首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Using CALIPSO to explore the sensitivity to cirrus height in the infrared observations from NPOESS/VIIRS and GOES-R/ABI
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Using CALIPSO to explore the sensitivity to cirrus height in the infrared observations from NPOESS/VIIRS and GOES-R/ABI

机译:在NPOESS / VIIRS和GOES-R / ABI的红外观测中,使用CALIPSO探索对卷云高度的敏感性

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This paper demonstrates how the availability of specific infrared channels impacts the ability of two future meteorological satellite imagers to estimate cloud-top pressure. Both of the imagers are planned for launch by the United States, one for a geostationary platform and the other for a polar-orbiting platform. The geostationary imager, the Advanced Baseline Imager (ABI), will be flown first on the GOES-R platform. In addition to the split window channels at 11 and 12 μm, it has one spectral channel located at 13.3 μm where there is relatively strong absorption of H_2O and CO_2. The polar-orbiting imager, called the Visible/Infrared Imager Radiometer Suite (VIIRS) and flown on the National Polar-Orbiting Environmental satellite Suite (NPOESS), has spectral channels in window regions only. The lack of an absorbing channel on VIIRS is shown to have negative consequences for the inference of cloud-top pressure. This paper investigates the impact on the ability of a satellite imager such as VIIRS to confidently estimate cloud-top pressure due to the absence of infrared absorption channels. The solution space is defined as the depth of the atmospheric layer in which a cloud can be placed where the calculated top-ofatmosphere radiances match the measurements used in the cloud-top pressure retrieval. For optically thin cirrus, the channels used by the operational VIIRS algorithm provide a solution space of over 200 hPa. However, the inclusion of the single CO_2 channel at 13.3 μm on the ABI narrows the solution space to under 30 hPa. Our imager-based analysis is performed using Moderate Resolution Imaging Spectroradiometer (MODIS) data, which provides the relevant channel information with sufficient spatial resolution and radiometric accuracy. Additional results are provided using data from the current GOES and POES imagers. Active lidar data from Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation/Cloud-Aerosol Lidar with Orthogonal Polarization (CALIPSO/CALIOP) observations are used to provide cloud boundaries for verification.
机译:本文演示了特定红外通道的可用性如何影响两个未来的气象卫星成像仪估计云顶压力的能力。两台成像仪均计划在美国发射,一台用于对地静止平台,另一台用于极地轨道平台。对地静止成像仪,即高级基线成像仪(ABI),将首先在GOES-R平台上飞行。除了在11和12μm处有分开的窗口通道外,它还有一个位于13.3μm处的光谱通道,其中H_2O和CO_2的吸收相对较强。称为“可见/红外成像仪辐射计套件”(VIIRS)的极轨成像仪,是在国家极地轨道环境卫星套件(NPOESS)上飞行的,仅在窗口区域具有光谱通道。 VIIRS上缺乏吸收通道对推断云顶压力具有负面影响。本文研究了由于缺少红外吸收通道而对诸如VIIRS之类的卫星成像仪自信地估计云顶压力的能力的影响。解空间定义为可以在其中放置云的大气层的深度,其中计算出的大气顶辐射率与在云顶压力获取中使用的测量值相匹配。对于光学薄卷云,操作VIIRS算法使用的通道可提供超过200 hPa的解空间。但是,在ABI上包含13.3μm的单个CO_2通道会将溶液空间缩小到30 hPa以下。我们的基于成像器的分析是使用中等分辨率成像光谱仪(MODIS)数据执行的,该数据可提供具有足够空间分辨率和辐射精度的相关通道信息。使用来自当前GOES和POES成像仪的数据可提供其他结果。来自云气溶胶激光雷达和红外探路者卫星观测/具有正交极化的云气溶胶激光雷达(CALIPSO / CALIOP)观测的主动激光雷达数据用于提供云边界以进行验证。

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