Physical Constraints of High Resolution Acoustic Imaging in the 50 Hz - 15 kHz Frequency Range

R. C. Aylward
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Abstract

Identification and spatial detection of low frequency airborne sound sources, 50 Hz - 15 kHz, both generative and reflective, is not a clear cut task. The purpose of this paper is to give an overview of the physics and related mathematics that govern and acoustic imaging system. Most of the theory is borrowed from optics and is now applied to the field of acoustics. The paper highlights the relationship between wavelength and effective aperture. Other important issues addressed are field depth and resolving power, i.e. the point spread function. Chromatic aberration, spectral aberration, due to refraction is also discussed. The last issue is the comparison of a mirror/lens approach vs. a microphone array approach. Finally the paper concludes with a discussion of two applications. First it looks at architectural acoustics and second at a low frequency acoustic radar/sonar application.
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50hz - 15khz频率范围内高分辨率声成像的物理约束
识别和空间检测低频机载声源,50赫兹- 15千赫,生成和反射,并不是一个明确的任务。本文的目的是概述控制声成像系统的物理和相关数学。大部分理论是从光学借鉴来的,现在应用于声学领域。重点讨论了波长与有效孔径之间的关系。其他重要的问题是景深和分辨力,即点扩散函数。还讨论了折射引起的色差、光谱像差。最后一个问题是镜面/透镜方法与麦克风阵列方法的比较。最后讨论了两种应用。首先是建筑声学,其次是低频声学雷达/声纳应用。
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