Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Frédéric Chambat"'
Autor:
Yanick Ricard, Frédéric Chambat
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 2, p 163 (2024)
Condensed planets contract or expand as their temperature changes. With the exception of the effect of phase changes, this phenomenon is generally interpreted as being solely related to the thermal expansivity of the planet’s components. However, c
Externí odkaz:
https://doaj.org/article/6f348ed569ce49ceab6276a0e7754be5
Publikováno v:
Comptes Rendus. Mathématique
Comptes Rendus. Mathématique, 2021, 359 (2), pp.805-811. ⟨10.5802/crmath.223⟩
Comptes Rendus. Mathématique, 2021, 359 (2), pp.805-811. ⟨10.5802/crmath.223⟩
International audience
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab62715d1dd292472807964d3c0a914f
https://hal.science/hal-04134276/document
https://hal.science/hal-04134276/document
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, 2017, 850 (1), pp.L9. ⟨10.3847/2041-8213/aa95bd⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 850 (1), pp.L9. ⟨10.3847/2041-8213/aa95bd⟩
The Astrophysical journal letters, 2017, 850 (1), pp.L9. ⟨10.3847/2041-8213/aa95bd⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 850 (1), pp.L9. ⟨10.3847/2041-8213/aa95bd⟩
International audience; The large transneptunian objects (TNO) with radii larger than 400 km are thought to be in hydrostatic equilibrium. Their shapes can bring clues on their internal structures that would reveal information on their formation and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0876d5ae985f25893d4f89f56aa9c08d
https://hal.sorbonne-universite.fr/hal-01662024/document
https://hal.sorbonne-universite.fr/hal-01662024/document
Publikováno v:
Geophysical Journal International. 189:1557-1564
SUMMARY In a system where two phases coexist, a seismic wave can disrupt the pre-existing equilibrium and induce a re-equilibration process. Because the kinetics of the phase change is not instantaneous, the transformation induces an attenuation of t
Publikováno v:
Astronomy & Astrophysics
Astronomy & Astrophysics, 2015, 584, ⟨10.1051/0004-6361/201527005⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2015, 584, ⟨10.1051/0004-6361/201527005⟩
Astronomy & Astrophysics, 2015, 584, ⟨10.1051/0004-6361/201527005⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2015, 584, ⟨10.1051/0004-6361/201527005⟩
International audience; Context. We investigate the hydrostatic shape and gravitational potential coefficients of self-gravitating and rotating bodies large enough to have undergone internal differentiation and chemical stratification. Quantifying th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::37befb0dfea88a1fef7a9c952515d5c4
https://hal-univ-lyon1.archives-ouvertes.fr/hal-02340928/file/aa27005-15.pdf
https://hal-univ-lyon1.archives-ouvertes.fr/hal-02340928/file/aa27005-15.pdf
Publikováno v:
Comptes Rendus Géoscience
Comptes Rendus Géoscience, Elsevier, 2014, 346 (5-6), pp.110-118. ⟨10.1016/j.crte.2014.04.006⟩
Comptes Rendus Géoscience, 2014, 346 (5-6), pp.110-118. ⟨10.1016/j.crte.2014.04.006⟩
Comptes Rendus Géoscience, Elsevier, 2014, 346 (5-6), pp.110-118. ⟨10.1016/j.crte.2014.04.006⟩
Comptes Rendus Géoscience, 2014, 346 (5-6), pp.110-118. ⟨10.1016/j.crte.2014.04.006⟩
cited By 3; International audience; We consider a fluid crossing a zone of rapid density change, so thin that it can be considered as a density jump interface. In this case, the normal velocity undergoes a jump. For a Newtonian viscous fluid with low
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b70d2a631eea5b6c6eb2cda92bdcbd7c
https://hal.archives-ouvertes.fr/hal-02046716
https://hal.archives-ouvertes.fr/hal-02046716
Publikováno v:
Earth and Planetary Science Letters
Earth and Planetary Science Letters, Elsevier, 2014, 388, pp.257-264. ⟨10.1016/j.epsl.2013.12.008⟩
Earth and Planetary Science Letters, Elsevier, 2014, 388, pp. 257--264. ⟨10.1016/j.epsl.2013.12.008.⟩
Earth and Planetary Science Letters, 2014, 388, pp. 257--264. ⟨10.1016/j.epsl.2013.12.008⟩
Earth and Planetary Science Letters, Elsevier, 2014, 388, pp.257-264. ⟨10.1016/j.epsl.2013.12.008⟩
Earth and Planetary Science Letters, Elsevier, 2014, 388, pp. 257--264. ⟨10.1016/j.epsl.2013.12.008.⟩
Earth and Planetary Science Letters, 2014, 388, pp. 257--264. ⟨10.1016/j.epsl.2013.12.008⟩
International audience; The small scale heterogeneity of the mantle is mostly due to the mixing of petrological heterogeneities by a smooth but chaotic convection and should consist in a laminated structure (marble cake) with a power spectrum S(k) va
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e5d8e6cfb755921ecb488085470125d
https://hal.archives-ouvertes.fr/hal-02944834/document
https://hal.archives-ouvertes.fr/hal-02944834/document
Publikováno v:
International Journal of Crashworthiness
International Journal of Crashworthiness, 2006, 338, pp.992-1001
Comptes Rendus Geoscience
International Journal of Crashworthiness, Taylor & Francis, 2006, 338, pp.992-1001
International Journal of Crashworthiness, 2006, 338, pp.992-1001
Comptes Rendus Geoscience
International Journal of Crashworthiness, Taylor & Francis, 2006, 338, pp.992-1001
The determination of Earth's gravity field has benefited from various gravity missions that have been launched recently (CHAMP and GRACE) and a new quantitative jump should be made by the GOCE mission in a few more years. For the first time, a global
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::280e5f59b1a548ce3cb2244cbc65bb3d
https://hal.science/hal-00337384
https://hal.science/hal-00337384
Autor:
Frédéric Chambat, Bernard Valette
Publikováno v:
Physics of the Earth and Planetary Interiors
Physics of the Earth and Planetary Interiors, Elsevier, 2005, 151 (1-2), pp.89-106. ⟨10.1016/j.pepi.2005.01.002⟩
Physics of the Earth and Planetary Interiors, 2005, 151 (1-2), pp.89-106. ⟨10.1016/j.pepi.2005.01.002⟩
Physics of the Earth and Planetary Interiors, Elsevier, 2005, 151, pp.89-106. ⟨10.1016/j.pepi.2005.01.002⟩
Physics of the Earth and Planetary Interiors, 2005, 151, pp.89-106. ⟨10.1016/j.pepi.2005.01.002⟩
Physics of the Earth and Planetary Interiors, Elsevier, 2005, 151 (1-2), pp.89-106. ⟨10.1016/j.pepi.2005.01.002⟩
Physics of the Earth and Planetary Interiors, 2005, 151 (1-2), pp.89-106. ⟨10.1016/j.pepi.2005.01.002⟩
Physics of the Earth and Planetary Interiors, Elsevier, 2005, 151, pp.89-106. ⟨10.1016/j.pepi.2005.01.002⟩
Physics of the Earth and Planetary Interiors, 2005, 151, pp.89-106. ⟨10.1016/j.pepi.2005.01.002⟩
International audience; The previous termgravitynext term potential of a planet is usually expanded previous termupnext term to first previous termordernext term only as a linear function of previous termtopographynext term and lateral variations of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e07a4fa8b26713bd473d8ece3129904
https://hal-insu.archives-ouvertes.fr/insu-00271517
https://hal-insu.archives-ouvertes.fr/insu-00271517
Autor:
Frédéric Chambat, Yanick Ricard
Publikováno v:
Geophysical Journal International
Geophysical Journal International, Oxford University Press (OUP), 2005, 162, pp.32-35
HAL
Geophysical Journal International, 2005, 162, pp.32-35
Geophysical Journal International, Oxford University Press (OUP), 2005, 162, pp.32-35
HAL
Geophysical Journal International, 2005, 162, pp.32-35
International audience; Various papers have discussed the forward relationships between internal density anomalies of a planet and its external gravity field. The inverse modeling, i.e. finding the internal density anomalies from the external potenti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6a2c4a92bc0c2cfe210a8d7f1ecfbb4
https://hal.archives-ouvertes.fr/hal-00093156
https://hal.archives-ouvertes.fr/hal-00093156