辐射屏蔽对抗深空辐射的混合方法
Rajarshi Pal Chowdhury1, Luke A Stegeman1, Matthew L Lund2
1Alan Levin Department of Mechanical and Nuclear Engineering, Kansas State University, Manhattan, KS, United States of America.
Life sciences in space research
|July 22, 2023
概括
这项研究探讨了深空任务的混合活性-被动屏蔽,寻找最佳的配置,以减少太阳粒子事件和银河系宇宙射线的辐射剂量.
科学领域:
- 太空探索 太空探索
- 辐射屏蔽的辐射屏蔽.
- 天体物理学 天体物理学
背景情况:
- 载人深空任务需要在地球磁层之外的强大的辐射保护.
- 由于恶劣的辐射环境,仅仅被动屏蔽对长期任务是不够的.
- 使用电磁场的活性屏蔽提供了一个有前途的补充解决方案.
研究的目的:
- 调查混合活性-被动屏蔽配置对太空辐射的有效性.
- 评估对太阳粒子事件 (SPEs) 和银河系宇宙射线 (GCRs) 的屏蔽性能.
- 为了优化对太阳最小值和太阳最大值条件的屏蔽.
主要方法:
- 一个新的静电活性屏蔽系统被开发和优化.
- 评估了组合了主动和被动屏蔽的混合配置.
- 通过减少有效剂量和放射生物效率 (RBE) 权重剂量来衡量性能.
主要成果:
- 优化的混合配置显示,对SPE和GCR的剂量显著降低.
- 对于SPE,主动屏蔽被放置在被动屏蔽之外.
- 对于GCRs,被动屏蔽先于积极屏蔽来分割HZE离子,从而提高保护.
结论:
- 混合屏蔽是一种可行的策略,可以提高深空中机组人员的安全性.
- 特定的配置对不同的辐射类型 (SPEs与GCRs) 有效.
- 对于未来的任务,积极屏蔽的进一步技术发展至关重要.
相关概念视频
Diamagnetic Shielding of Nuclei: Local Diamagnetic Current
902
An applied magnetic field causes the electrons present in the molecule to circulate, setting up a local diamagnetic current within the molecule. The local diamagnetic current arising from circulating sigma-bonding electrons induces a magnetic field, Blocal that opposes the applied magnetic field, B0. The effective magnetic field experienced by these nuclei is given by the difference between the applied and local magnetic fields in a phenomenon called local diamagnetic shielding. Essentially,...
902
Nuclear Power
7.8K
Controlled nuclear fission reactions are used to generate electricity. Any nuclear reactor that produces power via the fission of uranium or plutonium by bombardment with neutrons has six components: nuclear fuel consisting of fissionable material, a nuclear moderator, a neutron source, control rods, reactor coolant, and a shield and containment system.
Nuclear Fuels
Nuclear fuel consists of a fissile isotope, such as uranium-235, which must be present in sufficient quantity to provide a...
Nuclear Fuels
Nuclear fuel consists of a fissile isotope, such as uranium-235, which must be present in sufficient quantity to provide a...
7.8K
Absorption of Radiation
767
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
767
Radiation: Applications
1.2K
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...
1.2K
Radiation Pressure: Problem Solving
396
The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
396
Biological Effects of Radiation
15.5K
All radioactive nuclides emit high-energy particles or electromagnetic waves. When this radiation encounters living cells, it can cause heating, break chemical bonds, or ionize molecules. The most serious biological damage results when these radioactive emissions fragment or ionize molecules. For example, α and β particles emitted from nuclear decay reactions possess much higher energies than ordinary chemical bond energies. When these particles strike and penetrate matter, they...
15.5K


