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绝对重力测量的精度主要受振动噪声的限制. 振动补偿是一种简单可行的振动噪声处理方法, 它通过传感器探测振动噪声来对测量结果进行修正. 现阶段对于不同传感器的振动补偿性能缺乏系统的分析与评估, 仅停留在应用阶段. 本文从理论出发分析了传感器性能对补偿效果的影响, 并通过实验评估了不同振动环境下不同传感器的振动补偿性能. 实验结果显示, 采用低噪声地震计的振动补偿效果主要受带宽和量程的限制, 在安静环境下可实现优于百微伽的单次测量标准差, 但补偿效果随振动噪声高频成分的增强而降低, 在动态环境下地震计则受量程限制而无法工作. 采用加速度计的振动补偿效果主要受分辨率的限制, 在复杂和动态环境下均可实现毫伽量级的单次测量标准差. 本文为振动补偿技术应用于绝对重力测量提供了振动传感器选型的理论和实践依据, 有望为振动补偿技术的进一步发展提供技术支撑.Absolute gravity measurement refers to the measurement of the absolute value of gravitational acceleration ( g, approximately 9.8 m/s 2). The precision of absolute gravity measurement is limited mainly by vibration noises. Vibration correction is a simple and feasible way to deal with vibration noises, which corrects the measurement results by detecting vibration noises with a sensor. At present, the vibration correction performance of different sensors lacks systematic analysis and evaluation. In this paper, the theoretical analysis of how the sensor characteristics affect the correction performance is carried out. The vibration correction performances of three sensors, two different seismometers and one accelerometer, are evaluated experimentally in the three cases with different vibration noises. The experimental results show that the correction precision obtained by using low-noise seismometer is limited mainly by its bandwidth and range. In case I i.e. the quiet environment, the standard deviation of corrected results obtained by using both seismometers can reach tens of μGal (1 μGal = 10 –8m/s 2), which is close to that obtained by using an ultra-low-frequency vibration isolator. However, in case II i.e. the noisy environment, the standard deviation of corrected results obtained by both seismometers increase to hundreds of μGal due to the enhancement of high-frequency vibration components. This means that the correction performances of both seismometers deteriorate, and the performance of seismometer with narrower bandwidth turns even worse. Moreover, two seismometers cannot even work in case III with stronger vibration noises due to the range limitation. On the other hand, the correction precision obtained by using accelerometer is affected mainly by its resolution which is on the order of mGal (1mGal = 10 –5m/s 2). Its bandwidth can reach hundreds of or even thousands of hertz and its range is generally over ±2 g, which is large enough to meet the needs for noisy and dynamic applications. In case I, the standard deviation after correction with accelerometer is larger than that before correction. This is because the intensity of vibration noises in this case is close to or even smaller than the self-noise of accelerometer so that it could not be detected effectively by accelerometer. In case II, the resolution of accelerometer is sufficient to detect the vibration noises effectively. The standard deviation of the results is reduced from 2822 μGal to 1374 μGal after correction with accelerometer, and equal to a precision of 0.1 mGal after 100 drops. In case III where the amplitude of vibration noise rises to 0.1 m/s 2and seismometer cannot work, the accelerometer could still achieve a precision of 0.3 mGal after 100 drops. The systematic deviation is corrected from –1158 mGal to –285 μGal and the standard deviation is reduced from 34 mGal to 3.3 mGal. Therefore, the low-noise seismometer is more suitable for vibration correction in a quiet environment with stable foundation, which could realize a standard deviation superior to hundreds of μGal, while the accelerometer is more appropriate for vibration correction in a complex or dynamic environment, which could achieve a standard deviation of mGal-level. Finally, the present results and analysis provide a theoretical guidance for selecting and designing the sensors in vibration correction applications.
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型号 自噪声 –3 dB带宽 量程 CMG-3ESP 低于NLNM (40 s ~ 16 Hz) 0.0083—50 Hz 5 mm/s CS60 低于NLNM (100 s ~ 15 Hz) 0.0167—80 Hz 10 mm/s (1 Hz) JN06D –115 ~ –120 $ \rm dB\cdot g/\sqrt{Hz} $ (0 ~ 100 Hz) DC ~1360 Hz ± 30 g 
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未补偿 地震计CMG 地震计CS60 加速度计JN06D 隔振SuperSpring 安静
地基系统偏差Δg/μGal –8 –9 –1 –75 3 单次标准差STD/μGal 120 71 66 578 68 嘈杂
地基系统偏差Δg/μGal 841 28 5 18 8 单次标准差STD/μGal 2822 511 289 1374 93 万向
悬架系统偏差Δg/μGal –1158415 –285 单次标准差STD/μGal 42793 3353 下载:
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