additional, Saltus, Richard, additional, and Taylor, Patrick, additional

Published
2016
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45. Inference on core surface flow from observations and 3-D dynamo modelling

Author

Fournier, Alexandre, Aubert, Julien, Thébault, Erwan, Institut de Physique du Globe de Paris (IPGP), Centre National de la Recherche Scientifique (CNRS)-Université de La Réunion (UR)-Université Paris Diderot - Paris 7 (UPD7)-IPG PARIS-Institut national des sciences de l'Univers (INSU - CNRS), and Institut national des sciences de l'Univers (INSU - CNRS)-IPG PARIS-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[SDU]Sciences of the Universe [physics], Dynamo: theories and simulations, Rapid time variations, Core, Inverse theory, outer core and inner core
Abstract

International audience; We show how a 3-D, self-consistent numerical model of the geodynamo can be used as the subjective prior information for the determination of Earth's core surface flows from the geomagnetic field and its secular variation. This is achieved by estimating those parts of the numerical model state vector hidden from the observations, through a standard Kalman filtering (or stochastic inverse) procedure, where the Kalman gain matrix is based on the multivariate statistics of the geodynamo model. To allow for a direct comparison with observations, the field variables entering these statistics are scaled following two of the scaling laws that have recently come to the fore in numerical dynamo modelling, which express the dependency of the secular variation timescale and the magnetic energy density on their respective control parameters. We perform test experiments with noisy synthetic data, showing good to excellent recovery of the hidden parts of the state vector. A geomagnetic field model parent to a candidate model to the 2010 release of IGRF is then used for a core surface flow estimation. The estimated flow confirms the presence of convective columns underneath America, whereas exhibiting a high level of equatorial symmetry. We suggest that the discrete state estimation problem considered here (in connection with the classical core flow problem) could be used generically as a means to assess the degree of geophysical realism of a given geodynamo model. More generally, this study opens the way to using scaling laws and multivariate statistics from numerical models in the broader context of geomagnetic data assimilation. Assuming that we have knowledge of the radial component of the magnetic induction B r and of its rate-of-change ∂ t B r at the top of Earth's core, the so-called core flow problem consists of trying to estimate the flow u compatible with these observations, by using the radial component of the magnetic induction equation ∂ t B r = −∇ h · (u h B r) + λr −1 ∇ 2 (r B r), (1)

Published
2011

47. Core field acceleration pulse as a common cause of the 2003and 2007 geomagnetic jerks

Author

Chulliat, A., Thébault, Erwan, Hulot, Gauthier, Institut de Physique du Globe de Paris (IPGP), and Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-IPG PARIS-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[SDU]Sciences of the Universe [physics]
Abstract

International audience; Using observatory data, we report the detection of ageomagnetic jerk in 2007, which we relate to a jump inthe second derivative of the geomagnetic field previouslynoted in satellite data. Although not of worldwide extent,this jerk is very intense in the South Atlantic region.Using the CHAOS‐2 model, we show that both this jerkand the previous 2003 jerk are caused by a single corefield acceleration pulse reaching its maximum power near2006.0. This pulse seems to be simultaneously occurringin several regions of the core surface where it correspondsto dominant n = 5 and 6 spherical harmonic modes.Geometrical attenuation explains why the 2003 and 2007jerks are local and not fully synchronized at the Earth’ssurface. Our results suggest that this core field accelerationpulse is the relevant phenomenon to be investigated fromthe point of view of core dynamics, rather than the jerksthemselves. Citation: Chulliat, A., E. Thébault, and G. Hulot(2010), Core field acceleration pulse as a common cause of the2003 and 2007 geomagnetic jerks

Published
2010

49. Utique

Author

Monchambert, Jean-Yves, primary, Jerbania, Imed Ben, additional, Belarbi, Mehdi, additional, Bonadies, Luisa, additional, Bricchi-Duhem, Héloïse, additional, Jonghe, Marie De, additional, Gallet, Yves, additional, Nacef, Jihen, additional, Sghaïer, Yamen, additional, Tekki, Amel, additional, Thébault, Erwan, additional, and Vermeulen, Ségolène, additional

Published
2013
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