Baranov D G, Dergachev V A, Gagarin Yu F, Lyagushin V I, Nymmik R A, Panasyuk M I, Solov'ev A V, Yakubovskii E A
Ioffe Physico-Technical Institute, Russian Academy of Sciences, St. Petersburg, Russia.
Radiat Meas. 2002 Oct;35(5):423-31. doi: 10.1016/s1350-4487(02)00073-2.
The results are presented of measurements high-energy particles in a customary manned space station orbit (a 350-450-km altitude, a 51.6 degrees inclination; Salyut-6 and 7, MIR). The particles were recorded by the chambers composed of the Lavsan (polyethyleneterephtalate) solid-state nuclear track detector layers mounted outside a spacecraft for 1-3 years. A high resolution has been attained in the charge and energy spectra of 30-200 MeV/n Fe group particles. The results of measuring the particle fluxes in the space station orbits are used to restore the initial particle energy spectra in terms of the models that describe the galactic and solar cosmic rays and their penetration to the Earth's magnetosphere. The analysis demonstrates a high effectiveness of the described methods when applied to quite a number of space physics problems.
给出了在常规载人空间站轨道（高度350 - 450公里，倾角51.6度；礼炮6号和7号、和平号空间站）中高能粒子的测量结果。粒子由安装在航天器外部1 - 3年的由拉弗桑（聚对苯二甲酸乙二酯）固态核径迹探测器层组成的探测器记录。在30 - 200 MeV/n铁族粒子的电荷和能谱方面已达到高分辨率。利用空间站轨道中粒子通量的测量结果，根据描述银河宇宙射线和太阳宇宙射线及其进入地球磁层的模型来恢复初始粒子能谱。分析表明，所描述的方法应用于许多空间物理问题时具有很高的有效性。
