Absorbed dose of secondary neutrons from galactic cosmic rays inside the International Space Station

被引：15

作者：

Getselev, I

Rumin, S

Sobolevsky, N

Ufimtsev, M

Podzolko, M

机构：

[1] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119992, Russia

[2] Russian Acad Sci, Inst Nucl Res, Moscow, Russia

[3] Moscow MV Lomonosov State Univ, Dept Comp Sci, Moscow 119992, Russia

来源：

SPACE LIFE SCIENCES: RADIATION RISK ASSESSMENT AND RADIATION MEASUREMENT IN LOW EARTH ORBIT | 2004年 / 34卷 / 06期

关键词：

D O I：

10.1016/j.asr.2004.04.002

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

In this paper, we present the results of Monte-Carlo simulations of the flux and energy spectra of neutrons generated as a result of galactic cosmic ray proton interactions with the material of International Space Station (ISS) inside Zvezda Service Module, the Airlock between Russian and USA segments and one of Russian Research Modules for a full configuration of ISS. Calculations were made for ISS orbit for the energy ranges < 10 and > 10 MeV for both maximum and minimum of solar activity. To test the accuracy of the calculations the same simulations were made for MIR orbital station and for CORONAS-I satellite and compared with the results of measurements. Calculated and measured fluxes are in reasonable agreement. (C) 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：1429 / 1432

页数：4

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