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Radiative transfer in closely packed realistic regoliths

Author(s): Vahidinia, S; Cuzzi, J; Draine, Bruce T.; Marouf, E

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dc.contributor.authorVahidinia, S-
dc.contributor.authorCuzzi, J-
dc.contributor.authorDraine, Bruce T.-
dc.contributor.authorMarouf, E-
dc.date.accessioned2019-05-30T16:00:01Z-
dc.date.available2019-05-30T16:00:01Z-
dc.date.issued2011-12-01en_US
dc.identifier.citationVahidinia, S, Cuzzi, J, Draine, B, Marouf, E. (2011). Radiative transfer in closely packed realistic regoliths. AAPP Atti della Accademia Peloritana dei Pericolanti, Classe di Scienze Fisiche, Matematiche e Naturali, 89 (SUPPL. 1), 10.1478/C1V89S1P089en_US
dc.identifier.issn0365-0359-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr14f01-
dc.description.abstractWe have developed a regolith radiative transfer model (RRT) based on a frst-principles approach to regolith modeling that is essential for near-to-far infrared observations of grainy surfaces, and is readily confgured to answer fundamental questions about popular models with which all remote observations of all airless solar system bodies with granular surfaces are currently interpreted. Our model accounts for wavelength-size regolith particles which are closely packed and can be heterogeneous in composition and arbitrarily shaped. Here we present preliminary results showing the role of porosity on layer refectivity. © 2011 by the Author(s); licensee Accademia Peloritana dei Pericolanti, Messina, Italy.en_US
dc.language.isoen_USen_US
dc.relation.ispartofAAPP Atti della Accademia Peloritana dei Pericolanti, Classe di Scienze Fisiche, Matematiche e Naturalien_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleRadiative transfer in closely packed realistic regolithsen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1478/C1V89S1P089-
dc.identifier.eissn1825-1242-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/conference-proceedingen_US

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