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首页> 外文期刊>Journal of geophysical research. Planets >Charged particle spectra obtained with the Mars Science Laboratory Radiation Assessment Detector (MSL/RAD) on the surface of Mars
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Charged particle spectra obtained with the Mars Science Laboratory Radiation Assessment Detector (MSL/RAD) on the surface of Mars

机译:通过火星表面上的火星科学实验室辐射评估检测器(MSL/RAD)获得的带电粒子光谱

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摘要

The Radiation Assessment Detector (RAD)-situated inside the Mars Science Laboratory's Curiosity rover-is the first ever instrument to measure the energetic particle radiation environment on the surface of Mars. To fully understand the influence of this surface radiation field in terms of potential hazard to life, a detailed knowledge of its composition is necessary. Charged particles are a major component of this environment, both galactic cosmic rays propagating to the Martian surface and secondary particles created by interactions of these cosmic rays with the atoms of the Martian atmosphere and soil. Here we present particle fluxes for a wide range of ion species, providing detailed energy spectra in the low-energy range (up to several hundred MeV/nucleon particle energy), and integral fluxes for higher energies. In addition to being crucial for the understanding of the hazards of this radiation to possible future manned missions to Mars, the data reported here provide valuable input for evaluating and validating particle transport models currently used to estimate the radiation environment on Mars and elsewhere in space. It is now possible for the first time to compare model results for expected surface particle fluxes with actual ground-based measurements.
机译:在火星科学实验室的好奇心漫游车内,辐射评估探测器(RAD)是有史以来第一个测量火星表面上的能量颗粒辐射环境的仪器。为了完全了解这种表面辐射场的影响,这是对生命的潜在危害,对其组成的详细知识是必要的。带电的颗粒是这种环境的主要组成部分,是银河宇宙射线传播到火星表面和次级颗粒,这些粒子与这些宇宙射线与火星大气和土壤的原子的相互作用所产生。在这里,我们为各种离子物种提供了颗粒通量,在低能范围内提供详细的能量光谱(最高几百meV/核子颗粒能),并为较高能量提供积分磁通。除了对了解这种辐射对火星可能未来的载人任务的危害至关重要之外,此处报告的数据还为评估和验证粒子传输模型目前用于估计火星和太空中其他地方的辐射环境提供了宝贵的输入。现在可以首次将预期表面粒子通量与实际地面测量结果进行比较模型结果。

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