HESPERIA REleASE+: Improving Solar Proton Event Forecasting by Means of Automated Recognition of Type‐III Radio Bursts

Abstract This work reports on an attempt toward improving the Relativistic Electron Alert System for Exploration (REleASE): the occurrence of a type‐III radio burst as a precondition for a REleASE forecast. REleASE forecasts are based on the detection of early arrival of near‐relativistic electrons...

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Main Authors: Arik Posner, Olga Ε. Malandraki, Michalis Karavolos, Kostas Tziotziou, Fanis Smanis, Bernd Heber, Henrik Dröge, Patrick Kühl, Giorgos P. Veldes
Format: Article
Language:English
Published: Wiley 2024-12-01
Series:Space Weather
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Online Access:https://doi.org/10.1029/2024SW004013
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author Arik Posner
Olga Ε. Malandraki
Michalis Karavolos
Kostas Tziotziou
Fanis Smanis
Bernd Heber
Henrik Dröge
Patrick Kühl
Giorgos P. Veldes
author_facet Arik Posner
Olga Ε. Malandraki
Michalis Karavolos
Kostas Tziotziou
Fanis Smanis
Bernd Heber
Henrik Dröge
Patrick Kühl
Giorgos P. Veldes
author_sort Arik Posner
collection DOAJ
description Abstract This work reports on an attempt toward improving the Relativistic Electron Alert System for Exploration (REleASE): the occurrence of a type‐III radio burst as a precondition for a REleASE forecast. REleASE forecasts are based on the detection of early arrival of near‐relativistic electrons ahead of more hazardous protons from Solar Energetic Particle (SEP) events. The goal is to allow astronauts on a Lunar or Mars mission sufficient advance warning to reach a radiation shelter to minimize radiation dose exposure. We test a new system that sets a condition of the occurrence of a type‐III radio burst, thus adding independent evidence of particle escape from the Sun, with the aim of reducing known sources of false‐alarms of the existing REleASE system. The High Energy Solar Particle Events foRecastIng and Analysis (HESPERIA) REleASE+ system, which takes advantage of availability of real‐time solar radio observations during the passage of STEREO‐A by Earth in 2023, has now been incorporated in the HESPERIA framework. We discuss the techniques used for automatic detection of type‐III radio bursts preparing for its real‐time implementation, the determination of selection criteria for type‐III bursts that are candidates for solar proton events in the Earth‐moon system, and first results of the combined system.
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spelling doaj-art-2a149570021243e79558d6756ee19d832025-02-01T08:10:33ZengWileySpace Weather1542-73902024-12-012212n/an/a10.1029/2024SW004013HESPERIA REleASE+: Improving Solar Proton Event Forecasting by Means of Automated Recognition of Type‐III Radio BurstsArik Posner0Olga Ε. Malandraki1Michalis Karavolos2Kostas Tziotziou3Fanis Smanis4Bernd Heber5Henrik Dröge6Patrick Kühl7Giorgos P. Veldes8NASA Headquarters Washington DC USANational Observatory of Athens IAASARS Athens GreeceNational Observatory of Athens IAASARS Athens GreeceNational Observatory of Athens IAASARS Athens GreeceNational Observatory of Athens IAASARS Athens GreeceChristian‐Albrechts‐Universität zu Kiel Kiel GermanyChristian‐Albrechts‐Universität zu Kiel Kiel GermanyChristian‐Albrechts‐Universität zu Kiel Kiel GermanyUniversity of Thessaly Volos GreeceAbstract This work reports on an attempt toward improving the Relativistic Electron Alert System for Exploration (REleASE): the occurrence of a type‐III radio burst as a precondition for a REleASE forecast. REleASE forecasts are based on the detection of early arrival of near‐relativistic electrons ahead of more hazardous protons from Solar Energetic Particle (SEP) events. The goal is to allow astronauts on a Lunar or Mars mission sufficient advance warning to reach a radiation shelter to minimize radiation dose exposure. We test a new system that sets a condition of the occurrence of a type‐III radio burst, thus adding independent evidence of particle escape from the Sun, with the aim of reducing known sources of false‐alarms of the existing REleASE system. The High Energy Solar Particle Events foRecastIng and Analysis (HESPERIA) REleASE+ system, which takes advantage of availability of real‐time solar radio observations during the passage of STEREO‐A by Earth in 2023, has now been incorporated in the HESPERIA framework. We discuss the techniques used for automatic detection of type‐III radio bursts preparing for its real‐time implementation, the determination of selection criteria for type‐III bursts that are candidates for solar proton events in the Earth‐moon system, and first results of the combined system.https://doi.org/10.1029/2024SW004013forecasting techniques
spellingShingle Arik Posner
Olga Ε. Malandraki
Michalis Karavolos
Kostas Tziotziou
Fanis Smanis
Bernd Heber
Henrik Dröge
Patrick Kühl
Giorgos P. Veldes
HESPERIA REleASE+: Improving Solar Proton Event Forecasting by Means of Automated Recognition of Type‐III Radio Bursts
Space Weather
forecasting techniques
title HESPERIA REleASE+: Improving Solar Proton Event Forecasting by Means of Automated Recognition of Type‐III Radio Bursts
title_full HESPERIA REleASE+: Improving Solar Proton Event Forecasting by Means of Automated Recognition of Type‐III Radio Bursts
title_fullStr HESPERIA REleASE+: Improving Solar Proton Event Forecasting by Means of Automated Recognition of Type‐III Radio Bursts
title_full_unstemmed HESPERIA REleASE+: Improving Solar Proton Event Forecasting by Means of Automated Recognition of Type‐III Radio Bursts
title_short HESPERIA REleASE+: Improving Solar Proton Event Forecasting by Means of Automated Recognition of Type‐III Radio Bursts
title_sort hesperia release improving solar proton event forecasting by means of automated recognition of type iii radio bursts
topic forecasting techniques
url https://doi.org/10.1029/2024SW004013
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