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Asymptotic light field in the presence of a bubble-layer

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Abstract

We report that the submerged microbubbles are an efficient source of diffuse radiance and may contribute to a rapid transition to the diffuse asymptotic regime. In this asymptotic regime an average cosine is easily predictable and measurable.

©1999 Optical Society of America

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Figures (3)

Fig. 1.
Fig. 1. Bubble-stratus layer generated by breaking waves. Bubble population is continually replenished by wave activity (breaking waves at the surface) leading eventually to semi-homogeneous layer.
Fig. 2.
Fig. 2. Average cosine for downwelling radiation µ ¯ d (z) for (1) “infinitely” deep homogeneous ocean composed of CDOM, pure water, and particulates corresponding to chl=10mgm-3 (triangles); (2) “infinitely” deep homogeneous ocean with bubbles (cubes); (3) two-layer system composed of background CDOM, water, and particulates and 2m layer of submerged bubbles close to the surface (circles).
Fig. 3.
Fig. 3. Same as 2 but for the average cosine µ ¯ (z).
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