Zobrazeno 1 - 10
of 58
pro vyhledávání: '"J. Brillet"'
Publikováno v:
Annales Geophysicae, Vol 12, Pp 664-673 (1994)
Ground-based microwave measurements of the diurnal and seasonal variations of ozoneat 42±4.5 and 55±8 km are validated by comparing with results from a zero-dimensional photochemical model and a two-dimensional (2D) chemical/radiative/dynamical
Externí odkaz:
https://doaj.org/article/60201b1b381b46c5ad6c1e1aeaaa6e9e
Publikováno v:
Annales Geophysicae, Vol 12, Iss 7, Pp 664-673 (0000)
Ground-based microwave measurements of the diurnal and seasonal variations of ozoneat 42±4.5 and 55±8 km are validated by comparing with results from a zero-dimensional photochemical model and a two-dimensional (2D) chemical/radiative/dynamical mod
Externí odkaz:
https://doaj.org/article/56fb5819fb8046a3b92e3ca627bc7157
Publikováno v:
Annales Geophysicae
Annales Geophysicae, European Geosciences Union, 1994, 12 (7), pp.664-673. ⟨10.1007/s00585-994-0664-5⟩
Annales Geophysicae, Vol 12, Pp 664-673 (1994)
Annales Geophysicae, Vol 12, Iss 7, Pp 664-673 (0000)
Annales Geophysicae, European Geosciences Union, 1994, 12 (7), pp.664-673. ⟨10.1007/s00585-994-0664-5⟩
Annales Geophysicae, Vol 12, Pp 664-673 (1994)
Annales Geophysicae, Vol 12, Iss 7, Pp 664-673 (0000)
Ground-based microwave measurements of the diurnal and seasonal variations of ozoneat 42±4.5 and 55±8 km are validated by comparing with results from a zero-dimensional photochemical model and a two-dimensional (2D) chemical/radiative/dynamical mod
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::351c0372f8a7ecb03b7e31066dda1f23
https://www.ann-geophys.net/12/664/1994/
https://www.ann-geophys.net/12/664/1994/
Vertical temperature profile and mesospheric winds retrieval on Mars from CO millimeter observations
Autor:
F. Billebaud, Michel Dobrijevic, François Forget, J. Brillet, Thibault Cavalié, T. Encrenaz, E. Lellouch
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2008, 489 (2), pp.795-809. ⟨10.1051/0004-6361:200809815⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2008, 489 (2), pp.795-809. ⟨10.1051/0004-6361:200809815⟩
Astronomy and Astrophysics-A&A, 2008, 489 (2), pp.795-809. ⟨10.1051/0004-6361:200809815⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2008, 489 (2), pp.795-809. ⟨10.1051/0004-6361:200809815⟩
Aims. We have recorded high spectral resolution spectra and derived precise atmospheric temperature profiles and wind velocities in the atmosphere of Mars. We have compared observations of the planetary mean thermal profile and mesospheric wind veloc
Publikováno v:
Astronomy & Astrophysics. 416:783-789
For meteor shower forecasting on the other planets of the Solar System, we have identified a list of periodic comets having close enough encounters with planetary orbits to produce regular showers. We revisit a previous study, done with an analytical
Publikováno v:
Astronomy & Astrophysics. 398:335-344
Reaction rates included in photochemical models of planetary atmospheres carry with them a level of imprecision. This imprecision leads to an uncertainty in computed mole fractions of chemical species. We present estimations of the uncer- tainties on
Publikováno v:
Advances in Space Research. 17:223-226
The available light in the atmosphere of Titan has been calculated using a Monte Carlo method. The “recommended” temperature profile derived by Lellouch /1/, the aerosol distribution from McKay /2/ and their properties from Khare /3/, and an atmo
Autor:
J. Brillet, N. Biver, E. Lellouch, Michael Olberg, Michel Dobrijevic, Urban Frisk, Thibault Cavalié, Alain Lecacheux, Åke Hjalmarson, F. Billebaud, Paul Hartogh, Aa. Sandqvist
Publikováno v:
Planetary and Space Science
Planetary and Space Science, 2012, 61 (1), pp.3-14. ⟨10.1016/j.pss.2011.04.001⟩
Planetary and Space Science, Elsevier, 2012, 61 (1), pp.3-14. ⟨10.1016/j.pss.2011.04.001⟩
Planetary and Space Science, 2012, 61 (1), pp.3-14. ⟨10.1016/j.pss.2011.04.001⟩
Planetary and Space Science, Elsevier, 2012, 61 (1), pp.3-14. ⟨10.1016/j.pss.2011.04.001⟩
International audience; The Odin space telescope has monitored the H2O (110-101) line in Jupiter's stratosphere over the 2003-2009 period. When comparing these data with previous spectra obtained with SWAS and Odin over the 1999-2002 period, we see n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e214bd80cfe5149bc7a017b46eed63c3
https://hal.science/hal-00623438
https://hal.science/hal-00623438
Autor:
Michel Dobrijevic, G. H. Moriarty-Schieven, Emmanuel Lellouch, F. Billebaud, T. Encrenaz, T. Fouchet, Paul Hartogh, Thibault Cavalié, J. Brillet
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 510 (A88), ⟨10.1051/0004-6361/200912909⟩
Astronomy and Astrophysics-A&A, 2010, 510 (A88), ⟨10.1051/0004-6361/200912909⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 510 (A88), ⟨10.1051/0004-6361/200912909⟩
Astronomy and Astrophysics-A&A, 2010, 510 (A88), ⟨10.1051/0004-6361/200912909⟩
International audience; Context. The CO(3–2) line has been observed in the atmosphere of Saturn. The CO(3–2) observation proves that an external source of CO exists in the stratosphere of the planet. Aims. We attempt to constrain the type and mag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c64d86ec8615abbba174226645997dde
https://hal.archives-ouvertes.fr/hal-00458647
https://hal.archives-ouvertes.fr/hal-00458647
Autor:
Thierry Fouchet, J. Brillet, J. G. A. Wouterloot, Thibault Cavalié, E. Lellouch, G. H. Moriarty-Schieven, Michel Dobrijevic, F. Billebaud, Paul Hartogh, T. Encrenaz
Publikováno v:
Icarus
Icarus, Elsevier, 2009, 203 (2), pp.531-540. ⟨10.1016/j.icarus.2009.05.024⟩
Icarus, 2009, 203 (2), pp.531-540. ⟨10.1016/j.icarus.2009.05.024⟩
Icarus, Elsevier, 2009, 203 (2), pp.531-540. ⟨10.1016/j.icarus.2009.05.024⟩
Icarus, 2009, 203 (2), pp.531-540. ⟨10.1016/j.icarus.2009.05.024⟩
We have performed the first observation of the CO(3-2) spectral line in the atmosphere of Saturn with the James Clerk Maxwell Telescope. We have used a transport model of the atmosphere of Saturn to constrain the origin of the observed CO. The CO lin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::904221db360cb616e5244c2f95ca4ae3
https://hal.archives-ouvertes.fr/hal-00400419/file/cavalie2009-14.pdf
https://hal.archives-ouvertes.fr/hal-00400419/file/cavalie2009-14.pdf