利用AVHRR中波红外波段估算海表温度

Jennifer C. Davis, Jerry X. Tu, Sean P. Byme James, Lisowski, SciTec
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引用次数: 0

摘要

我们描述了一种利用AVHRR极地轨道器的MWIR波段数据估计海表温度(SST)的方法。目前,海温的计算通常采用分窗非线性多通道算法,结合AVHRR通道4和5的数据(分别为10.3-11.3和11.5-12.5 /spl mu/m)。这些结果的准确性在一定程度上取决于区域变化,并受到测量的空间分辨率的固有限制。然而,这些海温图通常被认为是可靠的,并被广泛用于研究洋流及其对天气模式的影响。然而,我们感兴趣的是,在没有LWIR测量的情况下,测试使用MWIR数据在夜间(当反射太阳辐射不是问题时)和白天(当反射太阳辐射是问题时)估计海温的可行性。例如,我们讨论的这种MWIR SST算法将使用来自没有LWIR能力的卫星的数据来计算辅助卫星任务的参数(但这仍然是非常有趣的)。我们描述的海表温度算法是基于MODTRAN在不同表面温度下的海洋辐射值,并在上述AVHRR波段上计算,与这些波段中收集的像素值进行比较。这些MODTRAN计算是特定场景的,因为视角和大气条件是重要的输入参数。因此,MODTRAN是从主要的SST程序体系结构中启动的,适用于一系列不同的温度。然而,这种计算的结果可以作为lza网格、标准大气和温度的查找表来实现。在评估像素的温度之前,必须对场景进行云层筛选,这往往会降低对污染像素的温度估计。我们使用CloudDI算法完成这种筛选,这是一种改进的最小二乘模板匹配方法。最后,我们针对AVHRR SST算法以及可用的地面真值测试了我们结果的有效性。由于MODTRAN计算需要传感器的几何形状和大气条件作为输入参数,理论上,在某些情况下,有可能校正高水汽水平对海表温度结果的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Estimation of sea surface temperature using the AVHRR mid-wave IR band
We describe a method for estimating sea surface temperature (SST) using MWIR band data from the AVHRR polar orbiter. Currently, SST is routinely calculated with a split-window, nonlinear multichannel algorithm incorporating data from AVHRR Channels 4 and 5 (10.3-11.3 and 11.5-12.5 /spl mu/m, respectively). The accuracy of these results is dependent to a certain degree upon regional variations and is inherently limited by the spatial resolution of the measurements. Nevertheless, these SST maps are generally considered reliable, and are widely used for studying ocean currents and their effect on weather patterns. We are interested, however, in testing the feasibility of using MWIR data in the absence of LWIR measurements for estimating SST both at night, when reflected solar radiance is not an issue, as well as during the day, when it is. A MWIR SST algorithm of the type we discuss would be using data, for example, from a satellite without LWIR capabilities in order to calculate a parameter that is ancillary to the satellite mission (but which is nevertheless of high interest). The SST algorithms we describe are based upon the comparison of MODTRAN ocean radiance values, at a variety of surface temperatures and calculated over the aforementioned AVHRR bands, to the values of the collected pixels in these bands. These MODTRAN calculations are scene-specific, as viewing angle and atmospheric conditions are important input parameters. MODTRAN is therefore launched from within the main SST program architecture for a range of different temperatures. The results of such calculations could conceivably be implemented, however, as a look-up table for a grid of LZAs, standard atmospheres and temperatures. Before the temperature of the pixels can be assessed, the scene must be screened for clouds, which tend to lower the temperature estimation for contaminated pixels. We accomplish this screening using our CloudDI algorithm, a modified least squares template-matching approach. Finally, we test the validity of our results against the AVHRR SST algorithms as well as against available ground truth. Since the MODTRAN calculations require sensor geometry and atmospheric conditions as input parameters, it is possible, in theory, to correct for the effect of high levels of water vapor on the SST results in certain situations.
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