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Progressive Atmospheric Correction of Satellite Ocean-Color Imagery

机译:卫星海洋彩色图像的渐进大气校正

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摘要

A methodology is proposed to correct satellite ocean-color imagery for the perturbing effects of the atmosphere and surface progressively, starting from the near infrared and advancing to the visible. First, a set of spectral bands is selected in the near infrared, for which the water body can be considered black, except in one of the spectral bands. The top-of-atmosphere reflectance in the selected bands, after correction for molecular scattering and sun glint contributions, is linearly combined to retrieve the ocean signal in the spectral band where the water body is not black. The coefficients of the linear combination minimize the perturbing effects, which are due to scattering and absorption by aerosols, and reflection by the surface. These effects are decomposed into principal components in the modeling. Second, other sets of spectral bands are selected, that progressively include shorter wavelengths. At each step, only the marine signal in one spectral band is unknown and therefore estimated. The methodology is developed for the Sea-viewing Wide Field-of-view Sensor (SeaWiFS), but is generally applicable to ocean-color sensors that measure in the visible and near infrared. Without measurements above one micrometer, however, the atmospheric correction is only accurate over Case-1 waters. Theoretical performance is evaluated from radiation-transfer simulations for a wide range of geophysical and angular conditions, including absorbing aerosols. Only Case-1 waters are considered in the simulations. The perturbing influence of the atmosphere and surface is minimized adequately for each set of wavelengths, except when the aerosol loading is large. The residual effects in the linear combination exhibit a bias of magnitude increasing with aerosol optical thickness. The bias can be reduced globally, by taking into account all the eigenvectors of the decomposition in principal components, not only the most significant ones. Errors in the estimated marine signal increase with decreasing wavelength (the residual effects at longer wavelengths propagate) and with increasing aerosol optical thickness. They become unacceptable when the aerosol optical thickness at 550 nm is above 0.3. Performance can be improved by optimizing the sets of selected wavelengths, or by using aerosol optical thickness estimated from the satellite data.
机译:提出了一种方法,从近红外开始,逐步推进到可见光,以逐步纠正卫星海洋彩色图像对大气和地表的干扰作用。首先,在近红外中选择一组光谱带,对于其中的水体,除了其中一个光谱带之外,可以将其视为黑色。在对分子散射和太阳闪烁影响进行校正之后,将选定波段中的最高大气反射率线性组合,以检索水体不为黑色的光谱带中的海洋信号。线性组合的系数使扰动效应最小化,这是由于气溶胶的散射和吸收以及表面的反射造成的。这些影响在模型中分解为主要成分。其次,选择其他组的光谱带,它们逐渐包括较短的波长。在每一步骤中,只有一个光谱带中的海洋信号是未知的,因此需要进行估计。该方法是为海景宽视野传感器(SeaWiFS)开发的,但通常适用于在可见光和近红外光中进行测量的海洋颜色传感器。但是,如果没有超过1微米的测量值,则大气校正仅在Case-1水域上才是准确的。通过辐射传输模拟对各种地球物理和角度条件(包括吸收气溶胶)的理论性能进行了评估。在模拟中仅考虑Case-1水。对于每组波长,大气和表面的扰动影响都应最小化,除非气溶胶负载量很大。线性组合中的残余效应显示出随着气溶胶光学厚度的增加而增加的幅度偏差。通过考虑主成分分解的所有本征向量,不仅是最重要的本征向量,可以整体降低偏差。估计的海洋信号中的误差随着波长的减小(在更长波长处的残留效应传播)和气溶胶光学厚度的增加而增加。当550nm处的气溶胶光学厚度大于0.3时,它们变得不可接受。通过优化所选波长集或使用根据卫星数据估算的气溶胶光学厚度,可以提高性能。

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