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Light scattering by size-shape distributions of randomly oriented axially symmetric particles of a size comparable to a wavelengthRigorously light scattering by size-shape distributions of randomly oriented axially symmetric particles are calculated by the T-matrix method, as extended to randomly oriented scatterers. The computational scheme is described along with a newly developed convergence procedure that makes it possible to substantially reduce computer time and storage requirements. The elements of the Stokes scattering matrix for a power-law size distribution of randomly oriented moderately aspherical spheroids are shown to be much smoother than and differ substantially from those of equivalent monodisperse spheroids; averaging over orientations does not eliminate the necessity of averaging over particle sizes. The angular-scattering behavior of the ensembles of nonspherical particles is found to be significantly different from that of the equivalent polydisperse spheres.
Document ID
19930070917
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mishchenko, Michael I.
(NASA Goddard Inst. for Space Studies; Hughes STX Corp. New York, United States)
Date Acquired
August 16, 2013
Publication Date
August 20, 1993
Publication Information
Publication: Applied Optics
Volume: 32
Issue: 24
ISSN: 0003-6935
Subject Category
Optics
Accession Number
93A54914
Distribution Limits
Public
Copyright
Other

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