An automated approach to link solar flares and energetic particle events measured with Solar Orbiter

dc.contributor.authorJanitzek, Nils
dc.contributor.authorJentgens, Henrik
dc.contributor.authorKistler, Fabian
dc.contributor.authorBischof, Louis
dc.contributor.authorStiefel, Muriel
dc.contributor.authorBarczyński, Krzysztof
dc.contributor.authorZhu, Yingjie
dc.contributor.authorHarra, Louise
dc.contributor.authorGómez-Herrero, Raúl
dc.contributor.authorWarmuth, Alexander
dc.contributor.authorRouillard, Alexis
dc.contributor.authorWimmer-Schweingruber, Robert F.
dc.contributor.authorRodríguez-Pacheco, Javier
dc.contributor.authorKrucker, Samuel
dc.date.accessioned2026-07-07T07:04:40Z
dc.date.issued2026
dc.description.abstractSolar flares and associated eruptions are a known source of solar energetic particles (SEPs), but it is often challenging to establish a precise link between individual flares and SEP events measured in-situ throughout the heliosphere. The Solar Orbiter mission, with its Spectrometer/Telescope for Imaging X-rays (STIX) and Energetic Particle Detector (EPD), provides excellent measurements for systematic studies of these phenomena. Based on these data, we developed an algorithm that automatically links solar flares to SEP electron events using a STIX flare list, SEP electron measurements from EPD, and considering model predictions of magnetic connectivity between the Sun and the spacecraft. As a result, the method identifies several hundred flares to be connected to SEP events - out of more than 25000 flares detected with STIX between 2021 and 2025. The precise linkage criteria can be set by the user - including the accepted distance between flare and modelled magnetic footpoint and the length of the accepted time window for SEP arrival. A first comparison of the automatic method with the CoSEE-Cat electron event catalogue for the time period 2021 - 2022 shows, that about 50% of the links found by the algorithm are actual physical links. The method is already available as quick-look online tool for flare-SEP linkage.
dc.eventEGU General Assembly 2026
dc.event.end2026-05-08
dc.event.start2026-05-03
dc.identifier.doi10.5194/egusphere-egu26-16991
dc.identifier.urihttps://irf.fhnw.ch/handle/11645/56959
dc.identifier.urihttps://doi.org/10.26041/fhnw-16424
dc.language.isoen
dc.relation.ispartofEGU General Assembly 2026
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.spatialWien
dc.subject.ddc520 - Astronomie, Kartografie
dc.titleAn automated approach to link solar flares and energetic particle events measured with Solar Orbiter
dc.type04B - Beitrag Konferenzschrift
dspace.entity.typePublication
fhnw.InventedHereYes
fhnw.ReviewTypepeer-reviewed
fhnw.openAccessCategoryGold
fhnw.publicationStatePublished
fhnw.targetcollectionb508cce9-5084-49ae-a565-d8e5c348c3ab
relation.isAuthorOfPublicationf99cde3e-af59-403e-83b0-b2eddab2ea25
relation.isAuthorOfPublicationab9121ab-4a49-4e1c-8dff-64de0d436131
relation.isAuthorOfPublication.latestForDiscoveryf99cde3e-af59-403e-83b0-b2eddab2ea25
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