Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Mathieu Hirtzig"'
Autor:
Clément Narteau, Roger N. Clark, Benjamin Charnay, T. Appéré, S. Courrech du Pont, Jason M. Soderblom, Thomas Cornet, B. J. Buratti, J. Bow, G. Vixie, Jasper F. Kok, Jason W. Barnes, Ralf Jaumann, Philip D. Nicholson, Mathieu Hirtzig, Pascal Rannou, S. Le Mouélic, Olivier Bourgeois, Jani Radebaugh, L. Maltagliati, Ralph D. Lorenz, Kevin H. Baines, Sebastien Rodriguez, Robert H. Brown, Christophe Sotin, Antoine Lucas, S. Rafkin, Caitlin A. Griffith, Katrin Stephan, Athena Coustenis
Publikováno v:
Nature Geoscience
Nature Geoscience, Nature Publishing Group, 2018, 11 (10), pp.727-732. ⟨10.1038/s41561-018-0233-2⟩
Nature Geoscience, vol 11, iss 10
NATURE GEOSCIENCE, vol 11, iss 10
Nature Geoscience, 2018, 11 (10), pp.727-732. ⟨10.1038/s41561-018-0233-2⟩
Nature Geoscience, Nature Publishing Group, 2018, 11 (10), pp.727-732. ⟨10.1038/s41561-018-0233-2⟩
Nature Geoscience, vol 11, iss 10
NATURE GEOSCIENCE, vol 11, iss 10
Nature Geoscience, 2018, 11 (10), pp.727-732. ⟨10.1038/s41561-018-0233-2⟩
Saturn’s moon Titan has a dense nitrogen-rich atmosphere, with methane as its primary volatile. Titan’s atmosphere experiences an active chemistry that produces a haze of organic aerosols that settle to the surface and a dynamic climate in which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d5b72f695b90f16c88f37e6a5cc5473
https://hal.archives-ouvertes.fr/hal-02331823
https://hal.archives-ouvertes.fr/hal-02331823
Autor:
Rosaly M. C. Lopes, S. Le Mouélic, Robert H. Brown, Katrin Stephan, Mathieu Hirtzig, Athena Coustenis, Pierre Drossart, Kenneth J. Lawrence, Sebastien Rodriguez, A. Solomonidou, Ralf Jaumann, Emmanuel Bratsolis, Christophe Sotin
Publikováno v:
Icarus
Icarus, Elsevier, 2016, 270, pp.85-99. ⟨10.1016/j.icarus.2015.05.003⟩
Icarus, 2016, 270, pp.85-99. ⟨10.1016/j.icarus.2015.05.003⟩
Icarus, Elsevier, 2016, 270, pp.85-99. ⟨10.1016/j.icarus.2015.05.003⟩
Icarus, 2016, 270, pp.85-99. ⟨10.1016/j.icarus.2015.05.003⟩
International audience; We analyze Cassini VIMS data of several areas on Titan's surface looking for variations with time. Three of these locations are near the equator (10-30°S), namely Hotei Regio, Tui Regio and Sotra Patera; in some cases changes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a905a977a1b12ff72d82c45a7d2aef6c
https://hal.archives-ouvertes.fr/hal-02373377
https://hal.archives-ouvertes.fr/hal-02373377
Autor:
Athena Coustenis, Alberto Negrão, Michel Loete, Jean-Paul Champion, Catherine de Bergh, Caitlin A. Griffith, Mathieu Hirtzig, Pierre Drossart, Tony Gabard, Bruno Bézard, Emmanuel Lellouch, Vincent Boudon
Publikováno v:
Reflets de la physique. :13-16
Le methane (CH4) joue sur Tian, le plus gros satellite de Saturne, un role similaire a celui de l'eau sur Terre. Il y est de plus a l'origine d'une chimie organique complexe. La spectroscopie etant la technique privilegiee pour mesurer le CH4 dans le
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::73fd51a5c915b4f46791a978156c17bc
https://doi.org/10.1051/refdp/2008023
https://doi.org/10.1051/refdp/2008023
Autor:
Stephen W. Bougher, Mathieu Hirtzig, Peter Gao, Yuk L. Yung, Larry W. Esposito, Christopher D. Parkinson
Publikováno v:
Planetary and Space Science
Planetary and Space Science, 2015, 113-114, pp.226-236. ⟨10.1016/j.pss.2015.02.015⟩
Planetary and Space Science, Elsevier, 2015, 113-114, pp.226-236. ⟨10.1016/j.pss.2015.02.015⟩
Planetary and Space Science, 2015, 113-114, pp.226-236. ⟨10.1016/j.pss.2015.02.015⟩
Planetary and Space Science, Elsevier, 2015, 113-114, pp.226-236. ⟨10.1016/j.pss.2015.02.015⟩
We use the JPL/Caltech 1-D photochemical model to solve continuity diffusion equation for atmospheric constituent abundances and total number density as a function of radial distance from the planet Venus. Photochemistry of the Venus atmosphere from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c8cbcd7480276cda5e4952f3fcb2512
https://hal.science/hal-02509301
https://hal.science/hal-02509301
Autor:
Emmanuel Lellouch, Samir Kassi, Bruno Bézard, C. de Bergh, Pascal Rannou, Sebastien Rodriguez, Vincent Boudon, Vl.G. Tyuterev, Didier Mondelain, Thibaud Cours, S. Le Mouélic, Mathieu Hirtzig, Athena Coustenis, Andrei Nikitin, Alain Campargue, Pierre Drossart
Publikováno v:
Icarus
Icarus, Elsevier, 2013, 226, pp.470-486. ⟨10.1016/J.ICARUS.2013.05.033⟩
Icarus, 2013, 226, pp.470-486. ⟨10.1016/J.ICARUS.2013.05.033⟩
Icarus, Elsevier, 2013, 226, pp.470-486. ⟨10.1016/J.ICARUS.2013.05.033⟩
Icarus, 2013, 226, pp.470-486. ⟨10.1016/J.ICARUS.2013.05.033⟩
International audience; We present an analysis of Titan data acquired by the Cassini Visual and Infrared Mapping Spectrometer (VIMS), making use of recent improvements in methane spectroscopic parameters in the region 1.3-5.2 μm. We first analyzed V
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7dc453af982e9e5c1af1c278c223beb
https://hal.archives-ouvertes.fr/hal-00997595
https://hal.archives-ouvertes.fr/hal-00997595
Autor:
Alain Campargue, C. de Bergh, Pascal Rannou, Sebastien Rodriguez, Pierre Drossart, Bruno Bézard, Vincent Boudon, S. Le Mouélic, Thibaud Cours, Mathieu Hirtzig, Emmanuel Lellouch, Vl.G. Tyuterev, Didier Mondelain, Andrei Nikitin, Samir Kassi, Athena Coustenis
Publikováno v:
Icarus
Icarus, Elsevier, 2013, 226, pp.1182-1182. ⟨10.1016/J.ICARUS.2013.07.015⟩
Icarus, 2013, 226, pp.1182-1182. ⟨10.1016/J.ICARUS.2013.07.015⟩
Icarus, Elsevier, 2013, 226, pp.1182-1182. ⟨10.1016/J.ICARUS.2013.07.015⟩
Icarus, 2013, 226, pp.1182-1182. ⟨10.1016/J.ICARUS.2013.07.015⟩
0019-1035/$ see front matter 2013 Elsevier Inc. All rights reserved. http://dx.doi.org/10.1016/j.icarus.2013.07.015 DOI of original article: http://dx.doi.org/10.1016/j.icarus.2013.05.033 ⇑ Corresponding author. Address: LESIA, Observatoire de Pari
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e77a629f297d3e3f22630a81b43ff06
https://hal.archives-ouvertes.fr/hal-00997633
https://hal.archives-ouvertes.fr/hal-00997633
Autor:
Konstantinos Kyriakopoulos, Xenophon Moussas, Emmanuel Bratsolis, Athena Coustenis, G. Bampasidis, Karen St. Seymour, Anezina Solomonidou, Mathieu Hirtzig
Publikováno v:
Planetary and Space Science
Planetary and Space Science, Elsevier, 2013, 77, pp.104-117. ⟨10.1016/j.pss.2012.05.003⟩
Planetary and Space Science, 2013, 77, pp.104-117. ⟨10.1016/j.pss.2012.05.003⟩
Planetary and Space Science, Elsevier, 2013, 77, pp.104-117. ⟨10.1016/j.pss.2012.05.003⟩
Planetary and Space Science, 2013, 77, pp.104-117. ⟨10.1016/j.pss.2012.05.003⟩
Spectro-imaging and radar measurements by the Cassini–Huygens mission suggest that some of the Saturnian satellites may be geologically active and could support tectonic processes. In particular Titan, Saturn's largest moon, possesses a complex and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::773e39fe378923c64cf744dec9515011
https://hal.archives-ouvertes.fr/hal-02518650
https://hal.archives-ouvertes.fr/hal-02518650
Autor:
Emmanuel Bratsolis, Anezina Solomonidou, Xenophon Moussas, Georgios Bampasidis, Panagiota Preka-Papadema, Konstantinos Kyriakopoulos, Mathieu Hirtzig, Athena Coustenis
Publikováno v:
2011 2nd International Conference on Space Technology.
The Synthetic Aperture Radar (SAR) instrumentation on board the Cassini orbiter has identified large hydrocarbon liquid deposits on the surface of Titan [e.g. 1], distributed mainly around its northern polar regions. Recent studies [2] suggest that t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::afab908c8a0c2cbf46563acd5c3c2f2c
https://doi.org/10.1109/icspt.2011.6064648
https://doi.org/10.1109/icspt.2011.6064648
Autor:
Emmanuel Bratsolis, Panagiota Preka-Papadema, Xenophon Moussas, Athena Coustenis, Georgios Bampasidis, Mathieu Hirtzig, Anezina Solomonidou, Konstantinos Kyriakopoulos
Publikováno v:
2011 2nd International Conference on Space Technology.
The exploration of the systems of the outer planets of the Solar System, in particular Jupiter and Saturn, is in the forefront of contemporary space exploration. Indeed, these two planetary systems host extreme environments which can provide us with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e4e4b0b96d7832051e3fc583c3835e19
https://doi.org/10.1109/icspt.2011.6064652
https://doi.org/10.1109/icspt.2011.6064652
Autor:
Emmanuel Bratsolis, Anezina Solomonidou, Georgios Bampasidis, Panagiota Preka-Papadema, Konstantinos Kyriakopoulos, Xenophon Moussas, Athena Coustenis, Mathieu Hirtzig
Publikováno v:
2011 2nd International Conference on Space Technology.
The icy moons of the Outer Solar System are extremely interesting planetary bodies since they possess evidence about the origin and evolution of their systems and the Solar System in general. In terms of surface morphology, internal structure as well
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e5074d699325121bf249960ebbd01e7f
https://doi.org/10.1109/icspt.2011.6064647
https://doi.org/10.1109/icspt.2011.6064647