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首页> 外文期刊>Annales Geophysicae >Correlation studies for B-spline modeled F2 Chapman parameters obtained from FORMOSAT-3/COSMIC data
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Correlation studies for B-spline modeled F2 Chapman parameters obtained from FORMOSAT-3/COSMIC data

机译:从FORMOSAT-3 / COSMIC数据获得的B样条模型F2 Chapman参数的相关性研究

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The determination of ionospheric key quantities such as the maximum electrondensity of the F2 layer NmF2, the corresponding F2 peak heighthmF2 and the F2 scale height HF2 are of highrelevance in 4-D ionosphere modeling to provide information on the verticalstructure of the electron density (Ne). The Nedistribution with respect to height can, for instance, be modeled by thecommonly accepted F2 Chapman layer. An adequate and observation drivendescription of the vertical Ne variation can be obtained fromelectron density profiles (EDPs) derived by ionospheric radio occultationmeasurements between GPS and low Earth orbiter (LEO) satellites. For thesepurposes, the six FORMOSAT-3/COSMIC (F3/C) satellites provide an excellentopportunity to collect EDPs that cover most of the ionospheric region, inparticular the F2 layer. For the contents of this paper, F3/C EDPs have beenexploited to determine NmF2, hmF2 andHF2 within a regional modeling approach. As mathematical basefunctions, endpoint-interpolating polynomial B-splines are considered tomodel the key parameters with respect to longitude, latitude and time. Thedescription of deterministic processes and the verification of this modelingapproach have been published previously in Limberger et al. (2013), whereas this papershould be considered as an extension dealing with related correlationstudies, a topic to which less attention has been paid in the literature. Relationsbetween the B-spline series coefficients regarding specific key parameters aswell as dependencies between the three F2 Chapman key parameters are in themain focus. Dependencies are interpreted from the post-derived correlationmatrices as a result of (1) a simulated scenario without data gaps by takingdense, homogenously distributed profiles into account and (2) two real datascenarios on 1 July 2008 and 1 July 2012 including sparsely, inhomogeneouslydistributed F3/C EDPs. Moderate correlations between hmF2and HF2 as well as inverse correlations between NmF2 andHF2 are reflected from the simulation. By means of the real datastudies, it becomes obvious that the sparse measurement distribution leads toan increased weighting of the prior information and suppresses the parametercorrelations which play an important role regarding the parameterestimability. The currently implemented stochastic model is in need ofimprovement and does not consider stochastic correlations which consequentlycannot occur.
机译:确定电离层关键量,例如F2层的最大电子密度 Nm F2,相应的F2峰高 hm F2和F2标尺高度 H F2在4-D电离层建模中具有高度相关性,可提供有关电子密度( N e )的垂直结构的信息。关于高度的 N e 分布可以例如通过公认的F2查普曼层建模。可以从GPS和低地球轨道卫星(LEO)之间的电离层无线电掩星测量得出的电子密度分布(EDP)中获得对垂直 N e 变化的充分描述和观察驱动。为了这些目的,六颗FORMOSAT-3 / COSMIC(F3 / C)卫星为收集覆盖电离层大部分区域(尤其是F2层)的EDP提供了极好的机会。对于本文的内容,已经利用F3 / C EDP来通过区域建模方法确定 Nm F2, hm F2和 H F2。作为数学基础函数,端点插值多项式B样条被认为可以建模关于经度,纬度和时间的关键参数。确定性过程的描述和该建模方法的验证先前已在Limberger等人中发表。 (2013年),而该论文应被视为涉及相关性研究的扩展,但在文献中对此主题的关注较少。 B样条序列系数与特定关键参数之间的关系以及三个F2 Chapman关键参数之间的相关性是重点。从(1)通过考虑密集,均匀分布的配置文件考虑到模拟场景而没有数据缺口的结果,以及(2)2008年7月1日和2012年7月1日的两个真实数据场景(包括稀疏,不均匀分布的F3),可以从派生后的关联矩阵中解释依赖性。 / C EDP。从 hm F2和 H F2之间适度的相关性以及 Nm F2和 H F2之间的逆相关性反映在模拟。通过实际的数据研究,很明显,稀疏的测量分布导致先验信息的加权增加,并且抑制了参数相关性,这在参数可估计性方面起着重要作用。当前实现的随机模型需要改进,并且没有考虑因此不可能发生的随机相关性。

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