Status of Galileo interim radiation electron model
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Engineering topics
Publications and source records attributed to Jun, I..
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Measurements of the high energy, omni-directional electron environment by the Galileo spacecraft Energetic Particle Detector (EDP) were used to develop a new model of Jupiter's trapped electron radiation in the jovian equatorial plane for the range 8 to 16 Jupiter radii.
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The total energy deposition profiles when highenergy electrons impinge on a thick slab of elemental aluminum, copper, and tungsten have been computed using representative Monte Carlo codes (NOVICE, TIGER, MCNP), and compared in this paper.
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The charge deposition profiles created when highenergy (1, 10, and 100 MeV) electrons impinge ona thick slab of elemental aluminum, copper, andtungsten are presented in this paper. The chargedeposition profiles were computed using existing representative Monte Carlo codes: TIGER3.0 (1D module of ITS3.0) and MCNP version 4B. The results showed that TIGER3.0 and MCNP4B agree very well (within ~20% of each other) in the majority of the problem geometry. The TIGER results were considered to be accurate based on previous studies. Thus, it was demonstrated that MCNP, with its powerful geometry capability and flexible source and tally options, could be used in calculations of electron charging in high energy electron-rich space radiation environments.
The enhancement of displacement damage energy deposition due to secondary neutrons, pions, deuterons, and alphas resulting from high energy proton interactions with aluminium and tungsten shielding are examined in this paper.
This paper examines the enhancement of displacement damage energy deposition due to secondary neutrons, pions, deuterons, and alphas resulting from high energy (100-1000MeV) proton interactions with aluminum and tungsten shielding.