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Heavy ion contributions to organ dose equivalent for the 1977 galactic cosmic ray spectrum
Authors:Steven A Walker  Lawrence W Townsend  John W Norbury
Institution:1. Dept. of Mathematics and Statistics, Old Dominion University, Norfolk, VA 23529, USA;2. Nuclear Engineering Dept., University of Tennessee, Knoxville, TN 37996, USA;3. NASA Langley Research Center, Hampton, VA 23681, USA
Abstract:Estimates of organ dose equivalents for the skin, eye lens, blood forming organs, central nervous system, and heart of female astronauts from exposures to the 1977 solar minimum galactic cosmic radiation spectrum for various shielding geometries involving simple spheres and locations within the Space Transportation System (space shuttle) and the International Space Station (ISS) are made using the HZETRN 2010 space radiation transport code. The dose equivalent contributions are broken down by charge groups in order to better understand the sources of the exposures to these organs. For thin shields, contributions from ions heavier than alpha particles comprise at least half of the organ dose equivalent. For thick shields, such as the ISS locations, heavy ions contribute less than 30% and in some cases less than 10% of the organ dose equivalent. Secondary neutron production contributions in thick shields also tend to be as large, or larger, than the heavy ion contributions to the organ dose equivalents.
Keywords:Galactic cosmic rays  Space radiation
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