A new method of evaluation of X-ray pulsar detector sensitivity

被引:0
|
作者
Hu Hui-jun [1 ]
Song Juan [1 ]
Shao Si-pei [1 ]
Liu Jin-sheng [1 ]
Wang Wen-cong [1 ]
机构
[1] Shan Dong Inst Space Elect Technol, Yantai 264670, Peoples R China
来源
FIFTH SYMPOSIUM ON NOVEL OPTOELECTRONIC DETECTION TECHNOLOGY AND APPLICATION | 2019年 / 11023卷
关键词
X-ray pulsar navigation; contour accumulation; detecting sensitivity; signal-to-noise ratio;
D O I
10.1117/12.2521915
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Detection sensitivity is an important indicator of the X-ray pulsar detector. In order to achieve the accuratesensitivity of the detector, a new method of calculate detection sensitivity is proposed calculation. Combining with the characteristics of X-ray pulsar radiation spectrum and detector spectral,classic pulse accumulation model is corrected.A new signal to noise ratio (SNR) calculation formula is deduced by using the new pulse accumulation model. Constructing a new variable Z, which has close relationship with SNR. Through setting the SNR, the analysis and simulation verification for detection sensitivity and confidence level can be made. Simulation verification shows that the monte carlo simulation result is consistent with the theoretical results, and the maximum deviation is only 5%, which is far less than the deviation caused by the space environment disturbance.
引用
收藏
页数:9
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