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Comparison of global datasets of sodium densities in the mesosphere and lower thermosphere from GOMOS, SCIAMACHY and OSIRIS measurements and WACCM model simulations from 2008 to 2012

机译:从2008年至2012年通过GOMOS,SCIAMACHY和OSIRIS测量以及WACCM模型模拟比较的中层和下层热层全球钠密度数据集的比较

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摘要

During the last decade, several limb sounding satellites havemeasured the global sodium (Na) number densities in the mesosphere and lowerthermosphere (MLT). Datasets are now available from Global OzoneMonitoring by Occultation of Stars (GOMOS), the SCanning Imaging AbsorptionspectroMeter for Atmospheric CHartography (SCIAMACHY) (both on Envisat) andthe Optical Spectrograph and InfraRed Imager System (OSIRIS) (on Odin).Furthermore, global model simulations of the Na layer in the MLT simulated bythe Whole Atmosphere Community Climate Model, including the Na species(WACCM-Na), are available. In this paper, we compare these global datasets.The observed and simulated monthly averages of Na vertical column densities agree reasonably well with each other. They show a clear seasonal cyclewith a summer minimum most pronounced at the poles. They also show signs of a semi-annual oscillation in the equatorial region. The vertical columndensities vary from 0. 5  ×  10 to 7  ×  10 cm near the poles and from 3  ×  10to 4  ×  10 cm at the Equator.The phase of the seasonal cycle and semi-annual oscillation shows small differences between the Na amounts retrieved from different instruments.The full width at half maximum of the profiles is 10 to 16 km for most latitudes, but significantly smaller in the polar summer. The centroidaltitudes of the measured sodium profiles range from 89 to 95 km, whereas the model shows on average 2 to 4 km lower centroid altitudes.This may be explained by the mesopause being 3 km lower in the WACCM simulations than in measurements.Despite this global 2–4 km shift, the model captures well the latitudinal and temporal variations.The variation of the WACCM dataset during the year at different latitudesis similar to the one of the measurements. Furthermore, the differences between the measured profiles with different instruments and thereforedifferent local times (LTs) are also present in the model-simulated profiles.This capturing of latitudinal and temporal variations is also found for the vertical column densities and profile widths.
机译:在过去的十年中,一些肢体探测卫星已经测量了中层和下层热层(MLT)的全球钠(Na)数密度。现在可以从全球星际掩星监测(GOMOS),用于大气作图的SCanning成像吸收光谱仪(SCIAMACHY)(均在Envisat上)和光学光谱仪和红外成像仪系统(OSIRIS)(在Odin上)中获得数据集。由整个大气群落气候模型模拟的MLT中的Na层的碳原子数(包括Na物种(WACCM-Na))是可用的。在本文中,我们比较了这些全局数据集.Na垂直柱密度的观察和模拟月平均值相互之间有相当好的一致性。它们显示出明显的季节周期,极地夏季最明显。它们还显示出赤道区域半年度振荡的迹象。垂直柱密度在两极附近为0. 5×10至7×10 cm,在赤道处为3×10至4×10 cm。大多数纬度的剖面半高全宽为10至16 km,但在极地夏季显着减小。测得的钠剖面的质心高度范围为89至95 km,而该模型显示的质心高度平均低2至4 km,这可能是因为WACCM模拟中的中途停泊高度比测量值低了3 km。该模型每偏移2?4 km,就可以很好地捕获纬度和时间的变化。WACCM数据集在一年中在不同纬度下的变化类似于其中一种测量。此外,使用不同仪器测量的剖面之间的差异以及因此不同的本地时间(LTs)也存在于模型模拟的剖面中。对于垂直列密度和剖面宽度,还可以找到这种对纬度和时间变化的捕获。

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