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<title>Overview of HZETRN and BRNTRN space radiation shielding codes</title>
Author(s) -
John Wilson,
F. A. Cucinotta,
Judy L. Shinn,
Lisa C. Simonsen,
Mohammad Badavi
Publication year - 1996
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.192
H-Index - 176
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.254055
Subject(s) - cosmic ray , spacecraft , electromagnetic shielding , radiation , radiation protection , physics , ionizing radiation , shield , heavy ion , space radiation , nasa deep space network , nuclear engineering , computer science , nuclear physics , irradiation , engineering , electrical engineering , astronomy , ion , petrology , quantum mechanics , geology
The NASA Radiation Health Program has supported basic research over the last decade in radiation physics to develop ionizing radiation transport codes and corresponding data bases for the protection of astronauts from galactic and solar cosmic rays on future deep space missions. The codes describe the interactions of the incident radiations with shield materials where their content is modified by the atomic and nuclear reactions through which high energy heavy ions are fragmented into less massive reaction products and reaction products are produced as radiations as direct knockout of shield constituents or produced as de-excitation products in the reactions. This defines the radiation fields to which specific devices are subjected onboard a spacecraft. Similar reactions occur in the device itself which is the initiating event for the device response. An overview of the computational procedures and data base with some applications to photonic and data processing devices is given.

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