Radiation Effects on the Silicon Semiconductor Detectors for the ASTRO-H Mission
Radiation Effects on the Silicon Semiconductor Detectors for the ASTRO-H Mission
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DOI:
10.1016/j.nima.2012.05.088
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发表时间:
2013-01
影响因子:
1.4
通讯作者:
Katsuhiro Hayashi;I. Park;Kyohei Dotsu;I. Ueno;S. Nishino;M. Matsuoka;H. Yasuda;Y. Fukazawa;T. Ohsugi;T. Mizuno;H. Takahashi;M. Ohno;S. Endo;Takaaki Tanaka;H. Tajima;M. Kokubun;S. Watanabe;Tadayuki Takahashi;K. Nakazawa;Y. Uchihori;H. Kitamura
中科院分区:
文献类型:
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作者:
Katsuhiro Hayashi;I. Park;Kyohei Dotsu;I. Ueno;S. Nishino;M. Matsuoka;H. Yasuda;Y. Fukazawa;T. Ohsugi;T. Mizuno;H. Takahashi;M. Ohno;S. Endo;Takaaki Tanaka;H. Tajima;M. Kokubun;S. Watanabe;Tadayuki Takahashi;K. Nakazawa;Y. Uchihori;H. Kitamura
Hard X-ray Imager (HXI) and Soft Gamma-ray Detector (SGD) onboard the 6th Japanese X-ray satellite, ASTRO–H, utilize double-sided silicon strip detectors (DSSD) and pixel array-type silicon sensors (Si-pad), respectively. The DSSD with a 3.4cm×3.4cm area has an imaging capability in the lower energy band for the HXI covering 5–80keV. The Si-pad consists of 16×16 pixels with a 5.4cm×5.4cm area and measures a photon direction with the Compton kinematics in 10–600keV. Since the ASTRO–H will be operated in a low earth orbit, these detectors will be damaged by irradiation of cosmic-ray protons mainly in the South Atlantic Anomaly. In order to evaluate damage effects of the sensors, we have carried out irradiation tests with 150MeV proton beams and60Co gamma-rays with a total dose of 10–20 years irradiation level. In both experiments, the leakage current has increased by ∼0.2−−1.1nA/cm2under an expected operation temperature at −15°C, which resulted in the noise level within a tolerance of 20 years. In this report, we present a summary of the basic performance of silicon detectors, and radiation effects on them by the irradiation tests.