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低地球轨道和深空辐射场的特征。

Characteristic of the radiation field in low Earth orbit and in deep space.

作者信息

Reitz Guenther

机构信息

German Aerospace Center-DLR, Institute of Aerospace Medicine, Radiation Biology, Köln, Germany.

出版信息

Z Med Phys. 2008;18(4):233-43. doi: 10.1016/j.zemedi.2008.06.015.

Abstract

The radiation exposure in space by cosmic radiation can be reduced through careful mission planning and constructive measures as example the provision of a radiation shelter, but it cannot be completely avoided. The reason for that are the extreme high energies of particles in this field and the herewith connected high penetration depth in matter. For missions outside the magnetosphere ionizing radiation is recognized as the key factor through its impact on crew health and performance. In absence of sporadic solar particle events the radiation exposure in Low Earth orbit (LEO) inside Spacecraft is determined by the galactic cosmic radiation (protons and heavier ions) and by the protons inside the South Atlantic Anomaly (SAA), an area where the radiation belt comes closer to the earth surface due to a displacement of the magnetic dipole axes from the Earth's center. In addition there is an albedo source of neutrons produced as interaction products of the primary galactic particles with the atoms of the earth atmosphere. Outside the spacecraft the dose is dominated by the electrons of the horns of the radiation belt located at about 60" latitude in Polar Regions. The radiation field has spatial and temporal variations in dependence of the Earth magnetic field and the solar cycle. The complexity of the radiation field inside a spacecraft is further increased through the interaction of the high energy components with the spacecraft shielding material and with the body of the astronauts. In interplanetary missions the radiation belt will be crossed in a couple of minutes and therefore its contribution to their radiation exposure is quite small, but subsequently the protection by the Earth magnetic field is lost, leaving only shielding measures as exposure reduction means. The report intends to describe the radiation field in space, the interaction of the particles with the magnetic field and shielding material and give some numbers on the radiation exposure in low earth orbits and in interplanetary missions.

摘要

通过精心的任务规划和建设性措施,例如提供辐射屏蔽,可以减少宇宙辐射在太空中造成的辐射暴露,但无法完全避免。原因在于该领域粒子的极高能量以及由此导致的在物质中的高穿透深度。对于磁层之外的任务,电离辐射因其对机组人员健康和性能的影响而被视为关键因素。在没有零星太阳粒子事件的情况下,航天器内低地球轨道(LEO)的辐射暴露由银河宇宙辐射(质子和重离子)以及南大西洋异常区(SAA)内的质子决定,南大西洋异常区是由于磁偶极轴偏离地球中心致使辐射带更靠近地球表面的区域。此外,还有一个反照率中子源,它是初级银河粒子与地球大气原子相互作用产生的产物。在航天器外部,剂量主要由极地地区约60°纬度处辐射带边缘的电子决定。辐射场会随着地磁场和太阳周期产生空间和时间上的变化。航天器内部辐射场的复杂性因高能成分与航天器屏蔽材料以及宇航员身体的相互作用而进一步增加。在行星际任务中,几分钟内就会穿过辐射带,因此其对辐射暴露的贡献相当小,但随后会失去地磁场的保护,只剩下屏蔽措施作为减少辐射暴露的手段。本报告旨在描述太空中的辐射场、粒子与磁场及屏蔽材料的相互作用,并给出低地球轨道和行星际任务中辐射暴露的一些数据。

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