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Improving GERB scene identification using SEVIRI: Infrared dust detection strategy

机译:使用SEVIRI改进GERB场景识别:红外粉尘检测策略

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The combination of the Spinning Enhanced Visible and Infrared Imager (SEVIRI) and the Geostationary Earth Radiation Budget (GERB) instruments on Meteosat-8 provides a powerful new tool for detecting aerosols and estimating their radiative effect at high temporal and spatial resolution. However, at present no specific aerosol treatment is performed in the GERB processing chain, severely limiting the use of the data for aerosol studies. A particular problem relates to the misidentification of Saharan dust outbreaks as cloud which can bias the shortwave and longwave fluxes. In this paper an algorithm is developed which employs multiple-linear regression, using information from selected thermal infrared SEVIRI channels, to detect dust aerosol over ocean and provide an estimate of the optical depth at 0.5.5 μm (τ{sub}(055)). To test the performance of the algorithm, it has been applied to a number of dust events observed by SEVIRI during March and June 2004. The results are compared to co-located MODIS observations taken from the Terra and Aqua platforms, and ground based observations from the Cape Verde AERONET site. In terms of detection capability, employing the algorithm results in a notable improvement in the routine GERB scene identification. Locations identified by MODIS as being likely to be dust contaminated were originally classified as cloud in over 99.5% of the cases studied. With the application of the detection algorithm approximately 60-70% of these points are identified as dusty depending on the dust model employed. The algorithm is also capable of detecting dust in regions and at times which would be excluded when using shortwave observations, due for example to the presence of sun-glint, or through the night. We further investigate whether the algorithm is capable of generating useful information concerning the aerosol loading. Comparisons with co-located retrievals from the SEVIRI 0.6 μm solar reflectance band observations show a level of agreement consistent with that expected from the simulations, with rms differences of between 0.5 and 0.8, and a mean bias ranging from -0.5 to 0.3 dependent on the dust representation employed in the algorithm. Temporally resolved comparisons with observations from the Capo Verde AERONET site through the months of March and June reinforce these findings, but also indicate that the algorithm is capable of discerning the diurnal pattern in aerosol loading. The algorithm has now been incorporated within the routine GERB processing in detection mode, and will be used to provide an experimental aerosol product for assessment by the scientific community.
机译:Meteosat-8上的旋转增强型可见光和红外成像仪(SEVIRI)与对地静止地球辐射预算(GERB)仪器的组合提供了一种功能强大的新工具,可用于检测气溶胶并以高时空分辨率估算气溶胶的辐射效应。但是,目前在GERB加工链中没有进行特定的气雾处理,严重限制了气雾研究数据的使用。一个特殊的问题涉及将撒哈拉尘埃暴发误识别为云,这会偏向短波和长波通量。本文开发了一种算法,该算法采用多线性回归,利用来自选定热红外SEVIRI通道的信息,检测海洋上的灰尘气溶胶,并提供0.5.5μm的光学深度估计值(τ{sub}(055) )。为了测试该算法的性能,该算法已应用于SEVIRI在2004年3月至6月期间观测到的许多尘埃事件。将结果与从Terra和Aqua平台获得的同地MODIS观测值以及从佛得角AERONET网站。在检测能力方面,采用该算法可以显着改善常规GERB场景识别。在超过99.5%的案例研究中,MODIS确定的可能被粉尘污染的位置最初被归类为云。通过检测算法的应用,根据所采用的粉尘模型,这些点中约有60-70%被识别为粉尘。该算法还能够检测由于使用短波观测(例如由于有日光照射或整夜)而在某些地区和某些时候被排除的灰尘。我们进一步研究该算法是否能够生成有关气溶胶负荷的有用信息。与SEVIRI 0.6μm太阳反射带观测资料的同地取回资料的比较表明,一致性水平与模拟预期的一致,均方根差在0.5到0.8之间,平均偏差在-0.5到0.3之间,具体取决于算法中采用的粉尘表示。暂时解析的与3月和6月间来自Capo Verde AERONET站点的观察结果进行的比较增强了这些发现,但同时也表明该算法能够识别气溶胶负荷中的昼夜模式。该算法现在已以检测模式并入常规GERB处理中,并将用于提供实验性气溶胶产品,供科学界进行评估。

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