本文介绍了一种基于2 bit阶梯波时间调制(step-wave time-modulation,SWTM)的高精度幅度调控方法。首先建立了2 bit SWTM理论模型,分析了阶梯波形对射频信号时间调制的幅度调控精度影响;然后设计了2 bit SWTM电路,进行了高精度幅度调控...本文介绍了一种基于2 bit阶梯波时间调制(step-wave time-modulation,SWTM)的高精度幅度调控方法。首先建立了2 bit SWTM理论模型,分析了阶梯波形对射频信号时间调制的幅度调控精度影响;然后设计了2 bit SWTM电路,进行了高精度幅度调控实验。测试结果表明,在40 MHz信号带宽下,该2 bit SWTM电路实现了0~31.75 dB衰减动态范围的7 bit幅度调控,误差范围小于±(0.1+0.8%AS)dB,均方根误差为0.07 dB。展开更多
This paper proposes a single channel, 6-bit 230-MS/s asynchronous successive approximation register analog-to-digital converter （ADC） in an SMIC 65 nm CMOS technology. Through adopting the modified 2 bits/stage asyn...This paper proposes a single channel, 6-bit 230-MS/s asynchronous successive approximation register analog-to-digital converter （ADC） in an SMIC 65 nm CMOS technology. Through adopting the modified 2 bits/stage asynchronous control logic, the presented ADC actualizes a peak 40.90-dB spurious-free dynamic range and 29.05-dB signal-to-noise and distortion ratio at 230-MS/s sampling rate. Utilizing the dynamic comparator without the preamplifier, this work attains low-power design with only 0.93 mW power consumption and accomplishes a figure of merit of 174.67 fJ/step at 1 V supply voltage.展开更多
Chang＇E-3 spacecraft was orbiting the Moon from December 6 14, 2013, and very long baseline interferometry （VLBI） observations were performed to improve the accuracy of its orbit determination. In the process of re...Chang＇E-3 spacecraft was orbiting the Moon from December 6 14, 2013, and very long baseline interferometry （VLBI） observations were performed to improve the accuracy of its orbit determination. In the process of recording VLBI raw data, 2 bits quantization was implemented. Interesting phenomenon was that signal-to-noise ratio （SNR） of each VLBI station experienced periodical change and had large variation on amplitude while in the Moon＇s orbit, whereas SNR kept in a stable level after Chang＇E-3 landed on the Moon. Influence of varying elevation angle on SNR was analyzed and compensation of 2 bits quantization harmonics to SNR calculation was investigated. Most importantly, telescope system noise temperature increase caused by the Moon was computed along the time of Chang＇E-3 orbiting the Moon, and well matched SNR changing trend in terms of correlation coefficients.展开更多
文摘本文介绍了一种基于2 bit阶梯波时间调制(step-wave time-modulation,SWTM)的高精度幅度调控方法。首先建立了2 bit SWTM理论模型,分析了阶梯波形对射频信号时间调制的幅度调控精度影响;然后设计了2 bit SWTM电路,进行了高精度幅度调控实验。测试结果表明,在40 MHz信号带宽下,该2 bit SWTM电路实现了0~31.75 dB衰减动态范围的7 bit幅度调控,误差范围小于±(0.1+0.8%AS)dB,均方根误差为0.07 dB。
基金supported by the National Science Foundation for Young Scientists of China(No.61306029)the National High Technology Research and Development Program of China(No.2013AA014103)
文摘This paper proposes a single channel, 6-bit 230-MS/s asynchronous successive approximation register analog-to-digital converter （ADC） in an SMIC 65 nm CMOS technology. Through adopting the modified 2 bits/stage asynchronous control logic, the presented ADC actualizes a peak 40.90-dB spurious-free dynamic range and 29.05-dB signal-to-noise and distortion ratio at 230-MS/s sampling rate. Utilizing the dynamic comparator without the preamplifier, this work attains low-power design with only 0.93 mW power consumption and accomplishes a figure of merit of 174.67 fJ/step at 1 V supply voltage.
基金supported by the National Natural Science Foundation of China(Nos.11473059,11273049,11403082)
文摘Chang＇E-3 spacecraft was orbiting the Moon from December 6 14, 2013, and very long baseline interferometry （VLBI） observations were performed to improve the accuracy of its orbit determination. In the process of recording VLBI raw data, 2 bits quantization was implemented. Interesting phenomenon was that signal-to-noise ratio （SNR） of each VLBI station experienced periodical change and had large variation on amplitude while in the Moon＇s orbit, whereas SNR kept in a stable level after Chang＇E-3 landed on the Moon. Influence of varying elevation angle on SNR was analyzed and compensation of 2 bits quantization harmonics to SNR calculation was investigated. Most importantly, telescope system noise temperature increase caused by the Moon was computed along the time of Chang＇E-3 orbiting the Moon, and well matched SNR changing trend in terms of correlation coefficients.
