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dc.contributor.authorMalandraki, O.E.
dc.contributor.authorCrosby, N.B.
dc.date2018
dc.date.accessioned2023-12-08T09:02:24Z
dc.date.available2023-12-08T09:02:24Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/11195
dc.descriptionThis chapter provides an overview on solar energetic particles (SEPs) and their association to space weather, both from the scientific as well as from the applications perspective. A historical overview is presented on how SEPs were discovered in the 1940s and how our understanding has increased and evolved since then. Current state-of-the-art based on unique measurements obtained in the 3-dimensional heliosphere (e.g. by the Ulysses, ACE, STEREO spacecraft) and their analysis is also presented. Key open questions on SEP research expected to be answered in view of future missions that will explore the solar corona and inner heliosphere are highlighted. This is followed by an introduction to why SEPs are studied, describing the risks that SEP events pose on technology and human health.Mitigation strategies for solar radiation storms as well as examples of current SEP forecasting systems are reviewed, in context of the two novel real-time SEP forecasting tools developed within the EU H2020 HESPERIA project.
dc.languageeng
dc.titleSolar Energetic Particles and SpaceWeather: Science and Applications
dc.typeBook chapter
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleSolar Particle Radiation Storms Forecasting and Analysis: The HESPERIA HORIZON 2020 Project and Beyond
dc.source.volumeAstrophysics and Space Science Library 444
dc.source.page1-26
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/978-3-319-60051-2_1
dc.identifier.url
dc.source.editorMalandraki, O.E.
dc.source.editorCrosby, N.B.


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