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悬浮沉积物和聚集体的质量比散射截面:理论极限与应用

Mass-specific scattering cross sections of suspended sediments and aggregates: theoretical limits and applications.

作者信息

Stavn Robert H

机构信息

Department of Biology, P.O. Box 26174, University of North Carolina, Greensboro, NC 27402, USA.

出版信息

Opt Express. 2012 Jan 2;20(1):201-19. doi: 10.1364/OE.20.000201.

Abstract

The spectral mass-specific scattering cross section σPIM is most important for the remote sensing inversion of the concentration of suspended mineral matter in the coastal ocean. This optical parameter is also important in optical theory and therefore the theoretical limits of this parameter are important. There are differing reports in the literature on the magnitude of σPIM and its spectral slope in different coastal ocean systems. To account for and predict these differences, I have applied a model of the size distribution of primary suspended mineral particles and aggregates of these particles to theoretical calculations of σPIM. I utilized a model of mineral particle aggregates by Khelifa and Hill [Khelifa, A. and P.S. Hill, J. Hydraul. Res. 44, 390 (2006)] and Latimer's optical model of aggregates [Latimer, P., Appl. Opt. 24, 3231, (1985)]. I have been able to account for the variations in magnitude and spectral slope of σPIM. This analysis will apply to not only inverting the concentration of suspended mineral matter but also provides the basis for inverting the processes of coagulation and aggregation of primary mineral particles in determining sedimentation rates, budgets, etc.

摘要

光谱质量比散射截面σPIM对于近岸海洋中悬浮矿物质浓度的遥感反演最为重要。这一光学参数在光学理论中也很重要,因此该参数的理论极限很关键。关于不同近岸海洋系统中σPIM的大小及其光谱斜率,文献中有不同的报道。为了解释和预测这些差异,我将初级悬浮矿物颗粒及其聚集体的尺寸分布模型应用于σPIM的理论计算。我采用了Khelifa和Hill [Khelifa, A.和P.S. Hill, J. Hydraul. Res. 44, 390 (2006)]提出的矿物颗粒聚集体模型以及Latimer的聚集体光学模型[Latimer, P., Appl. Opt. 24, 3231, (1985)]。我能够解释σPIM大小和光谱斜率的变化。该分析不仅适用于反演悬浮矿物质的浓度,还为在确定沉降速率、收支等时反演初级矿物颗粒的凝聚和聚集过程提供了基础。

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