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タイトルNASA Galactic Cosmic Radiation Environment Model: Badhwar - O'Neill (2014)
本文(外部サイト)http://hdl.handle.net/2060/20150016022
著者(英)Golge, S.; Slaba, T. C.; O'Neill, P. M.
著者所属(英)NASA Johnson Space Center
発行日2015-07-30
言語eng
内容記述The Badhwar-O'Neill (BON) Galactic Cosmic Ray (GCR) flux model has been used by NASA to certify microelectronic systems and in the analysis of radiation health risks for human space flight missions. Of special interest to NASA is the kinetic energy region below 4.0 GeV/n due to the fact that exposure from GCR behind shielding (e.g., inside a space vehicle) is heavily influenced by the GCR particles from this energy domain. The BON model numerically solves the Fokker-Planck differential equation to account for particle transport in the heliosphere due to diffusion, convection, and adiabatic deceleration under the assumption of a spherically symmetric heliosphere. The model utilizes a comprehensive database of GCR measurements from various particle detectors to determine boundary conditions. By using an updated GCR database and improved model fit parameters, the new BON model (BON14) is significantly improved over the previous BON models for describing the GCR radiation environment of interest to human space flight.
NASA分類Aerospace Medicine; Computer Programming and Software; Space Radiation
レポートNOJSC-CN-33828
権利Copyright, Distribution as joint owner in the copyright


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