University of Rome and INFN Tor Vergata, Department of Physics, Via della Ricerca Scientifica 1, 00133, Rome, Italy.
Radiat Res. 2011 Sep;176(3):397-406. doi: 10.1667/rr2179.1. Epub 2011 May 11.
The uneven shielding of the International Space Station from the vessel hull, racks and experiments produces a modulation of the internal radiation environment. A detailed knowledge of this environment, and therefore of the Station's shielding effectiveness, is mandatory for an accurate assessment of radiation risk. We present here the first 3D measurements of the Station's radiation environment, discriminating particle trajectories and LET, made possible using the detection capability of the ALTEA-space detector. We provide evidence for a strong (factor ≈ 3) anisotropy in the inner integral LET for high-LET particles (LET > 50 keV/µm) showing a minimum along the longitudinal station axis (most shielded) and a maximum normal to it. Integrating over all measured LETs, the anisotropy is strongly reduced, showing that unstopped light ions plus the fragments produced by heavier ions approximately maintain flux/LET isotropy. This suggests that, while changing the quality of radiation, the extra shielding along the station main axis is not producing a benefit in terms of total LET. These features should be taken into account (1) when measuring radiation with detectors that cannot distinguish the direction of the impinging radiation or that are unidirectional, (2) when planning radiation biology experiments on the ISS, and (3) when simulating the space radiation environment for experiments on the ground. A novel analysis technique that fully exploits the ability to retrieve the angular distribution of the radiation is also presented as well as the angular particle flux and LET characteristic of three geomagnetic zones measured during 2009 by the ALTEA-space detector. This technique is applied to the ALTEA-space detector, but a wider applicability to other detectors is suggested.
国际空间站对船体、机架和实验的不均匀屏蔽会导致内部辐射环境发生调制。因此,为了准确评估辐射风险,必须详细了解这种环境,也就是空间站的屏蔽效果。我们在此介绍了首次使用 ALTEA-space 探测器的检测能力对空间站辐射环境进行的 3D 测量,对粒子轨迹和 LET 进行了区分。我们提供了高 LET 粒子(LET > 50 keV/μm)内部积分 LET 存在强烈各向异性的证据(因子≈3),沿空间站纵轴(屏蔽最强)最小,垂直于此轴最大。对所有测量的 LET 积分后,各向异性大大降低,表明未被阻止的轻离子加上较重离子产生的碎片基本保持通量/LET 各向同性。这表明,虽然改变了辐射的质量,但沿空间站主轴线增加的额外屏蔽并不能带来总 LET 的好处。在使用无法区分入射辐射方向或单向的探测器测量辐射时,在 ISS 上进行辐射生物学实验时,以及在为地面实验模拟空间辐射环境时,都应该考虑到这些特征。我们还提出了一种新的分析技术,它充分利用了恢复辐射角分布的能力,以及在 2009 年期间由 ALTEA-space 探测器测量的三个地磁区的角向粒子通量和 LET 特征。这种技术适用于 ALTEA-space 探测器,但也建议更广泛地应用于其他探测器。