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1. Moons and Jupiter Imaging Spectrometer (MAJIS) on Jupiter Icy Moons Explorer (JUICE)

Author

Poulet, F., Piccioni, G., Langevin, Y., Dumesnil, C., Tommasi, L., Carlier, V., Filacchione, G., Amoroso, M., Arondel, A., D’Aversa, E., Barbis, A., Bini, A., Bolsée, D., Bousquet, P., Caprini, C., Carter, J., Dubois, J.-P., Condamin, M., Couturier, S., Dassas, K., Dexet, M., Fletcher, L., Grassi, D., Guerri, I., Haffoud, P., Larigauderie, C., Le Du, M., Mugnuolo, R., Pilato, G., Rossi, M., Stefani, S., Tosi, F., Vincendon, M., Zambelli, M., Arnold, G., Bibring, J.-P., Biondi, D., Boccaccini, A., Brunetto, R., Carapelle, A., Cisneros González, M., Hannou, C., Karatekin, O., Le Cle’ch, J.-C., Leyrat, C., Migliorini, A., Nathues, A., Rodriguez, S., Saggin, B., Sanchez-Lavega, A., Schmitt, B., Seignovert, B., Sordini, R., Stephan, K., Tobie, G., Zambon, F., Adriani, A., Altieri, F., Bockelée, D., Capaccioni, F., De Angelis, S., De Sanctis, M.-C., Drossart, P., Fouchet, T., Gérard, J.-C., Grodent, D., Ignatiev, N., Irwin, P., Ligier, N., Manaud, N., Mangold, N., Mura, A., Pilorget, C., Quirico, E., Renotte, E., Strazzulla, G., Turrini, D., Vandaele, A.-C., Carli, C., Ciarniello, M., Guerlet, S., Lellouch, E., Mancarella, F., Morbidelli, A., Le Mouélic, S., Raponi, A., Sindoni, G., and Snels, M.

Published
2024
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2. NOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected Performance

Author

Vandaele, Ann Carine, López-Moreno, José Juan, Patel, Manish R., Bellucci, Giancarlo, Daerden, Frank, Ristic, Bojan, Robert, S., Thomas, Ian R., Wilquet, V., Allen, M., Alonso-Rodrigo, G., Altieri, F., Aoki, Shohei, Bolsée, D., Clancy, T., Cloutis, E., Depiesse, C., Drummond, R., Fedorova, A., Formisano, V., Funke, Bernd, González-Galindo, F., Geminale, A., Gérard, Jean-Claude, Giuranna, M., Hetey, L., Ignatiev, N., Kaminski, J., Karatekin, O., Kasaba, Y., Leese, M., Lefèvre, F., Lewis, S. R., López-Puertas, Manuel, López-Valverde, M. A., Mahieux, A., Mason, J., McConnell, J., Mumma, M., Neary, L., Neefs, E., Renotte, E., Rodriguez-Gomez, J., Sindoni, G., Smith, M., Stiepen, A., Trokhimovsky, A., Vander Auwera, J., Villanueva, Geronimo L., Viscardy, S., Whiteway, J., Willame, Y., Wolff, Michael T., Patel, M., D’aversa, E., Fussen, D., García Comas, Maia, Hewson, W., McConnel, J., Novak, R., Oliva, F., Piccialli, A., Aparicio del Moral, Beatriz, Barzin, P., BenMoussa, A., Berkenbosch, S., Biondi, D., Bonnewijn, S., Candini, G. P., Clairquin, R., Cubas, J., De-Lanoye, S., Giordanengo, B., Gissot, S., Gomez, A., Maes, J., Mazy, E., Mazzoli, A., Meseguer, J., Morales, Rafael, Orban, A., Pastor, Carmen, Perez-Grande, I., Queirolo, C., Saggin, B., Samain, V., Sanz Andres, A., Sanz Mesa, Rosario, Simar, J.-F., Thibert, T., Jerónimo, José María, The NOMAD Team, Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB), Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), School of Physical Sciences [Milton Keynes], Faculty of Science, Technology, Engineering and Mathematics [Milton Keynes], The Open University [Milton Keynes] (OU)-The Open University [Milton Keynes] (OU), 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), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Jet Propulsion Laboratory (JPL), California Institute of Technology (CALTECH)-NASA, Instituto Universitario de Microgravedad 'Ignacio Da Riva' (IDR), Universidad Politécnica de Madrid (UPM), Space Science Institute [Boulder] (SSI), Department of Geography [Winnipeg], University of Winnipeg, Space Research Institute of the Russian Academy of Sciences (IKI), Russian Academy of Sciences [Moscow] (RAS), Laboratoire de Physique Atmosphérique et Planétaire (LPAP), Université de Liège, Institute of Geophysics [Warsaw], Polska Akademia Nauk = Polish Academy of Sciences (PAN), Royal Observatory of Belgium [Brussels] (ROB), Tohoku University [Sendai], PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Fonds National de la Recherche Scientifique [Bruxelles] (FNRS), York University [Toronto], NASA Goddard Space Flight Center (GSFC), Centre Spatial de Liège (CSL), Laboratory for Atmospheric and Space Physics [Boulder] (LASP), University of Colorado [Boulder], Service de Chimie Quantique et Photophysique, Université libre de Bruxelles (ULB), Catholic University of America, Belgian Science Policy Office, European Space Agency, Ministerio de Ciencia e Innovación (España), European Commission, UK Space Agency, Agenzia Spaziale Italiana, and Fonds de la Recherche Scientifique (Fédération Wallonie-Bruxelles)

Subjects
010504 meteorology & atmospheric sciences, Solar occultation, education, Physique atomique et moléculaire, Exploration of Mars, 01 natural sciences, Occultation, law.invention, Orbiter, Mars atmosphere, law, 0103 physical sciences, Nadir, Chimie, natural sciences, 010303 astronomy & astrophysics, Spectroscopy, 0105 earth and related environmental sciences, Remote sensing, Ultraviolet, Martian, Astronomy and Astrophysics, Dust, Atmosphere of Mars, Mars Exploration Program, Nadir observations, ExoMars, Trace gas, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Spectroscopie [électromagnétisme, optique, acoustique], 13. Climate action, Space and Planetary Science, Visible, Environmental science, Infrared, Methane, Composition
Abstract

Open Access This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), The NOMAD (“Nadir and Occultation for MArs Discovery”) spectrometer suite on board the ExoMars Trace Gas Orbiter (TGO) has been designed to investigate the composition of Mars’ atmosphere, with a particular focus on trace gases, clouds and dust. The detection sensitivity for trace gases is considerably improved compared to previous Mars missions, compliant with the science objectives of the TGO mission. This will allow for a major leap in our knowledge and understanding of the Martian atmospheric composition and the related physical and chemical processes. The instrument is a combination of three spectrometers, covering a spectral range from the UV to the mid-IR, and can perform solar occultation, nadir and limb observations. In this paper, we present the science objectives of the instrument and explain the technical principles of the three spectrometers. We also discuss the expected performance of the instrument in terms of spatial and temporal coverage and detection sensitivity.© 2018, The Author(s)., The NOMAD experiment is led by the Royal Belgian Institute for Space Aeronomy (IASB-BIRA), assisted by Co-PI teams from Spain (IAA-CSIC), Italy (INAF-IAPS), and the United Kingdom (Open University). This project acknowledges funding by the Belgian Science Policy Office (BELSPO), with the financial and contractual coordination by the ESA Prodex Office (PEA 4000103401, 4000121493), by Spanish MICINN through its Plan Nacional and by European funds under grant ESP2015-65064-C2-1-P (MINECO/FEDER), as well as by UK Space Agency through grants ST/R005761/1, ST/P001262/1, ST/R001405/1 and ST/R001405/1 and Italian Space Agency through grant 2018-2-HH.0. The research was performed as part of the >Excellence of Science> project >Evolution and Tracers of Habitability on Mars and the Earth> (30442502). SA acknowledge support from the FNRS, Be.

Published
2018
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3. NOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected Performance

Author

Vandaele, A. C., López-Moreno, José Juan, Patel, M. R., Bellucci, G., Daerden, F., Ristic, B., Robert, S., Thomas, I. R., Wilquet, V., Allen, M., Alonso-Rodrigo, G., Altieri, F., Aoki, S., Bolsée, D., Clancy, T., Cloutis, E., Depiesse, C., Drummond, R., Fedorova, A., Formisano, V., Funke, Bernd, González-Galindo, F., Geminale, A., Gérard, Jean-Claude, Giuranna, M., Hetey, L., Ignatiev, N., Kaminski, J., Karatekin, O., Kasaba, Y., Leese, M., Lefèvre, F., Lewis, S. R., López-Puertas, Manuel, López-Valverde, M. A., Mahieux, A., Mason, J., McConnell, J., Mumma, M., Neary, L., Neefs, E., Renotte, E., Rodriguez-Gomez, J., Sindoni, G., Smith, M., Stiepen, A., Trokhimovsky, A., Vander Auwera, J., Villanueva, G., Viscardy, S., Whiteway, J., Willame, Y., Wolff, Michael T., Patel, M., D’aversa, E., Fussen, D., García Comas, Maia, Hewson, W., McConnel, J., Novak, R., Oliva, F., Piccialli, A., Aparicio del Moral, Beatriz, Barzin, P., BenMoussa, A., Berkenbosch, S., Biondi, D., Bonnewijn, S., Candini, G. P., Clairquin, R., Cubas, J., De-Lanoye, S., Giordanengo, B., Gissot, S., Gomez, A., Maes, J., Mazy, E., Mazzoli, A., Meseguer, J., Morales, Rafael, Orban, A., Pastor, Carmen, Perez-Grande, I., Queirolo, C., Saggin, B., Samain, V., Sanz Andres, A., Sanz Mesa, Rosario, Simar, J.-F., Thibert, T., Jerónimo, José María, The NOMAD Team, Belgian Science Policy Office, European Space Agency, Ministerio de Ciencia e Innovación (España), European Commission, UK Space Agency, Agenzia Spaziale Italiana, and Fonds de la Recherche Scientifique (Fédération Wallonie-Bruxelles)

Subjects
Mars atmosphere, Solar occultation, Visible, Dust, Infrared, Methane, ExoMars, Nadir observations, Spectroscopy, Composition, Ultraviolet
Abstract

Open Access This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/) The NOMAD (“Nadir and Occultation for MArs Discovery”) spectrometer suite on board the ExoMars Trace Gas Orbiter (TGO) has been designed to investigate the composition of Mars’ atmosphere, with a particular focus on trace gases, clouds and dust. The detection sensitivity for trace gases is considerably improved compared to previous Mars missions, compliant with the science objectives of the TGO mission. This will allow for a major leap in our knowledge and understanding of the Martian atmospheric composition and the related physical and chemical processes. The instrument is a combination of three spectrometers, covering a spectral range from the UV to the mid-IR, and can perform solar occultation, nadir and limb observations. In this paper, we present the science objectives of the instrument and explain the technical principles of the three spectrometers. We also discuss the expected performance of the instrument in terms of spatial and temporal coverage and detection sensitivity.© 2018, The Author(s). The NOMAD experiment is led by the Royal Belgian Institute for Space Aeronomy (IASB-BIRA), assisted by Co-PI teams from Spain (IAA-CSIC), Italy (INAF-IAPS), and the United Kingdom (Open University). This project acknowledges funding by the Belgian Science Policy Office (BELSPO), with the financial and contractual coordination by the ESA Prodex Office (PEA 4000103401, 4000121493), by Spanish MICINN through its Plan Nacional and by European funds under grant ESP2015-65064-C2-1-P (MINECO/FEDER), as well as by UK Space Agency through grants ST/R005761/1, ST/P001262/1, ST/R001405/1 and ST/R001405/1 and Italian Space Agency through grant 2018-2-HH.0. The research was performed as part of the >Excellence of Science> project >Evolution and Tracers of Habitability on Mars and the Earth> (30442502). SA acknowledge support from the FNRS, Be.

Published
2018

4. A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express

Author

Drossart, P, Piccioni, G, Gérard, JC, Lopez-Valverde, MA, Sanchez-Lavega, A, Zasova, L, Hueso, R, Taylor, FW, Bézard, B, Adriani, A, Angrilli, F, Arnold, G, Baines, KH, Bellucci, G, Benkhoff, J, Bibring, JP, Blanco, A, Blecka, MI, Carlson, RW, Coradini, A, Di Lellis, A, Encrenaz, T, Erard, S, Fonti, S, Formisano, V, Fouchet, T, Garcia, R, Haus, R, Helbert, J, Ignatiev, NI, Irwin, P, Langevin, Y, Lebonnois, S, Luz, D, Marinangeli, L, Orofino, V, Rodin, AV, Roos-Serote, MC, Saggin, B, Stam, DM, Titov, D, Visconti, G, Zambelli, M, Tsang, C, Ammannito, E, Barbis, A, Berlin, R, Bettanini, C, Boccaccini, A, Bonnello, G, Bouyé, M, Capaccioni, F, Cardesin, A, Carraro, F, Cherubini, G, Cosi, M, Dami, M, De Nino, M, Del Vento, D, Di Giampietro, M, Donati, A, Dupuis, O, Espinasse, S, Fabbri, A, Fave, A, Veltroni, IF, Filacchione, G, Garceran, K, Ghomchi, Y, Giustizi, M, Gondet, B, Hello, Y, Henry, F, Hofer, S, Huntzinger, G, Kachlicki, J, Knoll, R, Kouach, D, Mazzoni, A, Melchiorri, R, Mondello, G, Monti, F, Neumann, C, Nuccilli, F, Parisot, J, Pasqui, C, Perferi, S, Peter, G, Piacentino, A, Pompei, C, Réess, JM, Rivet, JP, Romano, A, Russ, N, Santoni, M, Scarpelli, A, Sémery, A, Soufflot, A, Stefanovitch, D, Suetta, E, Tarchi, F, Tonetti, N, Tosi, F, Ulmer, B, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Istituto de Astrofisica Spaziale et Fisica cosmica (IASF), Istituto Nazionale di Astrofisica (INAF), Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École des Ponts ParisTech (ENPC)-École polytechnique (X)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)

Subjects
010504 meteorology & atmospheric sciences, Infrared, Solar zenith angle, Venus, Atmospheric sciences, 01 natural sciences, Astrobiology, Atmosphere of Venus, Atmosphere, Altitude, [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology, Planet, 0103 physical sciences, 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS, Physics::Atmospheric and Oceanic Physics, 0105 earth and related environmental sciences, Venus Express, Multidisciplinary, biology, Airglow, VIRTIS, biology.organism_classification, 13. Climate action, Physics::Space Physics, Astrophysics::Earth and Planetary Astrophysics, Geology
Abstract

The upper atmosphere of a planet is a transition region in which energy is transferred between the deeper atmosphere and outer space. Molecular emissions from the upper atmosphere (90-120 km altitude) of Venus can be used to investigate the energetics and to trace the circulation of this hitherto little-studied region. Previous spacecraft and ground-based observations of infrared emission from CO2, O2 and NO have established that photochemical and dynamic activity controls the structure of the upper atmosphere of Venus. These data, however, have left unresolved the precise altitude of the emission owing to a lack of data and of an adequate observing geometry. Here we report measurements of day-side CO2 non-local thermodynamic equilibrium emission at 4.3 microm, extending from 90 to 120 km altitude, and of night-side O2 emission extending from 95 to 100 km. The CO2 emission peak occurs at approximately 115 km and varies with solar zenith angle over a range of approximately 10 km. This confirms previous modelling, and permits the beginning of a systematic study of the variability of the emission. The O2 peak emission happens at 96 km +/- 1 km, which is consistent with three-body recombination of oxygen atoms transported from the day side by a global thermospheric sub-solar to anti-solar circulation, as previously predicted.

Published
2007
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5. First observations of the planetary Fourier spectrometer at Mars

Author

Formisano, V., Cottini, V., Giuranna, M., Grassi, D., Khatuntsev, I., Ignatiev, N., Maturilli, A., Piccioni, G., Saggin, B., and Zasova, L.

Subjects
*MARS (Planet), *INNER planets, *ATMOSPHERE, *SPECTROMETERS, *TEMPERATURE
Abstract

Abstract: The first results of the Planetary Fourier Spectrometer (PFS) orbiting the planet Mars are reviewed and discussed here, with reference to a set of studies being published elsewhere. An average global spectrum ranging from 200 to 8200cm−1 is discussed by comparing it to the ISO SWS Martian spectrum and to the global synthetic spectrum computed using only CO2, CO, H2O gases. PFS is able to measure the vertical temperature–pressure profile in the Martian atmosphere and the temperature of the soil. The SW channel shows the major CO2 bands at 4.3 and 2.7μm. The bottom of the first band shows very clearly the non LTE emission of the high atmospheric CO2 gas, and the dust content in the atmosphere. In one of the first orbit passing over the Olympus Mons, the temperature field retrieved shows abnormal adiabatic cooling in the atmosphere above the mountain, while the soil temperature of the volcano is higher than the latitudinal profile expectation because of a better illumination from the sun. Many solar lines are observed, a few of them are studied and compared to ISO observations. [Copyright &y& Elsevier]

Published
2005
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