Kolomenskiĭ A V, Petrov V M, Shafirkin A V
Aviakosm Ekolog Med. 1998;32(4):44-9.
A technique for calculating the SS MIR absorbed doses from the galactic cosmic rays, protons of the Earth's radiation belts and solar flares is described. Calculated daily doses for different compartments along the MIR main axis are compared with doses calculated for the location of board radiometer R-16 in various periods of solar activity. Maximal doses in MIR compartments (in the absence of phantom) were compared with the doses in referential depths of a spherical phantom representing the blood forming tissue, skin, enteric epithelium, and the absorbed dose in the dosimeter location. This comparison allows more precise estimation of radiation hazard to cosmonauts in space flight.
描述了一种用于计算来自银河宇宙射线、地球辐射带质子和太阳耀斑的太空站轨道复合体（SS MIR）吸收剂量的技术。将沿太空站轨道复合体主轴不同舱室的计算日剂量与在太阳活动不同时期为机载辐射计R - 16位置计算的剂量进行比较。比较了太空站轨道复合体舱室中的最大剂量（无体模时）与代表造血组织、皮肤、肠上皮的球形体模参考深度处的剂量以及剂量计位置的吸收剂量。这种比较有助于更精确地估计太空飞行中宇航员的辐射危害。
