Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Sandrine D'Hoedt"'
Publikováno v:
Biological Control. 58:103-112
Quantitative food webs were constructed from the data collected, using visual observation technique, from May to July in 2005 and 2006 to describe separately the trophic relationships between the community of aphids and their natural enemies of preda
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::edbb5f4d2b56e955323dd26bb0e7532a
https://doi.org/10.1016/j.biocontrol.2011.04.005
https://doi.org/10.1016/j.biocontrol.2011.04.005
Autor:
Sandrine D’Hoedt, Anne Lemaitre
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 101:127-139
The averaged spin-orbit resonant motion of Mercury is considered, with e the orbital eccentricity, and io the orbital inclination introduced as very slow functions of time, given by any secular planetary theory. The basis is our Hamiltonian approach
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9b1fb9b87c0fd8e62d4a4fe05c0b809c
https://doi.org/10.1007/s10569-007-9115-4
https://doi.org/10.1007/s10569-007-9115-4
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 96:253-258
Mercury is observed in a stable Cassini’s state, close to a 3:2 spin-orbit resonance, and a 1:1 node resonance. This present situation is not the only possible mathematical stable state, as it is shown here through a simple model limited to the sec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2d31b94a2281365c0ed9af425f0d8a0f
https://doi.org/10.1007/s10569-006-9041-x
https://doi.org/10.1007/s10569-006-9041-x
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 95:213-224
Our purpose is to build a model of rotation for a rigid Mercury, involving the planetary perturbations and the non-spherical shape of the planet. The approach is purely analytical, based on Hamiltonian formalism; we start with a first-order basic ave
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::66433a6ecb02907251ba8bf11d4c3741
https://doi.org/10.1007/s10569-006-9032-y
https://doi.org/10.1007/s10569-006-9032-y
Autor:
Anne Lemaitre, Sandrine D’Hoedt
Publikováno v:
Celestial Mechanics and Dynamical Astronomy. 89:267-283
The paper develops a hamiltonian formulation describing the coupled orbital and spin motions of a rigid Mercury rotation about its axis of maximum moment of inertia in the frame of a 3:2 spin orbit resonance; the (ecliptic) obliquity is not constant,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::90cdf7d5612ae2426abfc9244a1ddc3a
https://doi.org/10.1023/b:cele.0000038607.32187.d4
https://doi.org/10.1023/b:cele.0000038607.32187.d4
Autor:
Sandrine D’Hoedt, Benoît Noyelles
Publikováno v:
Planetary and Space Science
Planetary and Space Science, 2012, 60 (1), pp.274-286. ⟨10.1016/j.pss.2011.07.024⟩
Planetary and Space Science, Elsevier, 2012, 60 (1), pp.274-286. ⟨10.1016/j.pss.2011.07.024⟩
Planetary and Space Science, 2012, 60 (1), pp.274-286. ⟨10.1016/j.pss.2011.07.024⟩
Planetary and Space Science, Elsevier, 2012, 60 (1), pp.274-286. ⟨10.1016/j.pss.2011.07.024⟩
Mercury is the target of the space missions MESSENGER and BepiColombo, that will in particular observe its rotation to get information on its internal structure. This requires a rigorous modelization of this rotation. A difficulty comes from the obli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9faf2c69afd5a3058b2a2b9a0e01eeec
https://hal.science/hal-02612827
https://hal.science/hal-02612827
Publikováno v:
Celestial Mechanics and Dynamical Astronomy
Celestial Mechanics and Dynamical Astronomy, 2010, 107 (1-2), pp.93-100. ⟨10.1007/s10569-010-9262-x⟩
Celestial Mechanics and Dynamical Astronomy, Springer Verlag, 2010, 107 (1-2), pp.93-100. ⟨10.1007/s10569-010-9262-x⟩
Celestial Mechanics and Dynamical Astronomy, 2010, 107 (1-2), pp.93-100. ⟨10.1007/s10569-010-9262-x⟩
Celestial Mechanics and Dynamical Astronomy, Springer Verlag, 2010, 107 (1-2), pp.93-100. ⟨10.1007/s10569-010-9262-x⟩
International audience; The resonant rotation of Mercury can be modelised by a kernel model on which we can add perturbations. Our kernel model is a two-degree of freedom one written in Hamiltonian formalism. For this kernel, we consider that Mercury
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a47918b9d82d1b03e52e2fb15b0edd03
https://hal.science/hal-00552505
https://hal.science/hal-00552505
Publikováno v:
Advances in Space Research
Advances in Space Research, 2009, 44, pp.597-603. ⟨10.1016/j.asr.2009.05.008⟩
Advances in Space Research, 2009, 44, pp.597-603. ⟨10.1016/j.asr.2009.05.008⟩
International audience; Mercury is the target of two space missions: MESSENGER, which carried out its first and second flybys of Mercury on January 14, 2008 and October 6, 2008, and the ESA/JAXA space mission BepiColombo, scheduled to arrive at Mercu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::175a627cb8ec9aac6595f940dfdd9a85
https://hal.science/hal-03742288
https://hal.science/hal-03742288
Publikováno v:
Periodic, Quasi-Periodic and Chaotic Motions in Celestial Mechanics: Theory and Applications ISBN: 9781402053245
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d78381065266c49034b1f4def4dd2fa4
https://doi.org/10.1007/978-1-4020-5325-2_12
https://doi.org/10.1007/978-1-4020-5325-2_12
Publikováno v:
57th International Astronautical Congress.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::32c922948c5855fea43f21507ad02139
https://doi.org/10.2514/6.iac-06-a3.p.2.02
https://doi.org/10.2514/6.iac-06-a3.p.2.02