L. W. Carrier, G. A. Cato, and K. J. von Essen, "The Backscattering and Extinction of Visible and Infrared Radiation by Selected Major Cloud Models," Appl. Opt. 6, 1209-1216 (1967)
Volume backscattering functions and optical extinction coefficients are computed for eight suggested major cloud models using the Mie theory for optical wavelengths of 0.488 μ, 0.694 μ, 1.06 μ, 4.0 μ, and 10.6 μ. Results show that there is no clear advantage of one wavelength over another for improving cloud transmission; however, backscattering is significantly reduced at the longer wavelengths. Variations in the optical properties of clouds are also discussed and calculations summarized to indicate the effects of cloud thickness, inhomogeneity, and geographical location on the backscatter function and extinction coefficient.
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Na = total concentration. rmode = mode radius ≡ radius corresponding to the maximum number of droplets, rmin = minimum radius. rmax = maximum radius.
Δr = bandwidth of the drop-size distribution at half-value points. μ = microns.
Table II
Summary of the Backscattering Functions and Extinction Coefficients of the Major Cloud Types
Calculations based on droplet spectrum reported by Durbin9 in September 1951.
Somewhat similar physical properties to cumulus congestus, where β(π) = 3.66 × 10−3 m−1sr−1 and b = 7.13 × 10−2m−1.
Stratus cloud physical properties after Singleton and Smith.22
Cumulus cloud physical properties after Khrgran.23
Note 1: Stratus size distribution (1975–2130 m) cutoff at 25 μ.
Note 2: Stratus size distribution (1975–2130 m) cutoff at low end.
Na = total concentration. rmode = mode radius ≡ radius corresponding to the maximum number of droplets, rmin = minimum radius. rmax = maximum radius.
Δr = bandwidth of the drop-size distribution at half-value points. μ = microns.
Table II
Summary of the Backscattering Functions and Extinction Coefficients of the Major Cloud Types
Calculations based on droplet spectrum reported by Durbin9 in September 1951.
Somewhat similar physical properties to cumulus congestus, where β(π) = 3.66 × 10−3 m−1sr−1 and b = 7.13 × 10−2m−1.
Stratus cloud physical properties after Singleton and Smith.22
Cumulus cloud physical properties after Khrgran.23
Note 1: Stratus size distribution (1975–2130 m) cutoff at 25 μ.
Note 2: Stratus size distribution (1975–2130 m) cutoff at low end.