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Snell’s window in wavy water

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Abstract

The angular diameter of Snell’s window as a function of maximum wave slope is calculated. For flat water the diameter is 97° and increases up to about 122° when the wave slope is about 16°. Steeper waves break and disrupt the smooth surface used in the analysis. Breaking waves produce a window almost 180° wide. The brightness of the dark area around Snell’s window is heavily influenced by turbidity and upwelling radiation, especially in shallow water.

© 2014 Optical Society of America

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Figures (7)

Fig. 1.
Fig. 1. Snell’s window. Note the ragged edges due to waves and the faint blue glow around the window. (Photograph and copyright by Simon Higton.)
Fig. 2.
Fig. 2. Optics of Snell’s window for flat water.
Fig. 3.
Fig. 3. Optical geometry of Snell’s window in the presence of surface waves.
Fig. 4.
Fig. 4. Width of Snell’s window as a function of maximum wave slope.
Fig. 5.
Fig. 5. Snell’s blanket in shallow water surrounding Snell’s window.
Fig. 6.
Fig. 6. Transmission of flat water producing Snell’s window (solid line) and reflectivity of the under surface of water producing Snell’s blanket. The angle from zenith is what an underwater observer would measure.
Fig. 7.
Fig. 7. For steeply inclined wave faces in breaking waves and turbulent, bubble-filled water, skylight can reach an underwater observer from a zenith angle of 90°. Thus skylight can be seen that originates from the entire upper celestial sphere (angular diameter 180°).

Equations (6)

Equations on this page are rendered with MathJax. Learn more.

W=Asin(2πx/λ),
α=tan1(2πA/λ).
httan1(4A/3λ).
R=180°htα.
it=90°htα.
St=α+rt=α+sin1(sin(90°αtan1[2tanα/(3π)])n).
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