Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural Networks

Abstract The Disturbance storm time (Dst) index has been widely used as a proxy for the ring current intensity, and therefore as a measure of geomagnetic activity. It is derived by measurements from four ground magnetometers in the geomagnetic equatorial region. We present a new model for predicting...

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Main Authors: A. Hu, E. Camporeale, B. Swiger
Format: Article
Language:English
Published: Wiley 2023-04-01
Series:Space Weather
Subjects:
Online Access:https://doi.org/10.1029/2022SW003286
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author A. Hu
E. Camporeale
B. Swiger
author_facet A. Hu
E. Camporeale
B. Swiger
author_sort A. Hu
collection DOAJ
description Abstract The Disturbance storm time (Dst) index has been widely used as a proxy for the ring current intensity, and therefore as a measure of geomagnetic activity. It is derived by measurements from four ground magnetometers in the geomagnetic equatorial region. We present a new model for predicting Dst with a lead time between 1 and 6 hr. The model is first developed using a Gated Recurrent Unit (GRU) network that is trained using solar wind parameters. The uncertainty of the Dst model is then estimated by using the Accurate and Reliable Uncertainty Estimate method (Camporeale & Carè, 2021, https://doi.org/10.1615/int.j.uncertaintyquantification.2021034623). Finally, a multi‐fidelity boosting method is developed in order to enhance the accuracy of the model and reduce its associated uncertainty. It is shown that the developed model can predict Dst 6 hr ahead with a root‐mean‐square‐error of 13.54 nT. This is significantly better than a persistence model or a single GRU model.
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spelling doaj-art-3cb36b81a5e0426399ade72233febb3a2025-01-14T16:26:47ZengWileySpace Weather1542-73902023-04-01214n/an/a10.1029/2022SW003286Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural NetworksA. Hu0E. Camporeale1B. Swiger2CIRES University of Colorado Boulder CO USACIRES University of Colorado Boulder CO USACIRES University of Colorado Boulder CO USAAbstract The Disturbance storm time (Dst) index has been widely used as a proxy for the ring current intensity, and therefore as a measure of geomagnetic activity. It is derived by measurements from four ground magnetometers in the geomagnetic equatorial region. We present a new model for predicting Dst with a lead time between 1 and 6 hr. The model is first developed using a Gated Recurrent Unit (GRU) network that is trained using solar wind parameters. The uncertainty of the Dst model is then estimated by using the Accurate and Reliable Uncertainty Estimate method (Camporeale & Carè, 2021, https://doi.org/10.1615/int.j.uncertaintyquantification.2021034623). Finally, a multi‐fidelity boosting method is developed in order to enhance the accuracy of the model and reduce its associated uncertainty. It is shown that the developed model can predict Dst 6 hr ahead with a root‐mean‐square‐error of 13.54 nT. This is significantly better than a persistence model or a single GRU model.https://doi.org/10.1029/2022SW003286machine learninguncertainty quantificationgeomagnetic stormspace weathersolar windensemble model
spellingShingle A. Hu
E. Camporeale
B. Swiger
Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural Networks
Space Weather
machine learning
uncertainty quantification
geomagnetic storm
space weather
solar wind
ensemble model
title Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural Networks
title_full Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural Networks
title_fullStr Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural Networks
title_full_unstemmed Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural Networks
title_short Multi‐Hour‐Ahead Dst Index Prediction Using Multi‐Fidelity Boosted Neural Networks
title_sort multi hour ahead dst index prediction using multi fidelity boosted neural networks
topic machine learning
uncertainty quantification
geomagnetic storm
space weather
solar wind
ensemble model
url https://doi.org/10.1029/2022SW003286
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AT ecamporeale multihouraheaddstindexpredictionusingmultifidelityboostedneuralnetworks
AT bswiger multihouraheaddstindexpredictionusingmultifidelityboostedneuralnetworks