ESA SEPEM project: Peak flux and fluence model

dc.contributor.author	Jiggens, P.T.A.
dc.contributor.author	Gabriel, S.B.
dc.contributor.author	Heynderickx, D.
dc.contributor.author	Crosby, N.
dc.contributor.author	Glover, A.
dc.contributor.author	Hilgers, A.
dc.date	2011
dc.date.accessioned	2016-03-29T12:43:51Z
dc.date.available	2016-03-29T12:43:51Z
dc.identifier.uri	https://orfeo.belnet.be/handle/internal/3086
dc.description	A new modelling methodology for the prediction of the solar proton environment a 1 AU is presented. This new method named Virtual Timelines is applied to the SEPEM Reference Event List derived from a long flu time series of space-based measurements to produce the SEPEM model for proton peak flux and fluence at 1 AU. There are several new components including the use of the Lévy distribution for time distributions and the accounting for the non-poin-like nature of SEP events.
dc.language	eng
dc.title	ESA SEPEM project: Peak flux and fluence model
dc.type	Conference
dc.subject.frascati	Physical sciences
dc.audience	Scientific
dc.source.title	Proceedings of the European Conference on Radiation and its Effects on Components and Systems, RADECS
dc.source.page	549-564
Orfeo.peerreviewed	No
dc.identifier.doi	10.1109/RADECS.2011.6131436
dc.identifier.scopus	2-s2.0-84860149945