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4SM: A Novel Self-Calibrated Algebraic Ratio Method for Satellite-Derived Bathymetry and Water Column Correction

机译:4SM:一种用于卫星测深和水柱校正的新型自校准代数比方法

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摘要

All empirical water column correction methods have consistently been reported to require existing depth sounding data for the purpose of calibrating a simple depth retrieval model; they yield poor results over very bright or very dark bottoms. In contrast, we set out to (i) use only the relative radiance data in the image along with published data, and several new assumptions; (ii) in order to specify and operate the simplified radiative transfer equation (RTE); (iii) for the purpose of retrieving both the satellite derived bathymetry (SDB) and the water column corrected spectral reflectance over shallow seabeds. Sea truth regressions show that SDB depths retrieved by the method only need tide correction. Therefore it shall be demonstrated that, under such new assumptions, there is no need for (i) formal atmospheric correction; (ii) conversion of relative radiance into calibrated reflectance; or (iii) existing depth sounding data, to specify the simplified RTE and produce both SDB and spectral water column corrected radiance ready for bottom typing. Moreover, the use of the panchromatic band for that purpose is introduced. Altogether, we named this process the Self-Calibrated Supervised Spectral Shallow-sea Modeler (4SM). This approach requires a trained practitioner, though, to produce its results within hours of downloading the raw image. The ideal raw image should be a “near-nadir” view, exhibit homogeneous atmosphere and water column, include some coverage of optically deep waters and bare land, and lend itself to quality removal of haze, atmospheric adjacency effect, and sun/sky glint.
机译:一致地报告了所有经验性水柱校正方法都需要现有的测深数据,以用于校准简单的深度取回模型。在非常明亮或非常黑暗的底部,它们产生的效果很差。相反,我们着手(i)仅使用图像中的相对辐射数据以及已发布的数据以及一些新的假设; (ii)为了规定和运行简化的辐射传递方程(RTE); (iii)为检索卫星衍生的测深法(SDB)和水柱校正的浅海底光谱反射率。海洋真相回归表明,通过该方法获得的SDB深度仅需进行潮汐校正。因此,应证明,在这种新假设下,不需要(i)正式的大气校正; (ii)将相对辐射度转换为校准反射率;或(iii)现有的深度探测数据,以指定简化的RTE,并产生SDB和光谱水柱校正的辐射度,以备底部打字。此外,为此目的引入了全色带的使用。总体而言,我们将此过程命名为“自校正监督光谱浅海建模器(4SM)”。但是,这种方法需要训练有素的从业人员在下载原始图像后的数小时内产生其结果。理想的原始图像应为“近天底”视图,并显示均匀的大气层和水柱,覆盖一些光学上深水和裸露的土地,并有助于去除雾度,大气邻接效应和太阳/天空闪烁。

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