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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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During the last decade, several limb sounding satellites have measured the global sodium (Na) number densities in the mesosphere and lower thermosphere (MLT). Datasets are now available from Global Ozone Monitoring by Occultation of Stars (GOMOS), the SCanning Imaging Absorption spectroMeter for Atmospheric CHartography (SCIAMACHY) (both on Envisat) and the Optical Spectrograph and InfraRed Imager System (OSIRIS) (on Odin). Furthermore, global model simulations of the Na layer in the MLT simulated by the Whole Atmosphere Community Climate Model, including the Na species (WACCM-Na), are available. In this paper, we compare these global datasets.brbrThe observed and simulated monthly averages of Na vertical column densities agree reasonably well with each other. They show a clear seasonal cycle with a summer minimum most pronounced at the poles. They also show signs of a semi-annual oscillation in the equatorial region. The vertical column densities vary from 0.?5??×??10sup9/sup to 7??×??10sup9/sup?cmsup?2/sup near the poles and from 3??×??10sup9/sup to 4??×??10sup9/sup?cmsup?2/sup 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 centroid altitudes 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 latitudes is similar to the one of the measurements. Furthermore, the differences between the measured profiles with different instruments and therefore different 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热层(MLT)的全球钠(Na)数密度。现在可以从全球星际掩星监测臭氧(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)获得数据集。此外,还提供了由整个大气群落气候模型模拟的MLT中Na层的全球模型模拟,包括Na物种(WACCM-Na)。在本文中,我们比较了这些全局数据集。 Na垂直柱密度的观测和模拟月平均值彼此之间有相当好的一致性。它们显示了一个清晰的季节周期,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。垂直列密度从0.?5??×??10 9 到7 ??×?? 10 9 ?cm ?2 在极点附近,从3 ??×?? 10 9 到4 ??×?? 10 9 ?cm ?2 赤道。季节性周期和半年振荡的相位表明,从不同仪器中检索到的Na含量之间的差异很小。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到95?km,而模型显示的质心高度平均低2至4?km。这可能是由于WACCM模拟中的绝经时间比测量中值低了3公里。尽管发生了这种全局的2-4 km的偏移,该模型仍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上的变化类似于其中一种测量。此外,在使用模型模拟的配置文件中,还存在使用不同仪器测量的配置文件之间的差异,因此存在不同的本地时间(LTs)。对于垂直列密度和轮廓宽度,也可以找到对横向和时间变化的捕获。

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