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2. Homogeneity assessment of the SuperCam calibration targets onboard rover perseverance

Author

Madariaga, J.M., Aramendia, J., Arana, G., Castro, K., Gómez-Nubla, L., Fdez-Ortiz de Vallejuelo, S., Garcia-Florentino, C., Maguregui, M., Manrique, J.A., Lopez-Reyes, G., Moros, J., Cousin, A., Maurice, S., Ollila, A.M., Wiens, R.C., Rull, F., Laserna, J., Garcia-Baonza, V., Madsen, M.B., Forni, O., Lasue, J., Clegg, S.M., Robinson, S., Bernardi, P., Brown, A.J., Caïs, P., Martinez-Frias, J., Beck, P., Bernard, S., Bernt, M.H., Beyssac, O., Cloutis, E., Drouet, C., Dromart, G., Dubois, B., Fabre, C., Gasnault, O., Gontijo, I., Johnson, J.R., Medina, J., Meslin, P.-Y., Montagnac, G., Sautter, V., Sharma, S.K., Veneranda, M., and Willis, P.A.

Published
2022
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7. SuperCam Calibration Targets: Design and Development

Author

Manrique, J. A., Lopez-Reyes, G., Cousin, A., Rull, F., Maurice, S., Wiens, R. C., Madsen, M. B., Madariaga, J. M., Gasnault, O., Aramendia, J., Arana, G., Beck, P., Bernard, S., Bernardi, P., Bernt, M. H., Berrocal, A., Beyssac, O., Caïs, P., Castro, C., Castro, K., Clegg, S. M., Cloutis, E., Dromart, G., Drouet, C., Dubois, B., Escribano, D., Fabre, C., Fernandez, A., Forni, O., Garcia-Baonza, V., Gontijo, I., Johnson, J., Laserna, J., Lasue, J., Madsen, S., Mateo-Marti, E., Medina, J., Meslin, P.-Y., Montagnac, G., Moral, A., Moros, J., Ollila, A. M., Ortega, C., Prieto-Ballesteros, O., Reess, J. M., Robinson, S., Rodriguez, J., Saiz, J., Sanz-Arranz, J. A., Sard, I., Sautter, V., Sobron, P., Toplis, M., and Veneranda, M.

Published
2020
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8. Apatites in Gale Crater

Author

Forni, O, Meslin, P.-Y, Drouet, C, Cousin, A, David, G, Mangold, N, Dehouck, E, Rampe, E. B, Gasnault, O, Nachon, M, Newsom, H, Blaney, D. L, Clegg, S. M, Ollila, A. M, Lasue, J, Maurice, S, and Wiens, R.C

Subjects
Space Sciences (General)
Abstract

ChemCam is an active remote sensing instrument suite that has operated successfully on MSL since landing Aug. 6th, 2012. It uses laser pulses to remove dust and to analyze rocks up to 7 m away. Laser-induced breakdown spectroscopy (LIBS) obtains emission spectra of materials ablated from the samples in electronically excited states. The intensities of the emission lines scale with the abundances of the related element. ChemCam is sensitive to most major rock-forming elements as well as to a set of minor and trace elements such as F, Cl, Li, P, Sr, Ba, and Rb. The measured chemical composition can then be used to infer the mineralogical composition of the ablated material. Here, we report a summary of inferred apatite detections along the MSL traverse at Gale Crater. We present the geologic settings of these findings and derive some interpretations about the formation conditions of apatite in time and space.

Published
2020

10. TRIDENT - Technology based impact assessment tool foR sustaInable, transparent Deep sEa miNing exploraTion and exploitation: A project overview

Author

Silva, E., Viegas, D., Martins, A., Almeida, J., Almeida, C., Neves, B., Madureira, Pedro, Wheeler, Andrew J., Salavasidis, G., Phillips, A., Schaap, A., Murton, Bramley, Berry, Alan, Weir, A., Dooly, G., Omerdic, E., Toal, D., Collins, P. C., Miranda, M., Petrioli, C., Barrera Rodríguez, C., Demoor, D., Drouet, C., Serafy, G.El, Jesus, S. M., Dañobeitia, Juan José, Tegas, Valentina, Cusí, Simó, Lopes, L., Bodo, B., Béguery, Laurent, Van Dam, S., Dumortier, J., Neves, L., Srivastava, V., Dahlgren, Thomas G., Hestetun, Jon Thomassen, Eiras, R., Caldeira, Rui, Rossi, Claudio, Spearman, Jeremy, Somoza, Luis, González Sanz, Francisco Javier, Bartolomé, Rafael, Bahurel, Pierre, Silva, E., Viegas, D., Martins, A., Almeida, J., Almeida, C., Neves, B., Madureira, Pedro, Wheeler, Andrew J., Salavasidis, G., Phillips, A., Schaap, A., Murton, Bramley, Berry, Alan, Weir, A., Dooly, G., Omerdic, E., Toal, D., Collins, P. C., Miranda, M., Petrioli, C., Barrera Rodríguez, C., Demoor, D., Drouet, C., Serafy, G.El, Jesus, S. M., Dañobeitia, Juan José, Tegas, Valentina, Cusí, Simó, Lopes, L., Bodo, B., Béguery, Laurent, Van Dam, S., Dumortier, J., Neves, L., Srivastava, V., Dahlgren, Thomas G., Hestetun, Jon Thomassen, Eiras, R., Caldeira, Rui, Rossi, Claudio, Spearman, Jeremy, Somoza, Luis, González Sanz, Francisco Javier, Bartolomé, Rafael, and Bahurel, Pierre

Abstract

By creating a dependable, transparent, and cost-effective system for forecasting and ongoing environmental impact monitoring of exploration and exploitation activities in the deep sea, TRIDENT seeks to contribute to the sustainable exploitation of seabed mineral resources. In order to operate autonomously in remote locations under harsh conditions and send real-time data to authorities in charge of granting licenses and providing oversight, this system will create and integrate new technology and innovative solutions. The efficient monitoring and inspection system that will be created will abide by national and international legal frameworks. At the sea surface, mid-water, and the bottom, TRIDENT will identify all pertinent physical, chemical, geological, and biological characteristics that must be monitored. It will also look for data gaps and suggest procedures for addressing them. These are crucial actions to take in order to produce accurate indicators of excellent environmental status, statistically robust environmental baselines, and thresholds for significant impact, allowing for the standardization of methods and tools. In order to monitor environmental parameters on mining and reference areas at representative spatial and temporal scales, the project consortium will thereafter develop and test an integrated system of stationary and mobile observatory platforms outfitted with the most recent automatic sensors and samplers. The system will incorporate high-capacity data processing pipelines able to gather, transmit, process, and display monitoring data in close to real-time to facilitate prompt actions for preventing major harm to the environment. Last but not least, it will offer systemic and technological solutions for predicting probable impacts of applying the developed monitoring and mitigation techniques

Published
2023

19. Homogeneity assessment of the SuperCam calibration targets onboard rover perseverance

Author

Química analítica, Kimika analitikoa, Madariaga Mota, Juan Manuel, Aramendia Gutiérrez, Julene, Arana Momoitio, Gorka, Gómez Nubla, Leticia, Fernández Ortiz de Vallejuelo, Silvia, García-Florentino, Cristina, Maguregui Hernando, Maite, Manrique, José Antonio, Lopez-Reyes, G., Moros, J., Cousin, A., Maurice, S., Ollila, A.M., Wiens, R.C, Rull, F., Laserna, J., Garcia-Baonza, V., Madsen, M.B., Forni, O., Lasue, J., Clegg, S.M., Robinson, S., Bernardi, P., Brown, A.J., Caïs, P., Martinez-Frias, J., Beck, P., Bernard, S., Bernt, M.H., Beyssac, O., Cloutis, E., Drouet, C., Dromart, G., Dubois, B., Fabre, C., Gasnault, O., Gontijo, I., Johnson, J.R., Medina, J., Meslin, P.-Y., Montagnac, G., Sautter, V., Sharma, S.K., Veneranda, Marco, Williss, P.A., Química analítica, Kimika analitikoa, Madariaga Mota, Juan Manuel, Aramendia Gutiérrez, Julene, Arana Momoitio, Gorka, Gómez Nubla, Leticia, Fernández Ortiz de Vallejuelo, Silvia, García-Florentino, Cristina, Maguregui Hernando, Maite, Manrique, José Antonio, Lopez-Reyes, G., Moros, J., Cousin, A., Maurice, S., Ollila, A.M., Wiens, R.C, Rull, F., Laserna, J., Garcia-Baonza, V., Madsen, M.B., Forni, O., Lasue, J., Clegg, S.M., Robinson, S., Bernardi, P., Brown, A.J., Caïs, P., Martinez-Frias, J., Beck, P., Bernard, S., Bernt, M.H., Beyssac, O., Cloutis, E., Drouet, C., Dromart, G., Dubois, B., Fabre, C., Gasnault, O., Gontijo, I., Johnson, J.R., Medina, J., Meslin, P.-Y., Montagnac, G., Sautter, V., Sharma, S.K., Veneranda, Marco, and Williss, P.A.

Abstract

The SuperCam instrument, onboard the Perseverance rover (Mars 2020 mission) is designed to perform remote analysis on the Martian surface employing several spectroscopic techniques such as Laser Induced Breakdown Spectroscopy (LIBS), Time-Resolved Raman (TRR), Time-Resolved Fluorescence (TRF) and Visible and Infrared (VISIR) reflectance. In addition, SuperCam also acquires high-resolution images using a color remote micro-imager (RMI) as well as sounds with its microphone. SuperCam has three main subsystems, the Mast Unit (MU) where the laser for chemical analysis and collection optics are housed, the Body Unit (BU) where the different spectrometers are located inside the rover, and the SuperCam Calibration Target (SCCT) located on the rover's deck to facilitate calibration tests at similar ambient conditions as the analyzed samples. To perform adequate calibrations on Mars, the 22 mineral samples included in the complex SCCT assembly must have a very homogeneous distribution of major and minor elements. The analysis and verification of such homogeneity for the 5-6 replicates of the samples included in the SCCT has been the aim of this work. To verify the physic-chemical homogeneity of the calibration targets, micro Energy Dispersive X-ray Fluorescence (EDXRF) imaging was first used on the whole surface of the targets, then the relative abundances of the detected elements were computed on 20 randomly distributed areas of 100*100 mum. For those targets showing a positive Raman response, micro-Raman spectroscopy imaging was performed on the whole surface of the targets at a resolution of 100*100 mum. The %RSD values (percent of relative standard deviation of mean values) for the major elements measured with EDXRF were compared with similar values obtained by two independent LIBS set-ups at spot sizes of 300 mum in diameter. The statistical analysis showed which elements were homogeneously distributed in the 22 mineral targets of the SCCT, providing their uncertainty v

Published
2022

20. Homogeneity assessment of the SuperCam calibration targets onboard rover perseverance

Author

Madariaga, J. M., Aramendia, J., Arana, G., Castro, K., Gomez-Nubla, L., de Vallejuelo, S. Fdez-Ortiz, Garcia-Florentino, C., Maguregui, M., Manrique, J. A., Lopez-Reyes, G., Moros, J., Cousin, A., Maurice, S., Ollila, A. M., Wiens, R. C., Rull, F., Laserna, J., Garcia-Baonza, V., Madsen, M. B., Forni, O., Lasue, J., Clegg, S. M., Robinson, S., Bernardi, P., Brown, A. J., Cais, P., Martinez-Frias, J., Beck, P., Bernard, S., Bernt, M. H., Beyssac, O., Cloutis, E., Drouet, C., Dromart, G., Dubois, B., Fabre, C., Gasnault, O., Gontijo, I., Johnson, J. R., Medina, J., Meslin, P. -Y., Montagnac, G., Sautter, V., Sharma, S. K., Veneranda, M., Willis, P. A., Madariaga, J. M., Aramendia, J., Arana, G., Castro, K., Gomez-Nubla, L., de Vallejuelo, S. Fdez-Ortiz, Garcia-Florentino, C., Maguregui, M., Manrique, J. A., Lopez-Reyes, G., Moros, J., Cousin, A., Maurice, S., Ollila, A. M., Wiens, R. C., Rull, F., Laserna, J., Garcia-Baonza, V., Madsen, M. B., Forni, O., Lasue, J., Clegg, S. M., Robinson, S., Bernardi, P., Brown, A. J., Cais, P., Martinez-Frias, J., Beck, P., Bernard, S., Bernt, M. H., Beyssac, O., Cloutis, E., Drouet, C., Dromart, G., Dubois, B., Fabre, C., Gasnault, O., Gontijo, I., Johnson, J. R., Medina, J., Meslin, P. -Y., Montagnac, G., Sautter, V., Sharma, S. K., Veneranda, M., and Willis, P. A.

Abstract

The SuperCam instrument, onboard the Perseverance rover (Mars 2020 mission) is designed to perform remote analysis on the Martian surface employing several spectroscopic techniques such as Laser Induced Breakdown Spectroscopy (LIBS), Time-Resolved Raman (TRR), Time-Resolved Fluorescence (TRF) and Visible and Infrared (VISIR) reflectance. In addition, SuperCam also acquires high-resolution images using a color remote micro imager (RMI) as well as sounds with its microphone. SuperCam has three main subsystems, the Mast Unit (MU) where the laser for chemical analysis and collection optics are housed, the Body Unit (BU) where the different spectrometers are located inside the rover, and the SuperCam Calibration Target (SCCT) located on the rover's deck to facilitate calibration tests at similar ambient conditions as the analyzed samples. To perform adequate calibrations on Mars, the 22 mineral samples included in the complex SCCT assembly must have a very homogeneous distribution of major and minor elements. The analysis and verification of such homogeneity for the 5-6 replicates of the samples included in the SCCT has been the aim of this work. To verify the physic chemical homogeneity of the calibration targets, micro Energy Dispersive X-ray Fluorescence (EDXRF) imaging was first used on the whole surface of the targets, then the relative abundances of the detected elements were computed on 20 randomly distributed areas of 100 x 100 mu m. For those targets showing a positive Raman response, micro-Raman spectroscopy imaging was performed on the whole surface of the targets at a resolution of 100 x 100 mu m. The %RSD values (percent of relative standard deviation of mean values) for the major elements measured with EDXRF were compared with similar values obtained by two independent LIBS set-ups at spot sizes of 300 mu m in diameter. The statistical analysis showed which elements were homogeneously distributed in the 22 mineral targets of the SCCT, providing their unc

Published
2022

21. SuperCam calibration targets on board the perseverance rover:Fabrication and quantitative characterization

Author

Cousin, Agnes, Sautter, Violaine, Fabre, Cécile, Dromart, Gilles, Montagnac, Gilles, Drouet, C., Meslin, Pierre-Yves, Gasnault, Olivier, Beyssac, Olivier, Bernard, S., Cloutis, Edward, Forni, O., Beck, P., Fouchet, T., Johnson, JR, Lasue, Jeremie, Ollila, A. M., De Parseval, P., Gouy, Sebastien, Caron, Brandiff R., Madariaga, J.M., Arana, G., Madsen, Morten Bo, Laserna, J., Moros, J., Manrique, J. A., Lopez-Reyes, Guillermo, Rull, F., Maurice, S., Wiens, R.C., Cousin, Agnes, Sautter, Violaine, Fabre, Cécile, Dromart, Gilles, Montagnac, Gilles, Drouet, C., Meslin, Pierre-Yves, Gasnault, Olivier, Beyssac, Olivier, Bernard, S., Cloutis, Edward, Forni, O., Beck, P., Fouchet, T., Johnson, JR, Lasue, Jeremie, Ollila, A. M., De Parseval, P., Gouy, Sebastien, Caron, Brandiff R., Madariaga, J.M., Arana, G., Madsen, Morten Bo, Laserna, J., Moros, J., Manrique, J. A., Lopez-Reyes, Guillermo, Rull, F., Maurice, S., and Wiens, R.C.

Published
2022

23. SuperCam calibration targets on board the perseverance rover: Fabrication and quantitative characterization

Author

Cousin, A., primary, Sautter, V., additional, Fabre, C., additional, Dromart, G., additional, Montagnac, G., additional, Drouet, C., additional, Meslin, P.Y., additional, Gasnault, O., additional, Beyssac, O., additional, Bernard, S., additional, Cloutis, E., additional, Forni, O., additional, Beck, P., additional, Fouchet, T., additional, Johnson, J.R., additional, Lasue, J., additional, Ollila, A.M., additional, De Parseval, P., additional, Gouy, S., additional, Caron, B., additional, Madariaga, J.M., additional, Arana, G., additional, Madsen, M. Bo, additional, Laserna, J., additional, Moros, J., additional, Manrique, J.A., additional, Lopez-Reyes, G., additional, Rull, F., additional, Maurice, S., additional, and Wiens, R.C., additional

Published
2022
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27. Calibration of the Fluorine, Chlorine and Hydrogen Content of Apatites With the ChemCam LIBS Instrument

Author

Meslin, P.-Y, Cicutto, L, Forni, O, Drouet, C, Rapin, W, Nachon, M, Cousin, A, Blank, J. G, McCubbin, F. M, Gasnault, O, Newsom, H, Mangold, N, Schroeder, S, Sautter, V, Maurice, S, and Wiens, R. C

Subjects
Lunar And Planetary Science And Exploration
Abstract

Determining the composition of apatites is important to understand the behavior of volatiles during planetary differentiation. Apatite is an ubiquitous magmatic mineral in the SNC meteorites. It is a significant reservoir of halogens in these meteorites and has been used to estimate the halogen budget of Mars. Apatites have been identified in sandstones and pebbles at Gale crater by ChemCam, a Laser-Induced Breakdown Spectroscometer (LIBS) instrument onboard the Curiosity rover. Their presence was inferred from correlations between calcium, fluorine (using the CaF molecular band centered near 603 nm, whose detection limit is much lower that atomic or ionic lines and, in some cases, phosphorus (whose detection limit is much larger). An initial quantification of fluorine, based on fluorite (CaF2)/basalt mixtures and obtained at the LANL laboratory, indicated that the excess of F/Ca (compared to the stoichiometry of pure fluorapatites) found on Mars in some cases could be explained by the presence of fluorite. Chlorine was not detected in these targets, at least above a detection limit of 0.6 wt% estimated from. Fluorapatite was later also detected by X-ray diffraction (with CheMin) at a level of approx.1wt% in the Windjana drill sample (Kimberley area), and several points analyzed by ChemCam in this area also revealed a correlation between Ca and F. The in situ detection of F-rich, Cl-poor apatites contrasts with the Cl-rich, F-poor compositions of apatites found in basaltic shergottites and in gabbroic clasts from the martian meteorite NWA 7034, which were also found to be more Cl-rich than apatites from basalts on Earth, the Moon, or Vesta. The in situ observations could call into question one of the few possible explanations brought forward to explain the SNC results, namely that Mars may be highly depleted in fluorine. The purpose of the present study is to refine the calibration of the F, Cl, OH and P signals measured by the ChemCam LIBS instrument, initiated for F, for Cl in soils, for P, and estimate their limit of detection. For this purpose, different types of apatites and mixtures of basalt powder and apatites were analyzed using ChemCam Engineering Qualification Model (EQM) at IRAP, Toulouse. The present abstract presents the initial results from the laboratory analyses. Differences between the response function of the EQM and the Flight Model of ChemCam are still to be refined to apply these new results to the Martian dataset.

Published
2016

34. Brushite (Ca,M)HPO4, 2H2O doping with bioactive ions (M = Mg2+, Sr2+, Zn2+, Cu2+, and Ag+): a new path to functional biomaterials?

Author

Sayahi M, Santos J, El-Feki H, Charvillat C, Bosc F, Karacan I, Milthorpe B, and Drouet C

Subjects
inorganic chemicals, 0303 Macromolecular and Materials Chemistry, 0912 Materials Engineering
Abstract

© 2019 Elsevier Ltd Dicalcium phosphate dihydrate, DCPD (CaHPO4·2H2O), brushite, is an important calcium phosphate compound encountered in mineralized tissues and used in medicine, especially in bone cement formulations. However, the use of DCPD as direct implantable biomaterial has not received dedicated attention. In addition, the possibility to dope DCPD with biologically active ions to modulate its performances was not systematically explored. We have investigated in depth the doping of DCPD with Mg2+, Sr2+, Zn2+, Cu2+, and Ag+ ions. Clear modifications in terms of chemical composition, particle size, pore distribution, crystal morphology, and affinity for water were pointed out. Then, the samples were cultured with human adipose-derived stem cells to explore cytotoxicity and proliferation. Various behaviors were noticed dependent on the incorporated metal ions. Such DCPD compounds associated with bioactive metal ions, and particularly Ag+ and Zn2+, appear promising as a new family of reactive materials for use, as such or in combination, in bone-related applications.

Published
2020

49. Quantification of water content by laser induced breakdown spectroscopy on Mars

Author

William Rapin, Y Meslin, P., Maurice, S., Wiens, R. C., Didier Laporte, Chauviré, B., Olivier Gasnault, Schröders, S., Beck, P., Bender, S., Beyssac, O., Cousin, A., Dehouck, E., Drouet, C., Forni, O., Nachon, M., Melikechi, N., Rondeau, B., Mangold, N., Thomas, N., Lasue, J., Fabre, C., Frydenvang, J., J-L, Lacour, Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Los Alamos National Laboratory (LANL), Laboratoire Magmas et Volcans (LMV), Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement et la société-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Physique du Globe de Clermont-Ferrand (OPGC), Institut national des sciences de l'Univers (INSU - CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Université Jean Monnet [Saint-Étienne] (UJM), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Optical Science Center for Applied Research (OSCAR), Delaware State University (DSU), University of Copenhagen = Københavns Universitet (KU), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Institut de Recherche pour le Développement et la société-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Physique du Globe de Clermont-Ferrand (OPGC), Institut national des sciences de l'Univers (INSU - CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), and University of Copenhagen = Københavns Universitet (UCPH)

Subjects
[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography, ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2019

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