Nonlinear impact monitoring: line of variation searches for impactors
- Author
- MILANI, Andrea1 ; CHESLEY, Steven R2 ; SANSATURIO, Maria Eugenia3 ; TOMMEI, Giacomo1 ; VALSECCHI, Giovanni B4
[1] Dipartimento di Matematica, Università di Pisa, Via Buonarroti 2, 56127 Pisa, Italy
[2] Jet Propulsion Laboratory, CalTech Pasadena, CA 91109, United States
[3] E.T.S. de Ingenieros Industriales, University of Valladolid, Paseo del Cauce s/n, 47011 Valladolid, Spain
[4] IASF-INAF, Via Fosso del Cavaliere 100, 00133 Roma, Italy - Source
Icarus (New York, NY). 2005, Vol 173, Num 2, pp 362-384, 23 p ; ref : 20 ref
- CODEN
- ICRSA5
- ISSN
- 0019-1035
- Scientific domain
- Astronomy earth cosmic environment; Geology
- Publisher
- Elsevier, San Diego, CA
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- Celestial mechanics; Asteroids dynamics; Impacts
- Keyword (fr)
- Astéroïde Classification Condition initiale Densité probabilité Dynamique Elément orbital Fonction densité probabilité Mécanique céleste Méthode itérative Non linéarité Orbite Performance Probabilité Problème n corps Section efficace Système solaire
- Keyword (en)
- Asteroids Classification Initial conditions Probability density Dynamics Orbital elements Probability density function Celestial mechanics Iterative methods Nonlinearity Orbits Performance Probability N-body problems Cross sections Solar system
- Keyword (es)
- Densidad probabilidad Función densidad probabilidad No linealidad
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16598548
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1016/j.icarus.2004.09.002 
https://dx.doi.org/10.1016/j.icarus.2004.09.002
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