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Model for Solar Proton Risk AssessmentA statistical model for cumulative solar proton event fluences and for worst-case flux during space missions is presented. New features include the solar minimum time period and proton energy spectra that extend to higher energies.
Document ID
20040171182
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Xapsos, 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
August 22, 2013
Publication Date
January 1, 2004
Subject Category
Solar Physics
Meeting Information
Meeting: International Nuclear and Space Radiation Conference
Location: Atlanta, GA
Country: United States
Start Date: July 19, 2004
End Date: July 23, 2004
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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