Zobrazeno 1 - 10
of 115
pro vyhledávání: '"V. Vanzani"'
Autor:
Athena Coustenis, J. A. M. McDonnell, G. Bianchini, John C. Zarnecki, V. Vanzani, Enrico Flamini, Konrad Schwingenschuh, Ari-Matti Harri, Peter Falkner, F.H. Neubauer, William J. Borucki, Alvin Seiff, A. Bar-Nun, G.W. Leppelmeier, Håkan Svedhem, Réjean Grard, M. A. Barucci, Giovanni Picardi, Arne Pedersen, J. J. López-Moreno, C. P. McKay, Francesco Angrilli, Michel Hamelin, Valerio Pirronello, Marcello Fulchignoni, Francesca Ferri, Rafael Rodrigo, M. Coradini
Publikováno v:
Space Science Reviews. 104:395-431
The Huygens Atmospheric Structure Instrument (HASI) is a multi-sensor package which has been designed to measure the physical quantities characterising the atmosphere of Titan during the Huygens probe descent on Titan and at the surface. HASI sensors
Autor:
Francesco Marzari, V. Vanzani
Publikováno v:
Planetary and Space Science. 42:101-107
In this paper we study the trapping of dust particles into exterior mean motion resonances with the Earth. We integrate a large number of particle orbits in the context of a many-body problem taking into account the effects of Poynting-Robertson and
Autor:
G. Cattapan, V. Vanzani
Publikováno v:
Few Body Systems and Nuclear Forces I ISBN: 9783540089179
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::876631925e56ad576fa1c62212969a28
https://doi.org/10.1007/3-540-08917-9_304
https://doi.org/10.1007/3-540-08917-9_304
Autor:
V. Vanzani
Publikováno v:
Few Body Systems and Nuclear Forces I ISBN: 9783540089179
We present a general formalism for the N-body scattering problem which allows us to establish various relationships between different formulations existing in the literature. Several of the proposed approaches differ considerably in the way of treati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::18af6c673c204804524b8a047a89f829
https://doi.org/10.1007/3-540-08917-9_301
https://doi.org/10.1007/3-540-08917-9_301
Publikováno v:
Il Nuovo Cimento C. 13:139-145
A systematic comparison of a variable cosmogenic-production rate model (proposed in a previous paper) with the conventional constant-production rate model is carried out. Attention is focussed on the time-integrated concentrations in meteorites. A gr
Autor:
M. Fulchignoni, E. Ferri, F. Angrilli, A. Bar-Nun, M. A. Barucci, G. Bianchini, W. Borucki, M. Coradini, A. Coustenis, P. Falkner, E. Flamini, R. Grard, M. Hamelin, A. M. Harri, G. W. Leppelmeier, J. J. Lopez-Moreno, J. A. M. Mcdonnell, C. P. Mckay, F. H. Neubauer, A. Pedersen, G. Picardi, V. Pirronello, R. Rodrigo, K. Schwingenschuh, A. Seiff, H. Svedhem, V. Vanzani, J. Zarnecki
Publikováno v:
The Cassini-Huygens Mission ISBN: 9789048162086
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c9124b2619f56c524a4a94482be22988
https://doi.org/10.1007/978-94-017-3251-2_11
https://doi.org/10.1007/978-94-017-3251-2_11
Publikováno v:
Scopus-Elsevier
This paper discusses the problem of orbiting a comet nucleus from a perspective of orbital stability. The main forces perturbing the motion of the spacecraft around the comet: shape and rotation rate of the nucleus, comet outgassing, solar radiation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bddd5aea0d4ca5a896770cbd24e0f069
http://hdl.handle.net/11577/2462933
http://hdl.handle.net/11577/2462933
The combined effects are studied of gas drag and gravitational perturbations by a proto-Jupiter on the orbital evolution of a swarm of planetesimals in the primordial asteroid belt in the 2:1 mean motion resonance region. The gas drag in the primordi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c610c6905be7f3b586c11add9e2d720
http://hdl.handle.net/11577/2467876
http://hdl.handle.net/11577/2467876
The evolution of the Earth obliquity when the tidal interactions of the Earth-Moon system will have expanded the lunar orbit to about 66 and 68 Earth radii is studied. By integrating numerically the differential precession equations for the spin axis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1215ddff9d1c9b17b5bcc50340722e52
http://hdl.handle.net/11577/2464352
http://hdl.handle.net/11577/2464352
Most asteroid dynamical families are thought to be the outcomes of collisional disruption of parent asteroids destroyed by high-velocity impacts with other astroids. However, subsequent collisions modify both the sizes and the orbits of family member
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0824b8d11e5502fb28f860b60ddf0779
http://hdl.handle.net/11577/125175
http://hdl.handle.net/11577/125175