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Tropospheric phase delay in interferometric synthetic aperture radar estimated from meteorological model and multispectral imagery

机译:气象模型和多光谱成像估计的干涉式合成孔径雷达对流层相位延迟

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摘要

ENVISAT Medium Resolution Imaging Spectrometer Instrument (MERIS) multispectral data and the mesoscale meteorological model MM5 are used to estimate the tropospheric phase delay in synthetic aperture radar (SAR) interferograms. MERIS images acquired simultaneously with ENVISAT Advanced Synthetic Aperture Radar data provide an estimate of the total water vapor content W limited to cloud-free areas based on spectral bands ratio (accuracy 0.17 g cm^(−2) and ground resolution 300 m). Maps of atmospheric delay, 2 km in ground resolution, are simulated from MM5. A priori pertinent cumulus parameterization and planetary boundary layer options of MM5 yield near-equal phase correction efficiency. Atmospheric delay derived from MM5 is merged with available MERIS W product. Estimates of W measured from MERIS and modeled from MM5 are shown to be consistent and unbiased and differ by ~0.2 g cm^(−2) (RMS). We test the approach on data over the Lebanese ranges where active tectonics might contribute to a measurable SAR signal that is obscured by atmospheric effects. Local low-amplitude (1 rad) atmospheric oscillations with a 2.25 km wavelength on the interferograms are recovered from MERIS with an accuracy of 0.44 rad or 0.03 g cm^(−2). MERIS water product overestimates W in the clouds shadow due to mismodeling of multiple scattering and underestimates W on pixels with undetected semitransparent clouds. The proposed atmospheric filter models dynamic atmospheric signal which cannot be recovered by previous filtering techniques which are based on a static atmospheric correction. Analysis of filter efficiency with spatial wavelength shows that ~43% of the atmospheric signal is removed at all wavelengths.
机译:ENVISAT中分辨率成像光谱仪仪器(MERIS)的多光谱数据和中尺度气象模型MM5用于估计合成孔径雷达(SAR)干涉图中的对流层相位延迟。与ENVISAT Advanced Synthetic Aperture Radar数据同时获取的MERIS图像基于谱带比率(精度为0.17 g cm ^(-2)和地面分辨率为300 m)提供了仅限于无云区域的总水汽含量W的估计值。 MM5模拟了地面分辨率为2 km的大气延迟图。 MM5的先验相关累积参数化和行星边界层选项可产生几乎相等的相位校正效率。源自MM5的大气延迟与可用的MERIS W产品合并。由MERIS测量并根据MM5建模的W的估计值是一致且无偏的,相差〜0.2 g cm ^(-2)(RMS)。我们在黎巴嫩范围内的数据上测试了这种方法,在这种情况下,活跃的构造可能会产生可测量的SAR信号,而该信号会被大气影响遮盖。从干涉仪上以0.44 rad或0.03 g cm ^(-2)的精度从干涉仪上恢复了干涉图上波长为2.25 km的局部低振幅(1 rad)大气振荡。由于多重散射的模型错误,MERIS水产品高估了云层阴影中的W,而低估了具有未检测到的半透明云层的像素上的W。所提出的大气滤波器模拟动态大气信号,该信号不能通过基于静态大气校正的先前滤波技术来恢复。对空间波长的滤波器效率的分析表明,在所有波长下,约43%的大气信号都被去除了。

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