ORIGINAL RESEARCH article
Front. Astron. Space Sci.
Sec. Space Physics
Volume 12 - 2025 | doi: 10.3389/fspas.2025.1503134
This article is part of the Research TopicFrontier Research in Equatorial Aeronomy and Space PhysicsView all 13 articles
Modeling Ionograms and Critical Plasma Frequencies With Neural Networks
Provisionally accepted- 1Haystack Observatory, Massachusetts Institute of Technology, Cambridge, United States
- 2Cornell University, Ithaca, New York, United States
- 3Pontifical Catholic University of Peru, Lima, Peru
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Ionosondes provide superior spatial coverage and a more comprehensive sampling of the lower ionosphere than other alternatives. In this work, we used neural networks (NN) to forecast ionograms across two solar activity periods. The ionosonde data was obtained from the digisonde at the Jicamarca Radio Observatory (JRO). Each NN comprises one NN that estimates the ionogram trace and another one that estimates the critical frequency. Furthermore, two forecasting models were implemented. The first one was trained with all available data and was optimized for accurate predictions along that time range. The second one was trained using a rolling-window strategy with just three months of data to predict one day of ionograms. Our results show that both models are comparable and can often outperform predictions by empirical and numerical models.The hyperparameters of both models were optimized using a specialized library. Moreover, we found that a few months of data was enough to produce predictions of comparable accuracy to the reference models. We argue that this high accuracy is obtained because the NN captures the dominant periodic drivers. Finally, we provide suggestions for improving this model.
Keywords: neural networks, Forecasting, Ionosonde, Ionograms, Ionosphere
Received: 28 Sep 2024; Accepted: 14 Feb 2025.
Copyright: © 2025 Rojas Villalba, Aricoche and Milla. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
* Correspondence: Enrique Rojas Villalba, Haystack Observatory, Massachusetts Institute of Technology, Cambridge, United States
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