Machine learning models for ionospheric foF2 prediction: A comparative analysis

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Radio Science Pub Date : 2026-06-01 Epub Date: 2026-07-03 DOI:10.1029/2025RS008336
R. Atici;Z. Pala
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引用次数: 0

Abstract

Precise prediction of the ionospheric F2-layer critical frequency (foF2) is crucial for a range of technological applications, including high-frequency radio wave propagation, satellite communications, and global navigation satellite systems (GNSS). This study assesses the efficacy of various machine learning (ML) models, such as Support Vector Machines (SVM), Random Forest (RF), K-Nearest Neighbors (KNN), and Linear Regression (LM), in forecasting foF2, and contrasts their performance with the traditional IRI-2020 empirical model. The analysis was conducted at five ionosonde stations representing both high and low latitudes during the solar minimum (2019) and maximum (2023). The findings indicate that the SVM and RF models surpassed the IRI-2020 model, achieving reduced error rates and enhanced explanatory power. The geographical location and volume of the training data significantly influence the model performance. This study underscores the potential of ML models, particularly SVM and RF, for more precise ionospheric parameter predictions, particularly during periods of elevated solar activity.
电离层foF2预测的机器学习模型:比较分析
电离层f2层临界频率(foF2)的精确预测对于包括高频无线电波传播、卫星通信和全球卫星导航系统(GNSS)在内的一系列技术应用至关重要。本研究评估了各种机器学习(ML)模型,如支持向量机(SVM)、随机森林(RF)、k近邻(KNN)和线性回归(LM)在预测foF2方面的效果,并将它们的性能与传统的IRI-2020经验模型进行了对比。分析在太阳极小期(2019年)和极大期(2023年)分别代表高纬度和低纬度的5个电离层探空站进行。结果表明,SVM和RF模型优于IRI-2020模型,错误率降低,解释力增强。训练数据的地理位置和数量对模型性能有显著影响。这项研究强调了ML模型的潜力,特别是SVM和RF,用于更精确的电离层参数预测,特别是在太阳活动加剧的时期。
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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