Measurements of the linear energy transfer spectra on the Mir orbital station and comparison with radiation transport models

被引:42
作者
Badhwar, GD
Konradi, A
Atwell, W
Golightly, MJ
Cucinotta, FA
Wilson, JW
Petrov, VM
Tchernykh, IV
Shurshakov, VA
Lobakov, AP
机构
[1] NASA,LANGLEY RES CTR,HIGH ENERGY PHYS BRANCH,HAMPTON,VA 23681
[2] MINIST HLTH,INST BIOMED PROBLEMS,DEPT SPACE RADIAT,MOSCOW 123007,RUSSIA
[3] NPO ENERGIA,KALININGRAD,RUSSIA
基金
美国国家航空航天局;
关键词
D O I
10.1016/1350-4487(95)00290-1
中图分类号
TL [原子能技术]; O571 [原子核物理学];
学科分类号
0827 ; 082701 ;
摘要
A tissue equivalent proportional counter designed to measure the linear energy transfer spectra (LET) in the range 0.2-1250 keV/mu m was flown in the Kvant module on the Mir orbital station during September 1994. The spacecraft was in a 51.65 degrees inclination, elliptical (390 x 402 km) orbit. This is nearly the lower limit of its flight altitude. The total absorbed dose rate measured was 411.3 +/- 4.41 mu Gy/day with an average quality factor of 2.44. The galactic cosmic radiation (GCR) dose rate was 133.6 mu Gy/day with a quality factor of 3.35. The trapped radiation belt dose rate was 277.7 mu Gy/day with an average quality factor of 1.94. The peak rate through the South Atlantic Anomaly was similar to 12 mu Gy/min and nearly constant from one pass to another. A detailed comparison of the measured LET spectra has been made with radiation transport models. The GCR results are in good agreement with model calculations; however, this is not the case for radiation belt particles and again points to the need for improving the AP8 omni-directional trapped proton models.
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页码:147 / &
页数:11
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