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ESA SEPEM project: Peak flux and fluence model

By: Heynderickx, D.; Gabriel, S.B.; Jiggens, P.T.A.; Hilgers, A.; Glover, A.; Crosby, N.;

2011 / IEEE / 978-1-4577-0586-1


This item was taken from the IEEE Conference ' ESA SEPEM project: Peak flux and fluence model ' 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 L� distribution for time distributions and the accounting for the non-poin-like nature of SEP events.