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HZE ion fragmentation cross-section sensitivity and propagated errors in HZE exposure estimates

机译:HZE离子碎裂截面灵敏度和HZE暴露估算中的传播误差

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It has long been recognized that galactic cosmic rays are of such high energy that they tend to pass through available shielding materials resulting in exposure of astronauts and equipment within space vehicles and habitats. Any protection provided by shielding materials result not so much from stopping such particles but by changing their physical character in interaction with shielding material nuclei forming, hopefully, less dangerous species. Clearly, the fidelity of the nuclear cross-sections is essential to correct specification of shield design and sensitivity to cross-section error is important in guiding experimental validation of cross-section models and database. We examine the Boltzmann transport equation which is used to calculate dose equivalent during solar minimum, with units (cSv/yr), associated with various depths of shielding materials. The dose equivalent is a weighted sum of contributions from neutrons, protons, light ions, medium ions and heavy ions using the ICRP-60 LET dependent quality factors. We investigate the sensitivity of dose equivalent calculations due to errors in nuclear fragmentation cross-sections. We do this error analysis for all possible projectile-fragment combinations (14,365 such combinations) to estimate the sensitivity of the shielding calculations to errors in the nuclear fragmentation cross-sections. Numerical differentiation with respect to the cross-sections will be evaluated in a broad class of materials including polyethylene, aluminum and copper. We will identify the most important cross-sections to ensure adequate experimental study and evaluate their impact on propagated errors in shielding estimates. Published by Elsevier Ltd.
机译:长期以来,人们已经认识到银河系宇宙射线具有如此高的能量,以至于它们倾向于穿过可用的屏蔽材料,从而导致宇航员和设备暴露在太空飞行器和栖息地中。屏蔽材料提供的任何保护并不能使颗粒停止,而可以通过与屏蔽材料的核形成相互作用而改变其物理特性,希望是危险性较小的物种。显然,核横截面的保真度对于正确设计屏蔽设计至关重要,并且对横截面误差的敏感性对指导横截面模型和数据库的实验验证非常重要。我们研究了玻耳兹曼输运方程,该方程用于计算最小太阳光期间的剂量当量,单位为(cSv / yr),与各种深度的屏蔽材料相关。当量剂量是使用依赖于ICRP-60 LET的质量因子的中子,质子,轻离子,中离子和重离子贡献的加权总和。我们研究了由于核碎裂截面的错误而导致的剂量当量计算的敏感性。我们对所有可能的弹丸碎片组合(14,365个这样的组合)进行此误差分析,以估计屏蔽计算对核碎裂截面中误差的敏感性。在包括聚乙烯,铝和铜在内的多种材料中,将评估横截面的数值差异。我们将确定最重要的横截面,以确保进行充分的实验研究,并评估其对屏蔽估计中传播误差的影响。由Elsevier Ltd.发布

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