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Size-Dependent Scattering Properties of Planetary Regolith AnalogsParticles in a planetary regolith can be treated as independent scatterers when their size is large compared with the wavelength of light. The nature of this scattering, however, is poorly understood as the particle size approaches and becomes smaller than the wavelength. In order to understand this interaction better, the reflectances of well-sorted particulate samples of known composition were measured. This reflectance data was then analyzed to determine how scattering properties change with particle size.
Document ID
20020074753
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Piatek, J. L.
(Pittsburgh Univ. United States)
Hapke, B.
(Pittsburgh Univ. United States)
Nelson, R. M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Hale, A. S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Smythe, W. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2002
Publication Information
Publication: Solar System Remote Sensing
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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