首页> 外文会议>International Congress on Sound and Vibration >EXPERIMENTAL STUDIES OF ACOUSTIC PROPAGATION CHARACTERISTICS IN THE LOW PRESSURE OF CO_2 AT-MOSPHERE BASED ON THE FIBER OPTICAL SENSING TECHNOLOGY
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EXPERIMENTAL STUDIES OF ACOUSTIC PROPAGATION CHARACTERISTICS IN THE LOW PRESSURE OF CO_2 AT-MOSPHERE BASED ON THE FIBER OPTICAL SENSING TECHNOLOGY

机译:基于纤维光学传感技术的CO_2型互压性声学传播特性的实验研究

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In order to meet the demand of correction for thermal model of future Mars probe and validation of performance of Mars probe in extreme environments, we need to simulate the Mars environment in the ground. The wind speed measurement is very important for the Mars environment simulation and test. The atmosphere on Mars is much different from that on earth, that the pressure ranges from 600 Pa to 1000 Pa and the dominant constituent is CO_2. In Earth, the fiber optical sensing technique has been successfully applied for the sound velocity measurement. It is interesting to study whether the fiber optical sensing technique could be used in Mars environment. The speed of sound in the low pressure of CO_2 atmosphere has been derived theoretically by assuming that the idea gas law applies to this case. We have carried out experiments to measure the speed of sound in a space environment simulator which we can fill with air or pure CO_2 respectively. The pressure in the chamber is adjusting from 10~5 Pa to 600 Pa with different intervals, the pitch-catch method using four pairs of piezoelectric actuators and sensors, with central frequencies being 21, 25, 34, and 40 kHz respectively, is applied to generate acoustic signals. We use the fiber optical sensing technology to measure the ultrasound waves speed at different pressures. The experimental results show that the fiber optical sensing technique can be applied for the sound velocity measurement in the low pressure of CO_2 atmosphere, the speed of sound rarely varies with the pressure in the range from 10~5 Pa and 600 Pa, while it depends on the composition of the gas and the temperature.
机译:为了满足未来火星热模型的校正需求,并在极端环境中验证火星探针的性能,我们需要在地面上模拟火星环境。风速测量对于MARS环境模拟和测试非常重要。火星上的气氛与地球上的大气有很大差异,压力范围从600 pa到1000 pa和主导成分是co_2。在地球中,纤维光学传感技术已成功应用于声速测量。研究是否可以在火星环境中使用光纤光学传感技术是有趣的。通过假设想法气体法适用于这种情况,从理论上推导出CO_2气氛低压的声速。我们已经进行了实验来测量空间环境模拟器中的声速,我们可以分别填充空气或纯CO_2。腔室中的压力从10〜5Pa到600Pa以不同的间隔调节,使用四对压电致动器和传感器的间距捕获方法分别具有21,25,34和40kHz的中央频率产生声学信号。我们使用光纤光学传感技术测量不同压力的超声波速度。实验结果表明,光纤光学传感技术可以应用于CO_2大气层的低压中的声速测量,随着10〜5Pa和600Pa的压力,声音速度很少变化,而这取决于在气体和温度的组成上。

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