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EMI测量接收机作为电磁兼容测试中的关键仪器应用越来越广泛,但目前该类仪器的脉冲响应校准所用的标准源完全依赖于进口,国内尚无可替代的标准脉冲信号产生器。介绍一种用于EMI测量接收机脉冲响应校准的标准脉冲信号产生方法,首先建立标准脉冲信号的参数模型并对其进行数值分析和仿真,验证其符合CISPR 16-1-1标准的要求,之后搭建实验系统,利用标准脉冲信号生成软件控制任意脉冲信号发生器输出标准脉冲信号并对其进行补偿修正,获得符合CISPR 16-1-1标准要求的标准脉冲信号,该信号可用于EMI测量接收机脉冲响应的校准。 相似文献
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《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(6):2711-2722
Distributed X-ray pulsar-based navigation (DXNAV) is an effective method to realize earth-orbit satellite positioning under weak pulsar signal conditions. In this paper, we propose a new DXNAV method based on multiple information fusion. The DXNAV system principle and the pulse phase estimate Cramér-Rao lower bound are deduced. To suppress the calculation complexity and the error source, the X-ray pulsar photon time-of-arrival detected by each satellite is equivalently converted to the leading satellite directly using the inter-satellite link ranging and starlight angular distance measurement. A high precision estimate model of the pulse phase is built using pulsar standard profile, observed profile, and star-geocentric angular distance from distributed satellites. The estimated pulse phase is real-time supplied to the navigation system, which is established in the form of a deviation equation. The two-stage Kalman filter is designed to estimate the pulse phase in profile histogram bin step and the leader position in real-time step. Compared separately with the maximum likelihood phase estimate method and the celestial navigation method using only the star-geocentric angular distance, the simulation analysis shows that the estimation precisions of position and velocity are improved by 29% and 25%. 相似文献
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《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(2):1319-1330
In radiation detector signal processing, usually, the charge-sensitive preamplifier converts the small charge signal coming from the semiconductor-based detector into voltage form and then the signal is further amplified to measure the energy of the incoming radiation. The voltage pulse from a charge-sensitive preamplifier (CSPA) is amplified using a shaping amplifier which reduces the signal bandwidth. To achieve better energy resolution, precise measurement of the peak amplitude of shaping amplifier output is required. The signal processing methods are available in which the signal from the charge-sensitive preamplifier can be directly digitized using high-speed Analog to Digital Converters (ADC), and then further signal processing such as gain and shaping is carried out inside the Field Programmable Gate Arrays (FPGA). For multiple detector systems, digital signal processing methods are quite difficult to implement in Field Programmable Gate Arrays (FPGA). In this context, The development of an alternative technique is initiated that uses a charge-sensitive preamplifier, shaping amplifier, low sampling analog-to-digital converter, and FPGA, where LaGrange’s interpolation technique is implemented in FPGA to precisely measure the peak of the analog pulse. In this paper, the comparison of the proposed method with other pulse amplitude measurement techniques is discussed. Results show that the implemented technique gives similar energy resolution compared to digital pulse processing and standard peak detector-based techniques. 相似文献
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量子级联激光器具有体积小,重量轻,波长可调谐,以及光源能够覆盖中远红外和太赫兹波段等特点,使其在痕量气体检测、定向红外对抗、自由空间光通讯以及红外成像和光谱等领域有着广泛的应用。自从1994年第一个量子级联激光器问世以来,大功率、高电光效率以及室温下连续工作的量子级联激光器一直是人们追求的目标。首先介绍了量子级联激光器的有源层设计、波导设计和器件散热设计方面的研究进展;其次重点讨论了4 μm~5 μm 中波红外和
8 μm~12 μm长波红外高功率室温下连续量子级联激光器的发展和演变、以及大功率脉冲量子级联激光器研究情况;最后简要介绍了大功率量子级联激光器芯片的外延制备技术。 相似文献
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