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长期暴露对太空辐射风险相加性的可能影响。

Possible effects of protracted exposure on the additivity of risks from space radiations.

作者信息

Curtis S B

机构信息

Fred Hutchinson Cancer Research Center, Seattle, WA 98104, USA.

出版信息

Adv Space Res. 1996;18(1-2):41-4. doi: 10.1016/0273-1177(95)00787-f.

Abstract

Conventional radiation risk assessments are presently based on the additivity assumption. This assumption states that risks from individual components of a complex radiation field involving many different types of radiation can be added to yield the total risk of the complex radiation field. If the assumption is not correct, the summations and integrations performed to obtain the presently quoted risk estimates are not appropriate. This problem is particularly important in the area of space radiation risk evaluation because of the many different types of high- and low-LET radiation present in the galactic cosmic ray environment. For both low- and high-LET radiations at low enough dose rates, the present convention is that the addivity assumption holds. Mathematically, the total risk, Rtot is assumed to be Rtot = summation (i) Ri where the summation runs over the different types of radiation present. If the total dose (or fluence) from each component is such that the interaction between biological lesions caused by separate single track traversals is negligible within a given cell, it is presently considered to be reasonable to accept the additivity assumption. However, when the exposure is protracted over many cell doubling times (as will be the case for extended missions to the moon or Mars), the possibility exists that radiation effects that depend on multiple cellular events over a long time period, such as is probably the case in radiation-induced carcinogenesis, may not be additive in the above sense and the exposure interval may have to be included in the evaluation procedure. It is shown, however, that "inverse" dose-rate effects are not expected from intermediate LET radiations arising from the galactic cosmic ray environment due to the "sensitive-window-in-the-cell-cycle" hypothesis.

摘要

传统的辐射风险评估目前基于可加性假设。该假设表明,复杂辐射场中涉及多种不同类型辐射的各个组成部分的风险可以相加,以得出复杂辐射场的总风险。如果该假设不正确,那么为获得当前引用的风险估计值而进行的求和与积分就不合适。由于银河宇宙射线环境中存在多种不同类型的高传能线密度和低传能线密度辐射,这个问题在空间辐射风险评估领域尤为重要。对于低剂量率下的低传能线密度和高传能线密度辐射,目前的惯例是可加性假设成立。从数学角度来看,总风险Rtot被假定为Rtot = ∑(i) Ri,其中求和涵盖存在的不同类型辐射。如果每个组成部分的总剂量(或注量)使得在给定细胞内由单独单径迹穿越引起的生物损伤之间的相互作用可忽略不计,那么目前认为接受可加性假设是合理的。然而,当暴露持续许多细胞倍增时间(对于前往月球或火星的长期任务就是这种情况)时,存在这样一种可能性,即依赖于长时间内多个细胞事件的辐射效应,比如辐射诱发癌症可能就是这种情况,在上述意义上可能不是可加的,并且暴露间隔可能必须纳入评估程序。然而,研究表明,由于“细胞周期中的敏感窗口”假说,预计银河宇宙射线环境产生的中等传能线密度辐射不会出现“反”剂量率效应。

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