Predicting Equatorial Ionospheric Convective Instability Using Machine Learning

Abstract The numerical forecast methods used to predict ionospheric convective plasma instabilities associated with Equatorial Spread‐F (ESF) have limited accuracy and are often computationally expensive. We test whether it is possible to bypass first‐principle numeric simulations and forecast irreg...

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Main Authors: D. Garcia, E. L. Rojas, D. L. Hysell
Format: Article
Language:English
Published: Wiley 2023-12-01
Series:Space Weather
Subjects:
Online Access:https://doi.org/10.1029/2023SW003505
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author D. Garcia
E. L. Rojas
D. L. Hysell
author_facet D. Garcia
E. L. Rojas
D. L. Hysell
author_sort D. Garcia
collection DOAJ
description Abstract The numerical forecast methods used to predict ionospheric convective plasma instabilities associated with Equatorial Spread‐F (ESF) have limited accuracy and are often computationally expensive. We test whether it is possible to bypass first‐principle numeric simulations and forecast irregularities using machine learning models. The data are obtained from the incoherent scatter radar at the Jicamarca Radio Observatory located in Lima, Peru. Our models map vertical plasma drifts, time, and solar activity to the occurrence and location of clusters of echoes telltale of ionospheric irregularities. Our results show that these models are capable of identifying the predictive power of the tested inputs, obtaining accuracies around 75%.
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institution Kabale University
issn 1542-7390
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spelling doaj-art-cee66584a35940569474526833f143ae2025-01-14T16:30:45ZengWileySpace Weather1542-73902023-12-012112n/an/a10.1029/2023SW003505Predicting Equatorial Ionospheric Convective Instability Using Machine LearningD. Garcia0E. L. Rojas1D. L. Hysell2Electrical and Computer Engineering Cornell University Ithaca NY USAEarth and Atmospheric Sciences Cornell University Ithaca NY USAEarth and Atmospheric Sciences Cornell University Ithaca NY USAAbstract The numerical forecast methods used to predict ionospheric convective plasma instabilities associated with Equatorial Spread‐F (ESF) have limited accuracy and are often computationally expensive. We test whether it is possible to bypass first‐principle numeric simulations and forecast irregularities using machine learning models. The data are obtained from the incoherent scatter radar at the Jicamarca Radio Observatory located in Lima, Peru. Our models map vertical plasma drifts, time, and solar activity to the occurrence and location of clusters of echoes telltale of ionospheric irregularities. Our results show that these models are capable of identifying the predictive power of the tested inputs, obtaining accuracies around 75%.https://doi.org/10.1029/2023SW003505machine learningequatorial spread Fforecastingneural networksrandom forestsionospheric irregularities
spellingShingle D. Garcia
E. L. Rojas
D. L. Hysell
Predicting Equatorial Ionospheric Convective Instability Using Machine Learning
Space Weather
machine learning
equatorial spread F
forecasting
neural networks
random forests
ionospheric irregularities
title Predicting Equatorial Ionospheric Convective Instability Using Machine Learning
title_full Predicting Equatorial Ionospheric Convective Instability Using Machine Learning
title_fullStr Predicting Equatorial Ionospheric Convective Instability Using Machine Learning
title_full_unstemmed Predicting Equatorial Ionospheric Convective Instability Using Machine Learning
title_short Predicting Equatorial Ionospheric Convective Instability Using Machine Learning
title_sort predicting equatorial ionospheric convective instability using machine learning
topic machine learning
equatorial spread F
forecasting
neural networks
random forests
ionospheric irregularities
url https://doi.org/10.1029/2023SW003505
work_keys_str_mv AT dgarcia predictingequatorialionosphericconvectiveinstabilityusingmachinelearning
AT elrojas predictingequatorialionosphericconvectiveinstabilityusingmachinelearning
AT dlhysell predictingequatorialionosphericconvectiveinstabilityusingmachinelearning