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ESA SEPEM project: Peak flux and fluence model
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.
Esa Sepem Project
Solar Proton Environment
Sepem Reference Event List
Long Flu Time Series
Proton Peak Flux Model
Time Series Analysis
Time Frequency Analysis
Monte Carlo Methods