Experimental characterization of Silicon Drift Detector for X-ray spectrometry: Comparison with theoretical estimation

被引:3
|
作者
Shanmugam, M. [1 ]
Acharya, Y. B. [1 ]
Vadawale, S. V. [1 ]
Mazumdar, H. S. [2 ]
机构
[1] Phys Res Lab, Ahmadabad, Gujarat, India
[2] Dharmsinh Desai Univ, Nadiad, Gujarat, India
关键词
Silicon Drift Detector; CSPA; Reverse saturation current; Ideality factor; Energy resolution; Equivalent noise charge; TEMPERATURE-DEPENDENCE; PERFORMANCE; SIMULATION; CHAMBER; DESIGN; GAP;
D O I
10.1016/j.measurement.2016.05.042
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
Reverse saturation current and the ideality factor (eta) are the main parameters that affect the performance of a radiation semiconductor detector in different space environmental conditions. We have measured both of these parameters for the Silicon Drift Detector (SDD) used as a radiation detector in the X-ray spectrometry for space borne applications having the active area of 40 mm(2) and 109 mm(2) with 450 mu m thick silicon. The measured reverse saturation current is compared with the theoretically estimated values using diode equation for various detector operating temperatures and shown that there is a strong dependence of reverse saturation current with ideality factor. Subsequently, using the reverse saturation current ratio method, the slope ratio for small area to the large area SDD is derived and compared with the theoretical slope ratio obtained using the measured ideality factor. It is shown that the slope ratios closely match with the diode equation of the form which has the ideality factor in both the product and exponential terms for these SDDs. The measured spectral energy resolution is similar to 150 eV at 5.9 keV for both small and large area SDDs when operated at -40 degrees C and -65 degrees C respectively. The noise performance of the spectrometer is also measured in terms of Equivalent Noise Charge (ENC) for various detector operating temperatures and shown that the value of ENC in rms noise electrons is minimal for the pulse shaping time of 3.3 mu s. (C) 2016 Elsevier Ltd. All rights reserved.
引用
收藏
页码:66 / 72
页数:7
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