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首页> 外文期刊>Applied optics >VALIDATION OF FASCOD3 AND MODTRAN3 - COMPARISON OF MODEL CALCULATIONS WITH GROUND-BASED AND AIRBORNE INTERFEROMETER OBSERVATIONS UNDER CLEAR-SKY CONDITIONS
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VALIDATION OF FASCOD3 AND MODTRAN3 - COMPARISON OF MODEL CALCULATIONS WITH GROUND-BASED AND AIRBORNE INTERFEROMETER OBSERVATIONS UNDER CLEAR-SKY CONDITIONS

机译:清晰条件下FASCOD3和MODTRAN3的验证-与基于地面和机载干涉仪观测的模型计算的比较

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摘要

The validation of FASCOD3 and MODTRAN3 against Ground-based and airborne high-resolution Michelson interferometer measurements under clear-sky conditions is presented. Important considerations including water vapor continuum; frequency-dependent sea surface emissivity in the IR window region, and spectral resolution of MODTRAN3 in the comparison of model calculations with high-resolution interferometer measurements are discussed. Our results indicate that it is not adequate to assume sea surface emissivity of 1.0 [epsilon(nu) = 1.0] or a constant in the simulation of upwelling radiance observed by the airborne Michelson interferometer. The use of spectral emissivity (frequency-dependent emissivity) leads to much better agreement between model calculations and interferometer measurements in the IR window region from 750.0 to 1050.0 cm(-1). This could have important implications for the retrieval of sea surface temperature, thin cirrus properties, and aerosol parameters because of the sea surface emissivity of 1.0 assumption commonly used by many researchers. Comparisons of MODTRAN3 calculations with interferometer measurements show that the agreement might not be adequate at the nominal resolution of 2.0 cm(-1), and further spectral degradation might be necessary to improve the agreement between measurements and MODTRAN3 calculations. MODTRAN should be used with caution for relatively high spectral resolution remote-sensing applications. (C) 1996 Optical Society of America [References: 22]
机译:提出了FASCOD3和MODTRAN3在晴空条件下针对地面和机载高分辨率迈克尔逊干涉仪测量的验证。重要考虑因素,包括水蒸气连续性;讨论了红外窗口区域中与频率有关的海面发射率,以及在模型计算与高分辨率干涉仪测量结果的比较中,MODTRAN3的光谱分辨率。我们的结果表明,在机载迈克尔逊干涉仪观测到的上升流辐射的模拟中,不足以假设海面发射率为1.0 [ε(nu)= 1.0]或一个常数。光谱发射率(与频率有关的发射率)的使用可在红外窗口范围从750.0到1050.0 cm(-1)的模型计算和干涉仪测量之间达成更好的一致性。这可能对海面温度,薄卷云特性和气溶胶参数的检索具有重要意义,因为许多研究人员通常使用1.0假设的海面发射率。 MODTRAN3计算与干涉仪测量结果的比较表明,在标称分辨率为2.0 cm(-1)时,该协议可能不足够,并且可能需要进一步的光谱衰减以改善测量与MODTRAN3计算之间的协议。对于相对高光谱分辨率的遥感应用,应谨慎使用MODTRAN。 (C)1996年美国眼镜学会[参考文献:22]

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