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首页> 外文期刊>Remote Sensing of Environment: An Interdisciplinary Journal >Sea surface temperature from a geostationary satellite by optimal estimation
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Sea surface temperature from a geostationary satellite by optimal estimation

机译:对地静止卫星海面温度的最佳估计

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Optimal estimation (OE) is applied as a technique for retrieving sea surface temperature (SST) from thermal imagery obtained by the Spinning Enhanced Visible and Infra-Red Imager (SEVIRI) on Meteosat 9. OE requires simulation of observations as part of the retrieval process, and this is done here using numerical weather prediction fields and a fast radiative transfer model. Bias correction of the simulated brightness temperatures (BTs) is found to be a necessary step before retrieval, and is achieved by filtered averaging of simulations minus observations over a time period of 20 days and spatial scale of 2.5 degrees in latitude and longitude. Throughout this study, BT observations are clear-sky averages over cells of size 0.5 degrees in latitude and longitude. Results for the OE SST are compared to results using a traditional non-linear retrieval algorithm ("NLSST"), both validated against a set of 30108 night-time matches with drifting buoy observations. For the OE SST the mean difference with respect to drifter SSTs is -0.01 K and the standard deviation is 0.47 K, compared to -0.38 K and 0.70 K respectively for the NLSST algorithm. Perhaps more importantly, systematic biases in NLSST with respect to geographical location, atmospheric water vapour and satellite zenith angle are greatly reduced for the OE SST. However, the OE SST is calculated to have a lower sensitivity of retrieved SST to true SST variations than the NLSST, This feature would be a disadvantage for observing SST fronts and diurnal variability, and raises questions as to how best to exploit OE techniques at SEVIRI's full spatial resolution.
机译:最佳估计(OE)用作从通过Meteosat 9上的自旋增强型可见光和红外成像仪(SEVIRI)获得的热图像中检索海表温度(SST)的技术。OE需要将观察结果模拟为检索过程的一部分。 ,这是使用数值天气预报字段和快速辐射传递模型完成的。发现对模拟亮度温度(BTs)的偏差校正是检索之前的必要步骤,并且可以通过对20天的时间段以及经度和纬度为2.5度的空间比例的模拟减去观测值进行滤波平均来实现。在整个研究中,BT观测值是经度和纬度大小为0.5度的像元上晴空的平均值。将OE SST的结果与使用传统的非线性检索算法(“ NLSST”)的结果进行比较,两者均针对一组30108夜间匹配并通过浮标观测进行了验证。对于OE SST,相对于漂移SST的平均差为-0.01 K,标准偏差为0.47 K,而NLSST算法分别为-0.38 K和0.70K。也许更重要的是,对于OE SST,NLSST在地理位置,大气水汽和卫星天顶角方面的系统性偏差已大大减少。但是,OE SST计算得出的SST对真实SST变异的敏感性比NLSST低。此功能对于观察SST前沿和日变化是不利的,并提出了如何在SEVIRI's最佳利用OE技术的问题。完整的空间分辨率。

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