Papers on Climate and Atmospheric Physics
Wavelength dependence of the optical depth of biomass burning, urban, and desert dust aerosols
Article first published online: 21 SEP 2012
Copyright 1999 by the American Geophysical Union.
Journal of Geophysical Research: Atmospheres (1984–2012)
Volume 104, Issue D24, pages 31333–31349, 27 December 1999
How to Cite
1999), Wavelength dependence of the optical depth of biomass burning, urban, and desert dust aerosols, J. Geophys. Res., 104(D24), 31333–31349, doi:10.1029/1999JD900923., , , , , , , and (
- Issue published online: 21 SEP 2012
- Article first published online: 21 SEP 2012
- Manuscript Accepted: 18 AUG 1999
- Manuscript Received: 11 MAY 1999
The Angstrom wavelength exponent α, which is the slope of the logarithm of aerosol optical depth (τa) versus the logarithm of wavelength (λ), is commonly used to characterize the wavelength dependence of τa and to provide some basic information on the aerosol size distribution. This parameter is frequently computed from the spectral measurements of both ground-based sunphotometers and from satellite and aircraft remote sensing retrievals. However, spectral variation of α is typically not considered in the analysis and comparison of values from different techniques. We analyze the spectral measurements of τa from 340 to 1020 nm obtained from ground-based Aerosol Robotic Network radiometers located in various locations where either biomass burning, urban, or desert dust aerosols are prevalent. Aerosol size distribution retrievals obtained from combined solar extinction and sky radiance measurements are also utilized in the analysis. These data show that there is significant curvature in the ln τa versus ln λ relationship for aerosol size distributions dominated by accumulation mode aerosols (biomass burning and urban). Mie theory calculations of α for biomass burning smoke (for a case of aged smoke at high optical depth) agree well with observations, confirming that large spectral variations in α are due to the dominance of accumulation mode aerosols. A second order polynomial fit to the ln τa versus ln λ data provides excellent agreement with differences in τa of the order of the uncertainty in the measurements (∼0.01-0.02). The significant curvature in ln τa versus ln λ for high optical depth accumulation mode dominated aerosols results in α values differing by a factor of 3–5 from 340 to 870 nm. We characterize the curvature in ln τa versus ln λ by the second derivative α′ and suggest that this parameter be utilized in conjunction with α to characterize the spectral dependence of τa. The second derivative of ln τa versus ln λ gives an indication of the relative influence of accumulation mode versus coarse mode particles on optical properties.