Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Emmanuel Lellouch"'
Autor:
Emmanuel Lellouch, F. M. Flasar, Pgj Irwin, R. Moreno, Todd M. Ansty, Sophie Bauduin, V. Cottini, Conor A. Nixon, Nicholas A Teanby
Publikováno v:
Icarus
Icarus, Elsevier, 2018, 311, pp.288-305. ⟨10.1016/j.icarus.2018.04.003⟩
Bauduin, S, Irwin, P G J, Lellouch, E, Cottini, V, Moreno, R, Nixon, C A, Teanby, N A, Ansty, T & Flasar, F M 2018, ' Retrieval of H 2 O abundance in Titan's stratosphere : A (re)analysis of CIRS/Cassini and PACS/Herschel observations ', Icarus, vol. 311, pp. 288-305 . https://doi.org/10.1016/j.icarus.2018.04.003
Icarus, 311
Icarus, Elsevier, 2018, 311, pp.288-305. ⟨10.1016/j.icarus.2018.04.003⟩
Bauduin, S, Irwin, P G J, Lellouch, E, Cottini, V, Moreno, R, Nixon, C A, Teanby, N A, Ansty, T & Flasar, F M 2018, ' Retrieval of H 2 O abundance in Titan's stratosphere : A (re)analysis of CIRS/Cassini and PACS/Herschel observations ', Icarus, vol. 311, pp. 288-305 . https://doi.org/10.1016/j.icarus.2018.04.003
Icarus, 311
Since its first measurement 20 years ago by the Infrared Space Observatory (ISO), the water (H2O) mole fraction in Titan's stratosphere remains uncertain due to large differences between the determinations from available measurements. More particular
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8867de10555e26cf1142aa0c03f1ac29
https://hal.archives-ouvertes.fr/hal-02291429
https://hal.archives-ouvertes.fr/hal-02291429
Autor:
Ekkehard Kührt, Olivier Groussin, Stefano Mottola, Gianrico Filacchione, W.-H. Ip, Emmanuel Lellouch, M. Hofstadter, David Kappel, Laurent Jorda, M. T. Capria, Yann Brouet, Nicolas Thomas, P. Schloerb, Sergey Rodionov, J.-B. Vincent, David Marshall, Rafael Rodrigo, Paul Hartogh, Gabriele Arnold, Ladislav Rezac
Publikováno v:
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2018, 616, pp.A122. ⟨10.1051/0004-6361/201833104⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 616, pp.A122. ⟨10.1051/0004-6361/201833104⟩
Marshall, D.; Groussin, O.; Vincent, J.-B.; Brouet, Yann; Kappel, D.; Arnold, G.; Capria, M. T.; Filacchione, G.; Hartogh, P.; Hofstadter, M.; Ip, W.-H.; Jorda, L.; Kuehrt, E.; Lellouch, E.; Mottola, S.; Rezac, L.; Rodrigo, Rafael; Rodionov, S.; Schloerb, P. and Thomas, Nicolas (2018). Thermal inertia and roughness of the nucleus of comet 67P/Churyumov-Gerasimenko from MIRO and VIRTIS observations. Astronomy and astrophysics, 616, A122. EDP Sciences 10.1051/0004-6361/201833104
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2018, 616, pp.A122. ⟨10.1051/0004-6361/201833104⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2018, 616, pp.A122. ⟨10.1051/0004-6361/201833104⟩
Marshall, D.; Groussin, O.; Vincent, J.-B.; Brouet, Yann; Kappel, D.; Arnold, G.; Capria, M. T.; Filacchione, G.; Hartogh, P.; Hofstadter, M.; Ip, W.-H.; Jorda, L.; Kuehrt, E.; Lellouch, E.; Mottola, S.; Rezac, L.; Rodrigo, Rafael; Rodionov, S.; Schloerb, P. and Thomas, Nicolas (2018). Thermal inertia and roughness of the nucleus of comet 67P/Churyumov-Gerasimenko from MIRO and VIRTIS observations. Astronomy and astrophysics, 616, A122. EDP Sciences 10.1051/0004-6361/201833104
Aims.Using data from the Rosetta mission to comet 67P/Churyumov–Gerasimenko, we evaluate the physical properties of the surface and subsurface of the nucleus and derive estimates for the thermal inertia (TI) and roughness in several regions on the
Publikováno v:
Icarus
Icarus, Elsevier, 2016, 270, pp.389-398. ⟨10.1016/j.icarus.2015.07.021⟩
Icarus, 2016, 270, pp.389-398. ⟨10.1016/j.icarus.2015.07.021⟩
Icarus, Elsevier, 2016, 270, pp.389-398. ⟨10.1016/j.icarus.2015.07.021⟩
Icarus, 2016, 270, pp.389-398. ⟨10.1016/j.icarus.2015.07.021⟩
We have analyzed spectroscopic observations of Titan performed in January 1997 by the Short Wavelength Spectrometer (SWS) on the Infrared Space Observatory in the wavelength range from 5.3 to 7.0 μm (1422–1890 cm −1 ). This spectral interval is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::94639d527ac4925425ff1fb723a40c7a
https://hal.archives-ouvertes.fr/hal-02459395
https://hal.archives-ouvertes.fr/hal-02459395
Autor:
Bruno Bézard, Emmanuel Lellouch, Barry L. Lutz, Catherine de Bergh, Jacques Crovisier, Jean-Pierre Maillard
Publikováno v:
Planetary and Space Science. 54:1398-1414
In January 1987, high-resolution spectra of the dayside of Venus in the 2080– 2185 cm - 1 range, recorded with the Canada–France–Hawaii telescope using a Fourier-transform spectrometer, revealed two sequences of narrow emission lines, correspon
Autor:
Emmanuel Lellouch
Publikováno v:
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences. 364:3139-3146
Narrow-band filter, high-spectral-resolution (0.2 cm −1 ) spectro-imaging infrared observations of Jupiter's auroral zones, acquired in October 1999 and October 2000 with the FTS/BEAR instrument at the Canada–France–Hawaii Telescope, have provi
Autor:
Bernard Schmitt, Alberto Salama, Athena Coustenis, Pierre Drossart, Bernhard Schulz, Thérèse Encrenaz, Emmanuel Lellouch, Vincent Boudon, Alberto Negrão, Andrei Nikitin, Pascal Rannou
Publikováno v:
Icarus
Icarus, Elsevier, 2006, 180, pp.176-185. ⟨10.1016/j.icarus.2005.08.007⟩
Icarus, Elsevier, 2006, 180, pp.176-185. 〈10.1016/j.icarus.2005.08.007〉
Icarus, 2006, 180, pp.176-185. ⟨10.1016/j.icarus.2005.08.007⟩
Icarus, Elsevier, 2006, 180, pp.176-185. ⟨10.1016/j.icarus.2005.08.007⟩
Icarus, Elsevier, 2006, 180, pp.176-185. 〈10.1016/j.icarus.2005.08.007〉
Icarus, 2006, 180, pp.176-185. ⟨10.1016/j.icarus.2005.08.007⟩
The near-infrared spectrum of Titan, Saturn's largest moon and one of the Cassini/Huygens' space mission primary targets, covers the 0.8 to 5 micron region in which it shows several weak CH 4 absorption regions, and in particular one centered near 2.
Autor:
Miguel Lopez-Valverde, J. J. Lopez-Moreno, Emmanuel Lellouch, Pierre Drossart, Vittorio Formisano, Davide Grassi, Manuel López-Puertas, A. Maturilli
Publikováno v:
Planetary and Space Science. 53:1079-1087
Daytime nadir spectra of the Martian atmosphere taken by the planetary Fourier spectrometer/Mars Express (PFS) and by the infrared space observatory (ISO) in the 4.3 μ m region are analyzed using a theoretical non-LTE model of the CO 2 infrared emis
Autor:
Emmanuel Lellouch, Thomas K. Greathouse, John R. Spencer, Miguel Lopez-Valverde, Jean-Marie Flaud, Kandis Lea Jessup, Matthew J. Richter
Publikováno v:
Icarus. 176:283-304
We have observed about 16 absorption lines of the ν 2 SO2 vibrational band on Io, in disk-integrated 19-μm spectra taken with the TEXES high spectral resolution mid-infrared spectrograph at the NASA Infrared Telescope Facility in November 2001, Dec
Autor:
Pablo Santos-Sanz, John Stansberry, Esa Vilenius, Cs. Kiss, Thomas G. Müller, András Pál, Florence Henry, Paul Hartogh, Emmanuel Lellouch, A. Delsanti, N. Szalai, Gábor Marton, E. Verebelyi
Publikováno v:
Experimental Astronomy
Experimental Astronomy, Springer Link, 2014, 37 (2), pp.161-174. ⟨10.1007/s10686-013-9350-5⟩
Experimental Astronomy, 2014, 37 (2), pp.161-174. ⟨10.1007/s10686-013-9350-5⟩
Experimental Astronomy, Springer Link, 2014, 37 (2), pp.161-174. ⟨10.1007/s10686-013-9350-5⟩
Experimental Astronomy, 2014, 37 (2), pp.161-174. ⟨10.1007/s10686-013-9350-5⟩
The "TNOs are Cool!: A survey of the trans-Neptunian region" is a Herschel Open Time Key Program that aims to characterize planetary bodies at the outskirts of the Solar System using PACS and SPIRE data, mostly taken as scan-maps. In this paper we su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::81152d72fbf348f73deafc3350698f3f
https://hal.archives-ouvertes.fr/hal-02544487
https://hal.archives-ouvertes.fr/hal-02544487
Autor:
Bruno Bézard, Helmut Feuchtgruber, T. Encrenaz, Emmanuel Lellouch, T. de Graauw, Thierry Fouchet
Publikováno v:
Astronomy & astrophysics, 370(2), 610-622. EDP Sciences
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (ISO) are used to determine the D/H ratio in Jupiter's and Saturn's atmospheres. The D/H ratio is measured independently in hydrogen (i.e. from the HD/H-