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A radiative transfer model to simulate light scattering in a compact granular medium using a Monte-Carlo approach: Validation and first applications

Author
PILORGET, C1 2 ; VINCENDON, M1 ; POULET, F1
[1] Institut d'Astrophysique Spatiale, Universite de Paris Sud 11, Orsay, France
[2] Division of Geological and Planetary Sciences, Caltech, Pasadena, California, United States
Source

Journal of geophysical research. Planets (Print). 2013, Vol 118, Num 12, pp 2488-2501, 14 p ; ref : 3/4 p

ISSN
2169-9097
Scientific domain
Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
Publisher
Wiley, Hoboken, NJ
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Albédo Diffusion lumière Facteur réflexion Fonction phase Modèle Méthode Monte Carlo Paramètre physique Propriété physique Surface planétaire Transfert radiatif
Keyword (en)
Albedo Light scattering Reflectivity Phase function Models Monte Carlo methods Physical parameter Physical properties Planetary surfaces Radiative transfer
Keyword (es)
Función fase Modelo Parámetro físico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A30 Fundamental aspects of astrophysics / 001E03A30J Radiative transfer ; scattering

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B35 Planetary, asteroid, and satellite characteristics and properties / 001E03B35G Surface features, cratering, and topography

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
28126639

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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