【摘 要】
：
The development decoding algorithms of two-dimensional cross strip anodes image readouts for applications in UV astronomy are described.We present results w
【机 构】
：
Xi'anInstituteofOpticsandPrecisionMechanicsofCAS,China
【出 处】
：
2014年光子与光学工程国际会议暨西部光子学学术会议
论文部分内容阅读
The development decoding algorithms of two-dimensional cross strip anodes image readouts for applications in UV astronomy are described.We present results with Monte Carlo simulation by GEANT4 toolkit,the results show that when the cross strip anode period is 0.5mm and the electrode width is 0.4mm,the spatial resolution accuracy is sufficient to reach better than 5 祄,the temporal resolution accuracy of the event detection can be as low as 100 ps.The influences of the cross strip detector parameters,such as the anode period,the width of anode fingers(electrode),the width of the charge footprint at the anode(determined by the distance and the field between the MCP and the anode),the gain of the MCP and equivalent noise charge(ENC)are also discussed.The development decoding algorithms and simulation results can be useful for the designing and performance improvement of future photon counting imaging detectors for UV Astronomy.
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