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Extinction-to-Backscatter Ratios of Saharan Dust Layers Derived from In-Situ Measurements and CALIPSO Overflights During NAMMAWe determine the extinction-to-backscatter (Sa) ratios of dust using (1) airborne in-situ measurements of microphysical properties, (2) modeling studies, and (3) the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) observations recorded during the NASA African Monsoon Multidisciplinary Analyses (NAMMA) field experiment conducted from Sal, Cape Verde during Aug-Sept 2006. Using CALIPSO measurements of the attenuated backscatter of lofted Saharan dust layers, we apply the transmittance technique to estimate dust Sa ratios at 532 nm and a 2-color method to determine the corresponding 1064 nm Sa. This method yielded dust Sa ratios of 39.8 plus or minus 1.4 sr and 51.8 plus or minus 3.6 sr at 532 nm and 1064 nm, respectively. Secondly, Sa at both wavelengths is independently calculated using size distributions measured aboard the NASA DC-8 and estimates of Saharan dust complex refractive indices applied in a T-Matrix scheme. We found Sa ratios of 39.1 plus or minus 3.5 sr and 50.0 plus or minus 4 sr at 532 nm and 1064 nm, respectively, using the T-Matrix calculations applied to measured size spectra. Finally, in situ measurements of the total scattering (550 nm) and absorption coefficients (532 nm) are used to generate an extinction profile that is used to constrain the CALIPSO 532 nm extinction profile and thus generate a stratified 532 nm Sa. This method yielded an Sa ratio at 532 nm of 35.7 sr in the dust layer and 25 sr in the marine boundary layer consistent with a predominantly seasalt aerosol near the ocean surface. Combinatorial simulations using noisy size spectra and refractive indices were used to estimate the mean and uncertainty (one standard deviation) of these Sa ratios. These simulations produced a mean (plus or minus uncertainty) of 39.4 (plus or minus 5.9) sr and 56.5 (plus or minus 16.5) sr at 532 nm and 1064 nm, respectively, corresponding to percent uncertainties of 15% and 29%. These results will provide a measurements-based estimate of the dust Sa for use in backscatter lidar inversion algorithms such as CALIOP.
Document ID
20110007908
Acquisition Source
Langley Research Center
Document Type
Preprint (Draft being sent to journal)
Authors
Omar, Ali H. (NASA Langley Research Center Hampton, VA, United States)
Liu, Zhaoyan (National Inst. of Aerospace Associates Hampton, VA, United States)
Vaughan, Mark A. (NASA Langley Research Center Hampton, VA, United States)
Thornhill, Kenneth L., II (Science Systems and Applications, Inc. Hampton, VA, United States)
Kittaka, Chieko (Science Systems and Applications, Inc. Hampton, VA, United States)
Ismail, Syed (NASA Langley Research Center Hampton, VA, United States)
Chen, Gao (NASA Langley Research Center Hampton, VA, United States)
Powell, Kathleen A. (NASA Langley Research Center Hampton, VA, United States)
Winker, David M. (NASA Langley Research Center Hampton, VA, United States)
Trepte, Charles R. (NASA Langley Research Center Hampton, VA, United States)
Trepte, Charles R. (NASA Langley Research Center Hampton, VA, United States)
Winstead, Edward L. (NASA Langley Research Center Hampton, VA, United States)
Anderson, Bruce E. (NASA Langley Research Center Hampton, VA, United States)
Date Acquired
August 25, 2013
Publication Date
January 1, 2010
Subject Category
Geosciences (General)
Report/Patent Number
NF1676L-11156
Funding Number(s)
WBS: WBS 653967.04.12.01
Distribution Limits
Public
Copyright
Public Use Permitted.

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