profiles of optical Extinction Coefficients Calculated from Droplet Spectra Observed in Marine Stratus Cloud Layers

V. Ray Noonkester Ocean and Atmospheric Sciences Division, Naval Ocean Systems Center, San Diego, CA 92152

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Abstract

Airborne measurements of droplet spectra n(r) where r is droplet radius were made in stratus cloud layers over the ocean 130 km southwest of San Diego. Optical extinction coefficients σe were calculated at selected wavelengths (λ= 0.53, 3.75 and 10.59 μm) from these n(r) and were used to construct average vertical profiles of σe between 200 m above cloud base to 250 m below cloud base. An approximation to σe a power function of the liquid water content w was found to be superior compared with approximations involving linear functions of w or the cross-section area. The horizontal variability of σe in the clouds was examined. The average horizontal scale size of σe was estimated to be 3 km and the horizontal measuring distance required to obtain values of σe with a relative accuracy of 10% was found to be in excess of 30 km.

Abstract

Airborne measurements of droplet spectra n(r) where r is droplet radius were made in stratus cloud layers over the ocean 130 km southwest of San Diego. Optical extinction coefficients σe were calculated at selected wavelengths (λ= 0.53, 3.75 and 10.59 μm) from these n(r) and were used to construct average vertical profiles of σe between 200 m above cloud base to 250 m below cloud base. An approximation to σe a power function of the liquid water content w was found to be superior compared with approximations involving linear functions of w or the cross-section area. The horizontal variability of σe in the clouds was examined. The average horizontal scale size of σe was estimated to be 3 km and the horizontal measuring distance required to obtain values of σe with a relative accuracy of 10% was found to be in excess of 30 km.

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