A low ionosphere occultation observation method based on differential weight separation

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Radio Science Pub Date : 2025-02-01 DOI:10.1029/2024RS008152
Jialiang Zhong;Sijia Han;Caiyun Wang;Wei Guo
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引用次数: 0

Abstract

Radio occultation observation has garnered significant attention owing to its low-cost, all-weather, and global coverage feature. However, traditional occultation inversion methods lead to error accumulation due to assumptions that are not entirely suitable in the real ionospheric environment, resulting in poor performance in the low ionosphere (D, E layers). In this article, we propose a new method for inverting the electron density in low ionosphere using high-precision 50 Hz occultation data. This method can eliminate the fixed constant term of 50 Hz data and obtain a sharper weighting function through epoch differencing. The inversion results have a good consistency with the results of the ionosonde, with a correlation coefficient of 0.92 and a determination coefficient of 0.85. In addition, the new method can retrieve local details of electron density profiles and capture sporadic E layer (Es), providing support for the study of Es layer morphology and structure.
基于差重分离的低电离层掩星观测方法
射电掩星观测以其低成本、全天候、全球覆盖的特点而备受关注。然而,传统掩星反演方法由于假设不完全适用于真实电离层环境,导致误差积累,导致在低电离层(D、E层)性能较差。本文提出了一种利用高精度50 Hz掩星数据反演低电离层电子密度的新方法。该方法可以消除50 Hz数据的固定常数项,通过历元差分得到更清晰的加权函数。反演结果与电离层探空仪的结果具有较好的一致性,相关系数为0.92,决定系数为0.85。此外,该方法可以获取电子密度分布的局部细节,并捕获零星的E层(Es),为Es层形貌和结构的研究提供支持。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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