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Infrared backscatteringAll particles in the atmosphere are not spherical. Moreover, the scattering properties of randomly oriented nonspherical particles are not equivalent to those of spherical particles no matter how the term equivalent is defined. This is especially true for scattering in the backward direction and at the infrared wavelengths at which some atmospheric particles have strong absorption bands. Thus calculations based on Mie theory of infrared backscattering by dry or insoluble atmospheric particles are suspect. To support this assertion, it was noted that peaks in laboratory-measured infrared backscattering spectra show appreciable shifts compared with those calculated using Mie theory. One example is ammonium sulfate. Some success was had in modeling backscattering spectra of ammonium sulfate particles using a simple statistical theory called the continuous distribution of ellipsoids (CDE) theory. In this theory, the scattering properties of an ensemble are calculated. Recently a modified version of this theory was applied to measured spectra of scattering by kaolin particles. The particles were platelike, so the probability distribution of ellipsoidal shapes was chosen to reflect this. As with ammonium sulfate, the wavelength of measured peak backscattering is shifted longward of that predicted by Mie theory.
Document ID
19900002767
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Bohren, Craig F.
(Pennsylvania State Univ. University Park, PA, United States)
Nevitt, Timothy J.
(Pennsylvania State Univ. University Park, PA, United States)
Singham, Shermila Brito
(Pennsylvania State Univ. University Park, PA, United States)
Date Acquired
September 6, 2013
Publication Date
February 1, 1989
Publication Information
Publication: NASA, Marshall Space Flight Center, NASA(MSFC FY88 Global Scale Atmospheric Processes Research Program Review
Subject Category
Geophysics
Accession Number
90N12083
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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