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Progressive Atmospheric Correction of Satellite Ocean-Color Imagery

机译:卫星海洋颜色图像的逐步大气修正

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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:提出了一种方法来校正卫星海洋颜色图像,用于逐渐为大气和表面的扰动效果,从近红外线开始,从近红外线推进到可见光。首先,在近红外选择一组光谱带,除了一个光谱带之外,可以认为水体可以被认为是黑色的。在分子散射和太阳闪烁贡献的校正后,选择的带中的大气层反射率是线性的,以检索水体不是黑色的光谱带中的海洋信号。线性组合的系数最小化了扰动效果,这是由于气溶胶的散射和吸收,以及表面的反射。这些效果被分解为模拟中的主要成分。其次,选择其他频谱频带,逐渐包括较短波长。在每个步骤中,只有一个光谱带中的海洋信号是未知的,因此估计。该方法是为海面观看宽视野传感器(SeaWIFS)开发的,但通常适用于在可见和近红外测量的海洋传感器。然而,在没有测量的情况下,大气校正仅适用于案例-1水。从辐射转移模拟评估理论性能,用于广泛的地球物理和角度条件,包括吸收气溶胶。只有在模拟中考虑了案例-1水域。除了当气溶胶载荷大之外,大气和表面的扰动对大气和表面的影响最小化。线性组合中的残余效果表现出偏大的幅度增加,随气溶胶光学厚度增加。通过考虑在主组件中的分解的所有特征向量,不仅是最重要的偏见,偏差可以减少。估计的海洋信号中的误差随着减小的波长(较长波长的剩余效果传播)和增加气溶胶光学厚度。当550nm的气溶胶光学厚度高于0.3时,它们变得不可接受。通过优化所选波长组或通过使用从卫星数据估计的气溶胶光学厚度来改善性能。

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