Probabilistic prediction of geomagnetic storms and the Kp index

Geomagnetic activity is often described using summary indices to summarize the likelihood of space weather impacts, as well as when parameterizing space weather models. The geomagnetic index K p in particular, is widely used for these purposes. Current state-of-the-art forecast models provide dete...

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Main Authors: Chakraborty Shibaji, Morley Steven Karl
Format: Article
Language:English
Published: EDP Sciences 2020-01-01
Series:Journal of Space Weather and Space Climate
Subjects:
Online Access:https://www.swsc-journal.org/articles/swsc/full_html/2020/01/swsc190086/swsc190086.html
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spelling doaj-f4b0b23cce8e4888b11a067beb4eabba2021-04-02T12:47:27ZengEDP SciencesJournal of Space Weather and Space Climate2115-72512020-01-01103610.1051/swsc/2020037swsc190086Probabilistic prediction of geomagnetic storms and the Kp indexChakraborty Shibaji0https://orcid.org/0000-0001-6792-0037Morley Steven Karl1https://orcid.org/0000-0001-8520-0199Bradley Department of Electrical & Computer Engineering, Virginia TechSpace Science and Applications (ISR-1), Los Alamos National LaboratoryGeomagnetic activity is often described using summary indices to summarize the likelihood of space weather impacts, as well as when parameterizing space weather models. The geomagnetic index K p in particular, is widely used for these purposes. Current state-of-the-art forecast models provide deterministic K p predictions using a variety of methods – including empirically-derived functions, physics-based models, and neural networks – but do not provide uncertainty estimates associated with the forecast. This paper provides a sample methodology to generate a 3-hour-ahead K p prediction with uncertainty bounds and from this provide a probabilistic geomagnetic storm forecast. Specifically, we have used a two-layered architecture to separately predict storm (K p  ≥ 5−) and non-storm cases. As solar wind-driven models are limited in their ability to predict the onset of transient-driven activity we also introduce a model variant using solar X-ray flux to assess whether simple models including proxies for solar activity can improve the predictions of geomagnetic storm activity with lead times longer than the L1-to-Earth propagation time. By comparing the performance of these models we show that including operationally-available information about solar irradiance enhances the ability of predictive models to capture the onset of geomagnetic storms and that this can be achieved while also enabling probabilistic forecasts.https://www.swsc-journal.org/articles/swsc/full_html/2020/01/swsc190086/swsc190086.htmlgeomagnetic stormsk p forecastingdeep learninglstmgaussian process
collection DOAJ
language English
format Article
sources DOAJ
author Chakraborty Shibaji
Morley Steven Karl
spellingShingle Chakraborty Shibaji
Morley Steven Karl
Probabilistic prediction of geomagnetic storms and the Kp index
Journal of Space Weather and Space Climate
geomagnetic storms
k p forecasting
deep learning
lstm
gaussian process
author_facet Chakraborty Shibaji
Morley Steven Karl
author_sort Chakraborty Shibaji
title Probabilistic prediction of geomagnetic storms and the Kp index
title_short Probabilistic prediction of geomagnetic storms and the Kp index
title_full Probabilistic prediction of geomagnetic storms and the Kp index
title_fullStr Probabilistic prediction of geomagnetic storms and the Kp index
title_full_unstemmed Probabilistic prediction of geomagnetic storms and the Kp index
title_sort probabilistic prediction of geomagnetic storms and the kp index
publisher EDP Sciences
series Journal of Space Weather and Space Climate
issn 2115-7251
publishDate 2020-01-01
description Geomagnetic activity is often described using summary indices to summarize the likelihood of space weather impacts, as well as when parameterizing space weather models. The geomagnetic index K p in particular, is widely used for these purposes. Current state-of-the-art forecast models provide deterministic K p predictions using a variety of methods – including empirically-derived functions, physics-based models, and neural networks – but do not provide uncertainty estimates associated with the forecast. This paper provides a sample methodology to generate a 3-hour-ahead K p prediction with uncertainty bounds and from this provide a probabilistic geomagnetic storm forecast. Specifically, we have used a two-layered architecture to separately predict storm (K p  ≥ 5−) and non-storm cases. As solar wind-driven models are limited in their ability to predict the onset of transient-driven activity we also introduce a model variant using solar X-ray flux to assess whether simple models including proxies for solar activity can improve the predictions of geomagnetic storm activity with lead times longer than the L1-to-Earth propagation time. By comparing the performance of these models we show that including operationally-available information about solar irradiance enhances the ability of predictive models to capture the onset of geomagnetic storms and that this can be achieved while also enabling probabilistic forecasts.
topic geomagnetic storms
k p forecasting
deep learning
lstm
gaussian process
url https://www.swsc-journal.org/articles/swsc/full_html/2020/01/swsc190086/swsc190086.html
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