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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Making limb and nadir measurements comparable: A common volume study of PMC brightness observed by Odin OSIRIS and AIM CIPS
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Making limb and nadir measurements comparable: A common volume study of PMC brightness observed by Odin OSIRIS and AIM CIPS

机译:制作肢体和Nadir测量可比:Odin Osiris和AIM CIPS观察到PMC亮度的常见卷研究

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AbstractCombining limb and nadir satellite observations of Polar Mesospheric Clouds (PMCs) has long been recognized as problematic due to differences in observation geometry, scattering conditions, and retrieval approaches. This study offers a method of comparing PMC brightness observations from the nadir-viewing Aeronomy of Ice in the Mesosphere (AIM) Cloud Imaging and Particle Size (CIPS) instrument and the limb-viewing Odin Optical Spectrograph and InfraRed Imaging System (OSIRIS). OSIRIS and CIPS measurements are made comparable by defining a common volume for overlapping OSIRIS and CIPS observations for two northern hemisphere (NH) PMC seasons: NH08 and NH09. We define a scattering intensity quantity that is suitable for either nadir or limb observations and for different scattering conditions. A known CIPS bias is applied, differences in instrument sensitivity are analyzed and taken into account, and effects of cloud inhomogeneity and common volume definition on the comparison are discussed. Not accounting for instrument sensitivity differences or inhomogeneities in the PMC field, the mean relative difference in cloud brightness (CIPS - OSIRIS) is ?102?±?55%. The differences are largest for coincidences with very inhomogeneous clouds that are dominated by pixels that CIPS reports as non-cloud points. Removing these coincidences, the mean relative difference in cloud brightness reduces to ?6 ± 14%. The correlation coefficient between the CIPS and OSIRIS measurements of PMC brightness variations in space and time is remarkably high, at 0.94. Overall, the comparison shows excellent agreement despite different retrieval approaches and observation geometries
机译:<![CDATA [ 抽象 组合肢体和Nadir卫星观察极性态度云(PMC)的卫星观察,由于差异,长期被认为是有问题的观察几何形状,散射条件和检索方法。本研究提供了一种比较PMC亮度观察的方法,这些方法从Messphere(AIM)云成像和粒度(CIPS)仪器和肢体观察Odin光谱仪和红外成像系统(Osiris)中的冰中的Nadir-Virecion通过定义用于重叠Osiris和两个北半球(NH)PMC Seasons:NH08和NH09的普通体积来进行欧洲航空公司和CIPS测量。我们定义了适用于Nadir或肢体观察的散射强度量,以及用于不同的散射条件。应用了已知的CIP偏压,讨论并考虑了仪器敏感性的差异,并讨论了云不均匀性和常见体积定义对比较的影响。没有考虑PMC场中的仪器敏感性差异或不均匀性,云亮度(CIPS - Osiris)的平均相对差异是?102?±55%。对于具有非常不均匀的云的巧合,差异是最大的,这些云是由CIPS报告为非云点的像素主导。除去这些巧合,云亮度的平均相对差异降低到6±14%。 CIP和Osiris之间的相关系数与空间和时间的亮度变化的测量值非常高,在0.94时显着高。总体而言,尽管不同的检索方法和观察几何形状表现出卓越的协议

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