Probabilistic Models for Solar Particle Events

Details Probabilistic Models for Solar Particle Events Probabilistic Models for Solar Particle Events

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh33a1484a&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SH33A-1484

Mathematics

Logic

[7514] Solar Physics, Astrophysics, And Astronomy / Energetic Particles, [7934] Space Weather / Impacts On Technological Systems, [7959] Space Weather / Models, [7984] Space Weather / Space Radiation Environment

Scientific paper

Probabilistic Models of Solar Particle Events (SPEs) are used in space mission design studies to describe the radiation environment that can be expected at a specified confidence level. The task of the designer is then to choose a design that will operate in the model radiation environment. Probabilistic models have already been developed for solar proton events that describe the peak flux, event-integrated fluence and mission-integrated fluence. In addition a probabilistic model has been developed that describes the mission-integrated fluence for the Z>2 elemental spectra. This talk will focus on completing this suite of models by developing models for peak flux and event-integrated fluence elemental spectra for the Z>2 elements. These new probabilistic models are based on an extensive survey of SPE measurements of peak and event-integrated elemental differential energy spectra. Attempts are made to fit the measured spectra with eight different published models. The model giving the best fit to each spectrum is chosen and used to represent that spectrum at any energy in the energy range covered by the model. The set of all such spectral representations for each element is then used to determine the worst case spectrum at each confidence level. The spectral representation that best fits these worst case spectra is found and its dependence on confidence level is parameterized. This procedure is used to create the probabilistic models for the peak and event-integrated spectra.

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