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Model for Solar Proton Risk AssessmentA statistical model for cumulative solar proton event fluences during space missions is presented that covers both the solar minimum and solar maximum phases of the solar cycle. It is based on data from the IMP and GOES series of satellites that is integrated together to allow the best features of each data set to be taken advantage of. This allows fluence-energy spectra to be extended out to energies of 327 MeV.
Document ID
20050156931
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Xapos, M. A. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Stauffer, C. (SGT, Inc. Greenbelt , MD, United States)
Gee, G. B. (SGT, Inc. Greenbelt , MD, United States)
Barth, J. L. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Stassinopoulos, E. G. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
McGuire, R. E. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2004
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Public Use Permitted.

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