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Atmospheric correction of hyperspectral data over dark surfaces via simulated annealing

机译:通过模拟退火对暗表面的高光谱数据进行大气校正

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A method [atmospheric correction via simulated annealing (ACSA)] is proposed that enhances the atmospheric correction of hyperspectral images over dark surfaces. It is based on the minimization of a smoothness criterion to avoid the assumption of linear variations of the reflectance within gas absorption bands. We first show that this commonly used approach generally fails over dark surfaces when the signal to noise ratio strongly declines. In this case, important residual features highly correlated with the shape of gas absorption bands are observed in the estimated surface reflectance. We add a geometrical constraint to deal with this correlation. A simulated annealing approach is used to solve this constrained optimization problem. The parameters involved in the implementation of the algorithm (initial temperature, number of iterations, cooling schedule, and correlation threshold) are automatically determined by using a standard simulated annealing theory, reflectance databases, and sensor characteristics. Applied to a HyMap image with available ground truths, we verify that ACSA adequately recovers ground reflectance over clear land surfaces, and that the added spectral shape constraint does not introduce any spurious feature in the spectrum. The analysis of an AVIRIS image of Central Switzerland clearly shows the ability of the method to perform enhanced water vapor estimations over dark surfaces. Over a lake (reflectance equal to 0.02, low signal to noise ratio equal to about 6), ACSA retrieves unbiased water vapor amounts (2.86 cm/spl plusmn/0.36 cm) in agreement with in situ measurements (2.97 cm/spl plusmn/0.30 cm). This corresponds to a reduction of the standard deviation by a factor 3 in comparison with standard unconstrained procedures (1.95 cm/spl plusmn/1.08 cm). Similar results are obtained using a Hyperion image of DoE ARM SGP test site containing a very dark area of the land surface.
机译:提出了一种方法[通过模拟退火进行大气校正(ACSA)],该方法可增强暗表面上高光谱图像的大气校正。它基于平滑度准则的最小化,以避免假设气体吸收带内反射率呈线性变化。我们首先显示,当信噪比大幅下降时,这种常用方法通常无法克服黑暗表面。在这种情况下,在估计的表面反射率中观察到与气体吸收带的形状高度相关的重要残留特征。我们添加了几何约束来处理这种相关性。使用模拟退火方法来解决此约束优化问题。通过使用标准的模拟退火理论,反射率数据库和传感器特性,可以自动确定算法实现过程中涉及的参数(初始温度,迭代次数,冷却计划和相关阈值)。将其应用于具有可用地面真实性的HyMap图像后,我们验证了ACSA能够在清晰的陆地表面上充分恢复地面反射率,并且添加的光谱形状约束不会在光谱中引入任何杂散特征。对瑞士中部AVIRIS图像的分析清楚地表明,该方法能够在深色表面上执行增强的水蒸气估算。在一个湖上(反射率等于0.02,低信噪比等于约6),ACSA与原位测量值(2.97 cm / spl plusmn / 0.30)一致,获得了无偏的水蒸气量(2.86 cm / spl plusmn / 0.36 cm)。厘米)。与标准无限制程序(1.95 cm / spl plusmn / 1.08 cm)相比,这相当于将标准偏差减少了3倍。使用DoE ARM SGP测试站点的Hyperion图像(包含陆地表面非常暗的区域)可获得类似的结果。

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