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首页> 外文期刊>Journal of geophysical research. Planets >Measurements of the neutron spectrum on the Martian surface with MSL/RAD
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Measurements of the neutron spectrum on the Martian surface with MSL/RAD

机译:用MSL/Rad的中子表面的中子光谱的测量

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摘要

The Radiation Assessment Detector (RAD), onboard the Mars Science Laboratory (MSL) rover Curiosity, measures the energetic charged and neutral particles and the radiation dose rate on the surface of Mars. An important factor for determining the biological impact of the Martian surface radiation is the specific contribution of neutrons, with their deeper penetration depth and ensuing high biological effectiveness. This is very difficult to measure quantitatively, resulting in considerable uncertainties in the total radiation dose. In contrast to charged particles, neutral particles (neutrons and gamma rays) are generally only measured indirectly. Measured spectra are a complex convolution of the incident particle spectrum with the detector response function and must be unfolded. We apply an inversion method (based on a maximum likelihood estimation) to calculate the neutron and gamma spectra from the RAD neutral particle measurements. Here we show the first spectra on the surface of Mars and compare them to theoretical predictions. The measured neutron spectrum (ranging from 8 to 740 MeV) translates into a radiation dose rate of 14 ± 4 μGy/d and a dose equivalent rate of 61 ± 15 μSv/d. This corresponds to 7% of the measured total surface dose rate and 10% of the biologically relevant surface dose equivalent rate on Mars. Measuring the Martian neutron and gamma spectra is an essential step for determining the mutagenic influences to past or present life at or beneath the Martian surface as well as the radiation hazard for future human exploration, including the shielding design of a potential habitat.
机译:辐射评估探测器(RAD),火星科学实验室(MSL)的好奇心,测量了火星表面上的充电和中性颗粒和中性颗粒以及辐射剂量的测量。确定火星表面辐射的生物学影响的一个重要因素是中子的特定贡献,其深度深度和随之而来的高生物学有效性。这很难定量测量,导致总辐射剂量的大量不确定性。与带电的颗粒相反,中性颗粒(中子和伽马射线)通常仅间接测量。测得的光谱是与检测器响应函数的入射颗粒光谱的复杂卷积,必须展开。我们应用一种反演方法(基于最大似然估计)来从RAD中性粒子测量值中计算中子和γ光谱。在这里,我们显示了火星表面上的第一光谱,并将其与理论预测进行了比较。测得的中子光谱(范围为8至740 MeV)转化为14±4μgy/d的辐射剂量速率,剂量等效速率为61±15μSV/d。这对应于测量的总表面剂量率的7%和火星上生物学相关的表面剂量当量率的10%。测量火星中子和伽马光谱是确定在火星表面或下方或以下生活的诱变影响以及未来人类勘探的辐射危害的重要步骤,包括潜在栖息地的屏蔽设计。

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