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归一化离水辐亮度:重新审视表面粗糙度的影响。

Normalized water-leaving radiance: revisiting the influence of surface roughness.

作者信息

Gordon Howard R

机构信息

Department of Physics, University of Miami, Coral Gables, Florida 33124, USA.

出版信息

Appl Opt. 2005 Jan 10;44(2):241-8. doi: 10.1364/ao.44.000241.

Abstract

Many spaceborne sensors have been deployed to image the ocean in the visible portion of the spectrum. Information regarding the concentration of water constituents is contained in the water-leaving radiance-the radiance that is backscattered out of the water and subsequently propagates to the top of the atmosphere. Recognizing that it depends on the viewing and Sun geometry, ways have been sought to normalize this radiance to a single Sun-viewing geometry--forming the normalized water-leaving radiance. This requires understanding both the bidirectional nature of the upwelling radiance just beneath the surface and the interaction of this radiance with the air-water interface. I believe that the latter has been incorrectly computed in the past when a water surface roughened by the wind is considered. The presented computation suggests that, for wind speeds as high as 20 m/s, the influence of surface roughness is small for a wide range of Sun-viewing geometries, i.e., the transmittance of the (whitecap-free) air-water interface is nearly identical (within 0.01) to that for a flat interface.

摘要

许多星载传感器已被部署用于对海洋光谱的可见光部分进行成像。有关水体成分浓度的信息包含在离水辐射率中,即从水中反向散射并随后传播到大气顶层的辐射率。由于认识到它取决于观测和太阳几何条件,人们一直在寻求将这种辐射率归一化到单一太阳观测几何条件的方法,即形成归一化离水辐射率。这需要理解表面下方向上辐射的双向特性以及这种辐射与气 - 水界面的相互作用。我认为,过去在考虑因风而变得粗糙的水面时,后者的计算是错误的。给出的计算表明,对于高达20米/秒的风速,在广泛的太阳观测几何条件范围内,表面粗糙度的影响很小,即(无白帽)气 - 水界面的透过率与平坦界面的透过率几乎相同(在0.01以内)。

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