SuperCam Calibration Targets: Design and Development
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SuperCam Calibration Targets: Design and Development J.A. Manrique1 · G. Lopez-Reyes1 · A. Cousin2 · F. Rull1 · S. Maurice2 · R.C. Wiens3 · M.B. Madsen4 · J.M. Madariaga5 · O. Gasnault2 · J. Aramendia5 · G. Arana5 · P. Beck6 · S. Bernard7 · P. Bernardi8 · M.H. Bernt4 · A. Berrocal9 · O. Beyssac7 · P. Caïs10 · C. Castro11 · K. Castro5 · S.M. Clegg3 · E. Cloutis12 · G. Dromart13 · C. Drouet14 · B. Dubois15 · D. Escribano16 · C. Fabre17 · A. Fernandez11 · O. Forni2 · V. Garcia-Baonza18 · I. Gontijo19 · J. Johnson20 · J. Laserna21 · J. Lasue2 · S. Madsen19 · E. Mateo-Marti22 · J. Medina1 · P.-Y. Meslin2 · G. Montagnac13 · A. Moral16 · J. Moros21 · A.M. Ollila3 · C. Ortega11 · O. Prieto-Ballesteros22 · J.M. Reess8 · S. Robinson3 · J. Rodriguez9 · J. Saiz1 · J.A. Sanz-Arranz1 · I. Sard11 · V. Sautter7 · P. Sobron23 · M. Toplis15 · M. Veneranda1 Received: 4 June 2020 / Accepted: 9 November 2020 © The Author(s) 2020
Abstract SuperCam is a highly integrated remote-sensing instrumental suite for NASA’s Mars 2020 mission. It consists of a co-aligned combination of Laser-Induced Breakdown The Mars 2020 Mission Edited by Kenneth A. Farley, Kenneth H. Williford and Kathryn M. Stack
B J.A. Manrique
[email protected]
1
Unidad Asocida UVA-CSIC-CAB, University of Valladolid (UVA), Valladolid, Spain
2
Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, CNES, Université de Toulouse, Toulouse, France
3
Los Alamos National Laboratory, Los Alamos, NM, USA
4
Niels Bohr Institute (NBI), University of Copenhagen, Copenhagen, Denmark
5
University of the Basque Country (UPV/EHU), Leioa, Spain
6
CNRS, Institut de Planetologie et d’Astrophysique de Grenoble (IPAG), Universite Grenoble Alpes, Saint-Martin d’Heres, France
7
Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC), CNRS, MNHN, Sorbonne Université, Paris, France
8
Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris-PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France
9
Ingeniería de Sistemas para la Defensa de España S.A. (ISDEFE), Madrid, Spain
10
Laboratoire d’astrophysique de Bordeaux, CNRS, Univ. Bordeaux, Bordeaux, France
11
Added Value Solutions (AVS), Elgóibar, Spain
12
U. Winnipeg, Winnipeg, Canada
13
Univ Lyon, ENSL, CNRS, LGL-TPE, Univ Lyon 1, 69007 Lyon, France
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Spectroscopy (LIBS), Time-Resolved Raman and Luminescence (TRR/L), Visible and Infrared Spectroscopy (VISIR), together with sound recording (MIC) and high-magnification imaging techniques (RMI). They provide information on the mineralogy, geochemistry and mineral context around the Perseverance Rover. The calibration of this complex suite is a major challenge. Not only does each technique require its own standards or references, their combination also introduces new requirements to obtain optimal scientific output. Elemental composition, molecular vibrational features, fluorescence, morphology and texture provide a full picture of the sample w
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