Forecasting the Remaining Duration of an Ongoing Solar Flare

Abstract The solar X‐ray irradiance is significantly heightened during the course of a solar flare, which can cause radio blackouts due to ionization of the atoms in the ionosphere. As the duration of a solar flare is not related to the size of that flare, it is not directly clear how long those bla...

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Main Authors: Jeffrey W. Reep, Will T. Barnes
Format: Article
Language:English
Published: Wiley 2021-10-01
Series:Space Weather
Subjects:
Online Access:https://doi.org/10.1029/2021SW002754
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author Jeffrey W. Reep
Will T. Barnes
author_facet Jeffrey W. Reep
Will T. Barnes
author_sort Jeffrey W. Reep
collection DOAJ
description Abstract The solar X‐ray irradiance is significantly heightened during the course of a solar flare, which can cause radio blackouts due to ionization of the atoms in the ionosphere. As the duration of a solar flare is not related to the size of that flare, it is not directly clear how long those blackouts can persist. Using a random forest regression model trained on data taken from X‐ray light curves, we have developed a direct forecasting method that predicts how long the event will remain above background levels. We test this on a large collection of flares observed with GOES‐15, and show that it generally outperforms simple linear regression, giving a median error of less than 2 min for the approximate end time of a flare. This random forest model is computationally light enough to be performed in real time, allowing for the prediction to be made during the course of a flare.
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spelling doaj-art-077219aa02cc47a08624e0103ba9019c2025-01-14T16:30:34ZengWileySpace Weather1542-73902021-10-011910n/an/a10.1029/2021SW002754Forecasting the Remaining Duration of an Ongoing Solar FlareJeffrey W. Reep0Will T. Barnes1Space Science Division US Naval Research Laboratory Washington DC USANational Research Council Research Associate Residing at the Naval Research Laboratory Washington DC USAAbstract The solar X‐ray irradiance is significantly heightened during the course of a solar flare, which can cause radio blackouts due to ionization of the atoms in the ionosphere. As the duration of a solar flare is not related to the size of that flare, it is not directly clear how long those blackouts can persist. Using a random forest regression model trained on data taken from X‐ray light curves, we have developed a direct forecasting method that predicts how long the event will remain above background levels. We test this on a large collection of flares observed with GOES‐15, and show that it generally outperforms simple linear regression, giving a median error of less than 2 min for the approximate end time of a flare. This random forest model is computationally light enough to be performed in real time, allowing for the prediction to be made during the course of a flare.https://doi.org/10.1029/2021SW002754solar flaresforecasting
spellingShingle Jeffrey W. Reep
Will T. Barnes
Forecasting the Remaining Duration of an Ongoing Solar Flare
Space Weather
solar flares
forecasting
title Forecasting the Remaining Duration of an Ongoing Solar Flare
title_full Forecasting the Remaining Duration of an Ongoing Solar Flare
title_fullStr Forecasting the Remaining Duration of an Ongoing Solar Flare
title_full_unstemmed Forecasting the Remaining Duration of an Ongoing Solar Flare
title_short Forecasting the Remaining Duration of an Ongoing Solar Flare
title_sort forecasting the remaining duration of an ongoing solar flare
topic solar flares
forecasting
url https://doi.org/10.1029/2021SW002754
work_keys_str_mv AT jeffreywreep forecastingtheremainingdurationofanongoingsolarflare
AT willtbarnes forecastingtheremainingdurationofanongoingsolarflare