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dc.contributor.authorNuñez-Paz, Marlon 
dc.date.accessioned2018-10-29T12:15:03Z
dc.date.available2018-10-29T12:15:03Z
dc.date.created2018
dc.date.issued2018-10-29
dc.identifier.urihttps://hdl.handle.net/10630/16741
dc.description.abstractThe UMASEP-10 tool [Núñez, 2011] works in an operational level since 2010, and its >10 MeV Solar Energetic Proton (SEP) predictions are diseminated by NASA’s integrated Space Weather Analysis system (iSWA). This presentation shows the real-time predictions of the SEP events that took place in July and September 2017. The UMASEP-10 tool predicts the occurrence and intensity of the first hours of >10 MeV SEP events using the Well-Connected prediction (WCP) model and the Poorly-Connected prediction (PCP) model. The WCP model infers the observer's interplanetary magnetic field connection to the shock source by correlating remote sensing SXR and proton data at near-Earth. This poster also presents a summary of the predictions of the UMASEP-100 [Núñez, 2015] and HESPERIA UMASEP-500 [Núñez et al., 2017] tools for predicting >100 MeV and >500 MeV events, respectively, during the aforementioned period.en_US
dc.description.sponsorshipUniversidad de Málaga. Campus de Excelencia Internacional Andalucía Tech.en_US
dc.language.isoengen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectRadiografíaen_US
dc.titleThe use of observations of soft X-rays and protons in the UMASEP scheme for making real-time predictions of the SEP events that took place in july and september 2017en_US
dc.typeinfo:eu-repo/semantics/conferenceObjecten_US
dc.centroE.T.S.I. Informáticaen_US
dc.relation.eventtitleSolar Heliospheric and Interplanetary Environment (SHINE) Workshop 2018en_US
dc.relation.eventplaceCocoa Beach, Florida, EE.UU,en_US
dc.relation.eventdateAgosto 2-4, 2018en_US


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