Iterative gradient correction (IGC) method for true height analysis of ionograms

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Radio Science Pub Date : 2023-11-01 DOI:10.1029/2023RS007808
M. Ankita;S. Tulasi Ram
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引用次数: 0

Abstract

Inversion of precise true height electron density profile from the measured virtual heights by the Ionosonde is a quite challenging and ill-posed problem. In this paper, we present a new method to compute the true height profiles from ionograms that relies on computing the propagation path of radio waves with time. This method does not use predefined polynomial functions to fit the vertical electron density distribution; hence, it is free from fitting errors. Instead, this method implements iterative corrections in the electron density gradient between the successive points and progressively reconstructs the true height profile. This Iterative Gradient Correction (IGC) method assures minimizing the error to below a tolerance limit at all sampled points on the ionogram. The true height profiles derived from this method exhibit better accuracy than those derived from the widely used POLynomial ANalysis, particularly, at cusp and F2-peak regions. Further, the IGC method gives the best results at higher sampling resolutions of ionograms and is less sensitive to scaling errors.
用于离子图真实高度分析的迭代梯度校正(IGC)方法
从离子探空仪测量的虚拟高度反演精确的真高度电子密度分布是一个非常具有挑战性和不适定的问题。本文提出了一种通过计算无线电波随时间的传播路径来计算电离图真实高度分布的新方法。该方法不使用预定义的多项式函数来拟合电子密度的垂直分布;因此,它不存在拟合误差。相反,该方法在连续点之间的电子密度梯度中进行迭代修正,逐步重建真实高度轮廓。这种迭代梯度校正(IGC)方法确保在离子图上的所有采样点将误差最小化到容限以下。与常用的多项式分析方法相比,该方法得到的真实高度剖面具有更好的精度,特别是在尖峰和f2峰区域。此外,IGC方法在更高的离子图采样分辨率下获得了最好的结果,并且对标度误差不太敏感。
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来源期刊
Radio Science
Radio Science 工程技术-地球化学与地球物理
CiteScore
3.30
自引率
12.50%
发文量
112
审稿时长
1 months
期刊介绍: Radio Science (RDS) publishes original scientific contributions on radio-frequency electromagnetic-propagation and its applications. Contributions covering measurement, modelling, prediction and forecasting techniques pertinent to fields and waves - including antennas, signals and systems, the terrestrial and space environment and radio propagation problems in radio astronomy - are welcome. Contributions may address propagation through, interaction with, and remote sensing of structures, geophysical media, plasmas, and materials, as well as the application of radio frequency electromagnetic techniques to remote sensing of the Earth and other bodies in the solar system.
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