ESA SEPEM project: Peak flux and fluence model
View/ Open
Authors
Jiggens, P.T.A.
Gabriel, S.B.
Heynderickx, D.
Crosby, N.
Glover, A.
Hilgers, A.
Discipline
Physical sciences
Audience
Scientific
Date
2011Metadata
Show full item recordDescription
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.
Citation
Jiggens, P.T.A.; Gabriel, S.B.; Heynderickx, D.; Crosby, N.; Glover, A.; Hilgers, A. (2011). ESA SEPEM project: Peak flux and fluence model. , Proceedings of the European Conference on Radiation and its Effects on Components and Systems, RADECS, 549-564, DOI: 10.1109/RADECS.2011.6131436.Identifiers
scopus: 2-s2.0-84860149945
Type
Conference
Peer-Review
No
Language
eng