CHARACTERIZATION OF THE RADIATION ENVIRONMENT BY LIULIN-TYPE SPECTROMETERS

被引:9
作者
Dachev, Ts. [1 ]
Spurny, F. [2 ]
Ploc, O. [2 ]
机构
[1] Bulgarian Acad Sci, Solar Terr Influences Inst, BU-1113 Sofia, Bulgaria
[2] Acad Sci Czech Republic, Inst Nucl Phys, Prague 18086, Czech Republic
关键词
CHANDRAYAAN-1; INSTRUMENT; DOSIMETRY; MODELS;
D O I
10.1093/rpd/ncq534
中图分类号
X [环境科学、安全科学];
学科分类号
08 ; 0830 ;
摘要
Liulin-type spectrometers can characterise the type of predominant particles and their energy in the radiation environment. The results from calibrations and space and aircraft experiments revealed that the most informative is by the shape of the deposited energy spectrum. Spectra generated by galactic cosmic rays (GCR) protons and their secondaries look like straight lines in the coordinates deposited energy/deposited per channel dose rate. The position of the maximum of the deposited energy spectra depends on the incident energy of the incoming protons. Spectra generated by relativistic electrons in the outer radiation belt have a maximum in the first channels. For higher energy depositions, these spectra are similar to the GCR spectra. All types of spectra have a knee close to 6.3 MeV of deposited energy, which corresponds to the stopping energy of protons in the detector.
引用
收藏
页码:680 / 683
页数:4
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