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Using IASI to simulate the total spectrum of outgoing long-wave radiances

机译:使用IASI模拟传出的长波面积的总光谱

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摘要

A new method of deriving high-resolution top-of-atmosphere spectral radiances in 10 181 bands, over the whole outgoing long-wave spectrum of the Earth, is presented. Correlations between different channels measured by the Infrared Atmospheric Sounding Interfermeter (IASI) on the MetOp-A (Meteorological Operation) satellite and unobserved wavenumbers are used to estimate far infrared (FIR) radiances at 0.5 cm(-1) intervals between 25.25 and 644.75 cm(-1) (the FIR), and additionally between 2760 and 3000 cm(-1) (the NIR - near infrared). Radiances simulated by the line-by-line radiative transfer model (LBLRTM) are used to construct the prediction model. The spectrum is validated by comparing the Integrated Nadir Long-wave Radiance (INLR) product spanning the whole 25.25-3000 cm(-1) range with the corresponding broadband measurements from the Clouds and the Earth's Radiant Energy System (CERES) instrument on the Terra and Aqua satellites at points of simultaneous nadir overpass. There is a mean difference of 0.3 W m(-2) sr(-1) (0.5% relative difference). This is well within the uncertainties associated with the measurements made by either instrument. However, there is a noticeable contrast when the bias is separated into night-time and daytime scenes with the latter being significantly larger, possibly due to errors in the CERES Ed3 Spectral Response Functions (SRF) correction method. In the absence of an operational spaceborne instrument that isolates the FIR, this product provides a useful proxy for such measurements within the limits of the regression model it is based on, which is shown to have very low root mean squared errors. The new high-resolution spectrum is presented for global mean clear and all skies where the FIR is shown to contribute 44 and 47% to the total INLR, respectively. In terms of the spectral cloud effect (Cloud Integrated Nadir Long-wave Radiance - CINLR), the FIR contributes 19% and in some subtropical instances appears to be negative; results that would go unobserved with a traditional broadband analysis.
机译:提出了一种在整个外出的地球的传出的长波谱中获得10 181频段高分辨率顶层谱辐射的新方法。由Metop-A(气象操作)卫星和未观察波数的红外大气探测干扰管(IASI)测量的不同通道之间的相关性用于估计在25.25和644.75cm之间的0.5cm(-1)间隔下的远红外(FIR)辐射(-1)(FIR),另外在2760和3000厘米(-1)之间(NIR - 近红外线)。由逐行线路辐射传输模型(LBLRTM)模拟的放射用于构建预测模型。通过将跨越整个25.25-3000cm(-1)范围的集成Nadir长波辐射(InlR)产品与云层的相应宽带测量值进行比较,通过比较整个25.25-3000cm(-1)范围的集成Nadir长波辐射(InlR)产品进行验证。和Aqua Satellites在同时Nadir立交桥。平均差异为0.3W m(-2)sr(-1)(相对差异0.5%)。这在与任何一种仪器进行的测量相关的不确定性内。然而,当偏差被分离成夜间和日间场景时,存在明显的对比度,其中后者显着更大,可能是由于CETES ED3光谱响应函数(SRF)校正方法中的错误。在没有隔离FIR的操作太乐器的情况下,该产品在基于回归模型的限制范围内提供了有用的代理,其是基于的,这被示出具有非常低的根均匀的误差。新的高分辨率频谱呈现出全球平均透明,并且所有Skies都分别显示了FIR的贡献44%和47%。就光谱云效应而言(云集成Nadir长波光线 - CinlR),FIR贡献19%,在一些亚热带实例中似乎是负的;结果将通过传统的宽带分析进行不受欢迎。

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