O'Sullivan D
Dublin Institute for Advanced Studies, Astrophysics Section, 5 Merrion Square, Dublin 2, Ireland.
Radiat Prot Dosimetry. 2007;125(1-4):407-11. doi: 10.1093/rpd/ncm317. Epub 2007 Sep 9.
Several investigations of the radiation field at aircraft altitudes have been undertaken during solar cycle 23 which occurred in the period 1993-2003. The radiation field is produced by the passage of galactic cosmic rays and their nuclear reaction products as well as solar energetic particles through the Earth's atmosphere. Galactic cosmic rays reach a maximum intensity when the sun is least active and are at minimum intensity during solar maximum period. During solar maximum an increased number of coronal mass ejections and solar flares produce high energy solar particles which can also penetrate down to aircraft altitudes. It is found that the very complicated field resulting from these processes varies with altitude, latitude and stage of solar cycle. By employing several active and passive detectors, the whole range of radiation types and energies were encompassed. In-flight data was obtained with the co-operation of many airlines and NASA. The EURADOS Aircraft Crew in-flight data base was used for comparison with the predictions of various computer codes. A brief outline of some recent studies of exposure to radiation in Earth orbit will conclude this contribution.
在1993年至2003年发生的太阳活动周期23期间,人们对飞机高度的辐射场进行了多项调查。辐射场是由银河宇宙射线及其核反应产物以及太阳高能粒子穿过地球大气层而产生的。当太阳活动最小时,银河宇宙射线达到最大强度,而在太阳活动极大期则处于最小强度。在太阳活动极大期,日冕物质抛射和太阳耀斑数量增加,会产生高能太阳粒子,这些粒子也能穿透到飞机高度。研究发现,这些过程产生的非常复杂的辐射场会随高度、纬度和太阳活动周期阶段而变化。通过使用多种主动和被动探测器,涵盖了所有类型和能量的辐射。飞行数据是在多家航空公司和美国国家航空航天局的合作下获得的。欧洲辐射剂量学组织(EURADOS)的机组人员飞行数据库用于与各种计算机代码的预测结果进行比较。本文将以对地球轨道辐射暴露的一些最新研究的简要概述作为结束。