A method to predict space radiation biological effectiveness for non-cancer effects following intense Solar Particle Events

IF 4.6 Q2 MATERIALS SCIENCE, BIOMATERIALS ACS Applied Bio Materials Pub Date : 2024-04-02 DOI:10.1016/j.lssr.2024.03.006
R.L. Ramos , M.P. Carante , E. Bernardini , A. Ferrari , P. Sala , V. Vercesi , F. Ballarini
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Abstract

In addition to the continuous exposure to cosmic rays, astronauts in space are occasionally exposed to Solar Particle Events (SPE), which involve less energetic particles but can deliver much higher doses. The latter can exceed several Gy in a few hours for the most intense SPEs, for which non-stochastic effects are thus a major concern. To identify adequate shielding conditions that would allow respecting the dose limits established by the various space agencies, the absorbed dose in the considered organ/tissue must be multiplied by the corresponding Relative Biological Effectiveness (RBE), which is a complex quantity depending on several factors including particle type and energy, considered biological effect, level of effect (and thus absorbed dose), etc.

While in several studies only the particle-type dependence of RBE is taken into account, in this work we developed and applied a new approach where, thanks to an interface between the FLUKA Monte Carlo transport code and the BIANCA biophysical model, the RBE dependence on particle energy and absorbed dose was also considered. Furthermore, we included in the considered SPE spectra primary particles heavier than protons, which in many studies are neglected. This approach was then applied to the October 2003 SPE (the most intense SPE of solar cycle 23, also known as “Halloween event”) and the January 2005 event, which was characterized by a lower fluence but a harder spectrum, i.e., with higher-energy particles. The calculation outcomes were then discussed and compared with the current dose limits established for skin and blood forming organs in case of 30-days missions.

This work showed that the BIANCA model, if interfaced to a radiation transport code, can be used to calculate the RBE values associated to Solar Particle Events. More generally, this work emphasizes the importance of taking into account the RBE dependence on particle energy and dose when calculating equivalent doses.

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预测强烈太阳粒子事件后空间辐射生物效应对非癌症影响的方法
除了持续暴露于宇宙射线之外,宇航员在太空中偶尔也会暴露于太阳粒子事件(SPE),这种事件涉及的粒子能量较低,但可产生高得多的剂量。在最强烈的太阳粒子事件中,后者的剂量在几小时内可超过几个 Gy,因此非随机效应是一个主要问题。为了确定适当的屏蔽条件,以遵守各航天机构规定的剂量限制,必须将所考虑的器官/组织的吸收剂量乘以相应的相对生物效应(RBE),这是一个复杂的量,取决于多个因素,包括粒子类型和能量、所考虑的生物效应、效应水平(以及吸收剂量)等。有几项研究只考虑了 RBE 与粒子类型的关系,而在本研究中,我们开发并应用了一种新方法,通过 FLUKA Monte Carlo 传输代码与 BIANCA 生物物理模型之间的接口,我们还考虑了 RBE 与粒子能量和吸收剂量的关系。此外,我们还在所考虑的 SPE 光谱中加入了比质子更重的原生粒子,而这在许多研究中都被忽略了。这种方法随后被应用于 2003 年 10 月的 SPE(太阳周期 23 中最强烈的 SPE,也被称为 "万圣节事件")和 2005 年 1 月的事件,后者的特点是通量较低,但光谱较硬,即粒子能量较高。这项工作表明,如果将 BIANCA 模型与辐射传输代码连接起来,就可以用来计算与太阳粒子事件相关的 RBE 值。更广泛地说,这项工作强调了在计算当量剂量时考虑 RBE 与粒子能量和剂量相关性的重要性。
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来源期刊
ACS Applied Bio Materials
ACS Applied Bio Materials Chemistry-Chemistry (all)
CiteScore
9.40
自引率
2.10%
发文量
464
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