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Monte Carlo simulations of light scattering by composite particles in a planetary surface

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dc.contributor.author Hillier, J. en_US
dc.contributor.author Buratti, B. en_US
dc.date.accessioned 2004-09-23T21:14:21Z
dc.date.available 2004-09-23T21:14:21Z
dc.date.issued 2001-01 en_US
dc.identifier.citation Icarus, v. 149, no. 1, pp.251-261 en_US
dc.identifier.citation Aberdeen, WA USA en_US
dc.identifier.clearanceno 00-1702 en_US
dc.identifier.uri http://hdl.handle.net/2014/15909
dc.description.abstract Composite particles containing internal scatterers have been proposed as an explanation for the fact that most photometric studies of planetary surfaces based on Hapke's bidirectional reflectance model have found the planetary particles to exhibit moderately backscattering phase functions. en_US
dc.format.extent 848133 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Bidirectional reflectance spectroscopy asymmetry parameters en_US
dc.title Monte Carlo simulations of light scattering by composite particles in a planetary surface en_US


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