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13 December 2018 Characteristic geometric features of the sun glint on the sea surface for satellite optical measurements
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Proceedings Volume 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 108334J (2018) https://doi.org/10.1117/12.2504235
Event: XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2018, Tomsk, Russian Federation
Abstract
On the base of the top-of-atmosphere radiance calculations carried out with the use of an isotropic version of the CoxMunk model of sea surface slopes distribution and the Sobolev model of light scattering in the atmosphere, the sun glint quantitative characteristics such as its length, maximal width and maximal contrast are presented for measurements of scanning satellite instruments in the visible and near-infrared ranges from 0.4 to 1.6 μm for sea wind speeds from 2 to 14 m/s and atmospheric aerosol optical thicknesses from 0.03 to 0.33.
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Nick E. Lebedev and Alexander S. Zapevalov "Characteristic geometric features of the sun glint on the sea surface for satellite optical measurements", Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 108334J (13 December 2018); https://doi.org/10.1117/12.2504235
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