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Influence of systematic error on least squares retrieval of upper atmospheric parameters from the ultraviolet airglow

机译:系统误差对紫外线气辉的最小二乘检索高层大气参数的影响

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This paper investigates the effect of simple systematic error, or bias (i.e., in the magnitude of data or an associated model), on physical parameters retrieved by least squares algorithms from observations that are indexed by an independent variable. This factor is now of critical interest with the advent of global, space-based ultraviolet remote sensing of thermospheric and ionospheric composition by experimental and operational systems. A finite bias between an observed intensity profile and the parametric physical model used to compute a least squares solution will contaminate the values of retrieved physical parameters. The simplest mitigation method is to retrieve an additional bias adjustment parameter (additive or multiplicative) as part of the solution. The result is a measurably superior fit. The utility of this approach can depend on the particular spectral feature of interest. The discussion includes derivation of relevant equations and diagnostic tests. An illustrative application concerns recent observations of the dayside O II 834 ? airglow, which contains information on O+, the dominant ion in the ionospheric F region.
机译:本文研究了简单的系统误差或偏差(即数据大小或相关模型的偏差)对最小二乘算法从由独立变量索引的观测值中检索到的物理参数的影响。随着通过实验和操作系统对热层和电离层成分进行全球性的,基于空间的紫外线遥感的出现,这一因素现已引起人们的极大关注。在观察到的强度分布和用于计算最小二乘解的参数物理模型之间的有限偏差将污染检索到的物理参数的值。最简单的缓解方法是检索其他偏差调整参数(加法或乘法)作为解决方案的一部分。结果是非常出色的合身性。该方法的实用性可以取决于感兴趣的特定光谱特征。讨论包括相关方程和诊断测试的推导。一个示例性的应用涉及最近对OII 834的观察。气辉,其中包含有关O +(电离层F区中的主要离子)的信息。

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