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Practical methods for rapid and accurate computation of interferometric spectra for remote sensing applications

机译:用于遥感应用的快速准确计算干涉光谱的实用方法

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摘要

The apodization of an interferogram corresponds to a linear transformation in spectral space between unapodized and apodized radiances. Many apodization functions have well-behaved numerical inverse transformations, and we show an analytic inverse for the Hamming apodization function. The inverse transformation has many practical uses for remote sensing applications and can also be used theoretically to show the equivalence between unapodized spectra and properly apodized spectra. The inverse transformation, which is a representation of the discrete convolution theorem, can be used to readily convert computed apodized spectra to spectra computed for other symmetric apodization functions (including unapodized), which may have poorer characteristics with regard to calculating channel-transmittance parameters or radiances. We also show a quantitative method for comparing apodization functions of different mathematical forms.
机译:干涉图的变迹对应于未变迹和变迹的辐射之间的光谱空间中的线性变换。许多切趾函数具有良好的数值逆变换,我们为汉明切趾函数显示了解析逆。逆变换在遥感应用中有许多实际用途,并且在理论上也可以用于显示未切趾的光谱和适当切趾的光谱之间的等价关系。逆变换是离散卷积定理的表示,可以用于将计算的变迹光谱容易地转换为针对其他对称变迹函数(包括未变迹)的光谱,这些对称变径在计算通道透射率参数或光辉。我们还展示了一种定量方法,用于比较不同数学形式的切趾函数。

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