斯堪的纳维亚多仪器电离层层析成像与贝叶斯统计反演和相关先验

J. Norberg, J. Vierinen, L. Roininen, O. Amm, M. Lehtinen
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引用次数: 0

摘要

我们提出了一种新的电离层层析成像算法和用它获得的最新结果。电离层层析成像在数学上是一个稀疏的有限角层析成像问题,因此严重不适定。这意味着要获得合理的重构,问题需要很强的正则化。在电离层层析成像中,正则化通常使用一组有限的基函数、吉洪诺夫正则化、迭代方法的初始剖面或这些方案的不同组合来实现。这些方法已经被证明可以产生令人满意的重建,但是正则化的作用以及所选择的方法实际上在多大程度上限制了可能的结果并不总是很清楚。我们的断层扫描方案是在贝叶斯统计框架中实现的(Markkanen等)。安。地球物理学。,第13卷,第1277-1287页,1995年)。在贝叶斯推理中,正则化以先验分布的形式给出。先验分布包含了测量前未知参数的信息。第二步是在给定观测值的情况下,为未知参数建立似然函数。通过将似然与先验密度函数相结合,我们得到了后验分布,根据我们掌握的信息,我们可以从其中获得具有最高概率的估计。在这里,我们给出了具有新的相关先验的先验分布(Roininen等)。逆Probl。图像放大。, vol. 5, issue 2, pp. 611-647, 2011)。本质上,相关先验是高斯马尔可夫随机场,其中我们可以以一种可解释的方式陈述电离层的物理假设。通过这种实现,我们对正则化先验分布的作用有了非常透彻的理解。除此之外,统计框架还提供了一种非常自然的方法来结合不同的电离层测量。因此,我们可以在同一模型中使用低地球轨道(LEO)和全球定位系统(GPS)卫星以及地面测量数据。从2011年开始,作为TomoScand项目的一部分,芬兰气象研究所一直在为LEO信标卫星安装一个新的接收器网络。目前,我们与Sodankyla地球物理观测站的接收网络一起,从11个接收站收集数据。最北部的接收器位于斯瓦尔巴群岛,最南部位于爱沙尼亚。我们还从芬兰Geotrim公司提供的86个GPS接收站收集数据。我们在二维情况下展示了新的网络和算法的最新结果,然而,在不久的将来,我们的目标是将模型扩展到三维情况,以覆盖斯堪的纳维亚半岛。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Multi-instrument ionospheric tomography in Scandinavia with Bayesian statistical inversion and correlation priors
We present a novel algorithm for ionospheric tomography and the latest results obtained with it. Ionospheric tomography is mathematically a sparse limited-angle tomography problem and therefore severely ill-posed. This means that to obtain reasonable reconstructions the problem needs a strong regularisation. In ionospheric tomography the regularisation is often implemented with a limited set of base functions, Tikhonov regularisation, initial profiles for iterative methods, or with a different combinations of these schemes. These methods have been shown to produce satisfactory reconstructions, but the role of the regularisation and how much the chosen method actually constraints the possible outcomes is not always clear. Our tomography scheme is implemented in the Bayesian statistical framework (Markkanen et al. Ann. Geophys., vol. 13, pp. 1277-1287, 1995). In Bayesian inference the regularisation is given as an a priori distribution. The a priori distribution contains the information about the unknown parameters before the measurements. The second step is to build a likelihood function for the unknown parameters, given the observed measurements. By combining the likelihood with the prior density function, we obtain the a posteriori distribution, from where we can obtain the estimate with the highest probability, based on the information in our disposal. Here we give the a priori distribution with the novel correlation priors (Roininen et al. Inverse Probl. Imag., vol. 5, issue 2, pp. 611-647, 2011). Essentially the correlation priors are Gaussian Markov random fields, wherein we can state the physical assumptions of the ionosphere in an interpretable manner. With this implementation we get a very thorough understanding of what is the role of the regularising a priori distribution. On addition to that, the statistical framework also gives a very natural way to combine different ionospheric measurements. Therefore we can use measurements from Low Earth Orbit (LEO) and Global Positioning System (GPS) satellites as well as ground based measurements in the same model. Starting from 2011, as a part of TomoScand project, Finnish Meteorological Institute has been installing a new receiver network for LEO beacon satellites. At the moment, together with the receiver network of Sodankyla Geophysical Observatory, we collect data from 11 receivers stations. The northern most receiver located in Svalbard and southern most in Estonia. We also collect data from 86 GPS receiver stations provided by Finnish company Geotrim. We present the latest results with the new network and algorithm in a 2-dimensional case, however, the goal in the near future is to extend the model to a 3-dimensional case to cover over Scandinavia.
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