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 |