Reitz G
DLR, Institut für Luft- und Raumfahrtmedizin, Abteilung Strahlenbiologie, Linder Hohe, D-51140 Köln, Germany.
Radiat Meas. 2001 Jun;33(3):341-6. doi: 10.1016/s1350-4487(00)00153-0.
Detector packages consisting of thermoluminescence detectors (TLD), nuclear emulsions and plastic track detectors were exposed at identical positions inside MIR space station and on shuttle flights inside Spacelab and Spacehab during different phases of the solar cycle. The objectives of the investigations are to provide data on charge and energy spectra of heavy ions, and the contribution of events with low-energy deposit (protons, electrons, gamma, etc.) to the dose, as well as the contribution of secondaries, such as nuclear disintegration stars and neutrons. For neutron dosimetry 6LiF (TLD600) and 7LiF (TLD700) chips were used both of which have almost the same response to gamma rays but different response to neutrons. Neutrons in space are produced mainly in evaporation and knock-on processes with energies mainly of 1-10 MeV and up to several 100 MeV, respectively. The energy spectrum undergoes continuous changes toward greater depth in the attenuating material until an equilibrium is reached. In equilibrium, the spectrum is a wide continuum extending down to thermal energies to which the 6LiF is sensitive. Based on the difference of absorbed doses in the 6LiF and 7LiF chips, thermal neutron fluxes from 1 to 2.3 cm-2 s-1 are calculated using the assumption that the maximum induced dose in TLD600 for 1 neutron cm-2 is 1.6 x 10(-10) Gy (Horowitz and Freeman, Nucl. Instr. and Meth. 157 (1978) 393). It is assumed that the flux of high-energy neutrons is at least of that quantity. Tissue doses were calculated taking as a mean ambient absorbed dose per neutron 6 x10(-12) Gy cm2 (for a10 MeV neutron). The neutron equivalent doses for the above-mentioned fluxes are 52 micro Gy d-1 and 120 micro Gy d-1. In recent experiments, a personal neutron dosimeter was integrated into the dosimeter packages. First results of this dosimeter which is based on nuclear track detectors with converter foils are reported. For future measurements, a scintillator counter with anticoincidence logic is under development.
由热释光探测器(TLD)、核径迹乳胶和塑料径迹探测器组成的探测器组件,在太阳活动周期的不同阶段,于和平号空间站内部以及航天飞机搭载的太空实验室和太空舱内的相同位置进行了暴露实验。研究目的是获取重离子的电荷和能谱数据,以及低能量沉积事件(质子、电子、γ射线等)对剂量的贡献,还有诸如核裂变星和中子等次级粒子的贡献。对于中子剂量测定,使用了6LiF(TLD600)和7LiF(TLD700)芯片,它们对γ射线的响应几乎相同,但对中子的响应不同。太空中的中子主要产生于蒸发和碰撞过程,其能量主要分别为1 - 10 MeV和高达几百MeV。能谱在衰减材料中朝着更大深度不断变化,直至达到平衡。在平衡状态下,能谱是一个宽广的连续谱,延伸至热中子能量范围,6LiF对该范围敏感。基于6LiF和7LiF芯片中吸收剂量的差异,假设TLD600中每1个中子/cm²的最大诱导剂量为1.6×10⁻¹⁰ Gy(霍洛维茨和弗里曼,《核仪器与方法》157卷(1978年)393页),计算出热中子通量为1至2.3 cm⁻² s⁻¹。假设高能中子通量至少为该数量。以每个中子6×10⁻¹² Gy cm²(对于10 MeV中子)作为平均环境吸收剂量,计算出组织剂量。上述通量的中子当量剂量分别为52 μGy d⁻¹和120 μGy d⁻¹。在最近的实验中,一个个人中子剂量计被集成到剂量计组件中。报告了基于带有转换箔的核径迹探测器的该剂量计的初步结果。对于未来的测量,正在开发一种带有反符合逻辑的闪烁计数器。