Salama Mhd Suhyb, Stein Alfred
International Institute for Geo-Information Science and Earth Observation, ITC Hengelosestraat 99, 7500 AA Enschede, The Netherlands.
Appl Opt. 2009 Sep 10;48(26):4947-62. doi: 10.1364/AO.48.004947.
We describe a methodology to quantify and separate the errors of inherent optical properties (IOPs) derived from ocean-color model inversion. Their total error is decomposed into three different sources, namely, model approximations and inversion, sensor noise, and atmospheric correction. Prior information on plausible ranges of observation, sensor noise, and inversion goodness-of-fit are employed to derive the posterior probability distribution of the IOPs. The relative contribution of each error component to the total error budget of the IOPs, all being of stochastic nature, is then quantified. The method is validated with the International Ocean Colour Coordinating Group (IOCCG) data set and the NASA bio-Optical Marine Algorithm Data set (NOMAD). The derived errors are close to the known values with correlation coefficients of 60-90% and 67-90% for IOCCG and NOMAD data sets, respectively. Model-induced errors inherent to the derived IOPs are between 10% and 57% of the total error, whereas atmospheric-induced errors are in general above 43% and up to 90% for both data sets. The proposed method is applied to synthesized and in situ measured populations of IOPs. The mean relative errors of the derived values are between 2% and 20%. A specific error table to the Medium Resolution Imaging Spectrometer (MERIS) sensor is constructed. It serves as a benchmark to evaluate the performance of the atmospheric correction method and to compute atmospheric-induced errors. Our method has a better performance and is more appropriate to estimate actual errors of ocean-color derived products than the previously suggested methods. Moreover, it is generic and can be applied to quantify the error of any derived biogeophysical parameter regardless of the used derivation.
我们描述了一种方法,用于量化和分离从海洋颜色模型反演得出的固有光学特性(IOPs)的误差。其总误差被分解为三个不同来源,即模型近似和反演、传感器噪声以及大气校正。利用关于观测的合理范围、传感器噪声和反演拟合优度的先验信息来推导IOPs的后验概率分布。然后量化每个误差分量对IOPs总误差预算的相对贡献,所有这些贡献均具有随机性。该方法通过国际海洋颜色协调小组(IOCCG)数据集和美国国家航空航天局生物光学海洋算法数据集(NOMAD)进行了验证。对于IOCCG和NOMAD数据集,推导得出的误差分别与已知值接近,相关系数分别为60 - 90%和67 - 90%。推导得出的IOPs中模型引起的误差占总误差的10%至57%,而对于这两个数据集,大气引起的误差通常高于43%,最高可达90%。所提出的方法应用于合成的和现场测量的IOPs群体。推导值的平均相对误差在2%至20%之间。构建了针对中分辨率成像光谱仪(MERIS)传感器的特定误差表。它作为评估大气校正方法性能和计算大气引起误差的基准。与先前提出的方法相比,我们的方法具有更好的性能,更适合估计海洋颜色衍生产品的实际误差。此外,它具有通用性,可应用于量化任何衍生生物地球物理参数的误差,而不论所使用的推导方法如何。