Radiative transfer simulation of water rotational excitation in comets : Comparison of the Monte Carlo and escape probability methods
- Author
- ZAKHAROV, V1 ; BOCKELEE-MORVAN, D1 ; BIVER, N1 ; CROVISIER, J1 ; LECACHEUX, A1
[1] LESIA, Observatoire de Paris -Section de Meudon, 5 place Jules Janssen, 92195 Meudon, France - Source
Astronomy and astrophysics (Berlin. Print). 2007, Vol 473, Num 1, pp 303-310, 8 p ; ref : 1/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- comets: général line: formation methods: numerical radiative transfer radio lines: solar system submillimeter
- Keyword (fr)
- Algorithme Autoabsorption Comète Densité électron Distribution densité Détecteur IR Excitation Formation raie Gradient température Intensité excitation Intensité raie Modèle Méthode Monte Carlo Méthode numérique Probabilité Profil raie Symétrie sphérique Système solaire Taux production Température électron Transfert radiatif Transition rotationnelle Vitesse expansion
- Keyword (en)
- Algorithms Self-absorption Comets Electron density Density distribution Infrared detectors Excitation Line formation Temperature gradients Excitation intensity Line intensity Models Monte Carlo methods Numerical method Probability Line shape Spherical symmetry Solar system Production rate Electron temperature Radiative transfer Rotational transition Expansion velocity
- Keyword (es)
- Distribución densidad Intensidad excitación Modelo Método numérico Simetría esférica Índice producción Transición rotacional Velocidad expansión
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19064265
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
10.1051/0004-6361:20066715 
https://dx.doi.org/10.1051/0004-6361:20066715
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