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Titlebook: Biological Effects and Physics of Solar and Galactic Cosmic Radiation Part B; Charles E. Swenberg,Gerda Horneck,E. G. Stassinopo Book 1993

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,“Liquid–Vapor” Phase Transition,tric results suggest that the number of intermediate lineal energy events increase as the protons are attenuated. These results suggest that while shielding will reduce the total absorbed dose due to a solar proton event, it might not be equally effective in reducing the radiobiological effect of the exposure.
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History of Energetic Solar Protons for the Past Three Solar Cycles Including Cycle 22 Updateears that the 20th and 21st solar cycles are deficient in extremely high energy long duration solar particle events. A summary of solar proton events for the past 50 years is given together with information on the flux of solar protons to various spacecraft orbits.
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Solar Energy and its Interaction with Earth’s Atmospheremore details of the interacting components. Therefore, the near-Earth environments which comprise neutral atmospheric, ionospheric and magnetospheric regions will be discussed in relation to the direct and indirect influences of solar activity.
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HZE Reactions and Data-Base Developmenty (HZE) shielding studies. They will be compared with available experimental data. The background material for this lecture will be available as a review document of over 30 years of research at Langley but will include new results obtained over the last year.
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Relating Space Radiation Environments to Risk Estimatesadiation transport theory to the multistage problem of the induction by radiation of initial lesions in living material and their evolution via physical, chemical, and biological processes at the molecular, cellular, and tissue levels to produce the end point of importance.
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