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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
Description
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.
Related Topics
Esa Sepem Project
Solar Proton Environment
Virtual Timelines
Sepem Reference Event List
Long Flu Time Series
Proton Peak Flux Model
Lévy Distribution
Sep Events
Time Distributions
Solar Flares
Protons
Instruments
Space Vehicles
Predictive Models
Time Series Analysis
Time Frequency Analysis
Monte Carlo Methods
Statistical Model
Seps
Peak Flux
Fluence
Probabilistic Model
Probabilistic Models
Solar Radiation
Solar Flares
Radiation Effects
Protons
Statistical Analysis
Engineering
Space-based Measurements
