See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/257970896 Producing an intense collimated beam of sound via a nonlinear ultrasonic array Article in Journal of Applied Physics · June 2012 DOI: 10.1063/1.4729265 CITATION READS 1 1,629 4 authors, including: Martin Leo Smith John A. Scales Blindgoat Geophysics Colorado School of Mines 40 PUBLICATIONS 1,474 CITATIONS 124 PUBLICATIONS 3,677 CITATIONS SEE PROFILE Some of the authors of this publication are also working on these related projects: Current projects are both proprietary acoustic systems. View project tomography View project All content following this page was uploaded by John A. Scales on 29 May 2014. The user has requested enhancement of the downloaded file. SEE PROFILE Producing an intense collimated beam of sound via a nonlinear ultrasonic array Daniel Gibson, Martin Smith, John Scales, and Brian Zadler Citation: J. Appl. Phys. 111, 124910 (2012); doi: 10.1063/1.4729265 View online: http://dx.doi.org/10.1063/1.4729265 View Table of Contents: http://jap.aip.org/resource/1/JAPIAU/v111/i12 Published by the American Institute of Physics. Related Articles Controllable acoustic media having anisotropic mass density and tunable speed of sound Appl. Phys. Lett. 101, 061916 (2012) Tunable time-reversal cavity for high-pressure ultrasonic pulses generation: A tradeoff between transmission and time compression Appl. Phys. Lett. 101, 064104 (2012) Formation of collimated sound beams by three-dimensional sonic crystals J. Appl. Phys. 111, 104910 (2012) Contribution of dislocation dipole structures to the acoustic nonlinearity J. Appl. Phys. 111, 074906 (2012) Microparticle trapping in an ultrasonic Bessel beam Appl. Phys. Lett. 99, 233704 (2011) Additional information on J. Appl. Phys. Journal Homepage: http://jap.aip.org/ Journal Information: http://jap.aip.org/about/about_the_journal Top downloads: http://jap.aip.org/features/most_downloaded Information for Authors: http://jap.aip.org/authors Downloaded 01 Sep 2012 to 138.67.128.67. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions JOURNAL OF APPLIED PHYSICS 111, 124910 (2012) Producing an intense collimated beam of sound via a nonlinear ultrasonic array Daniel Gibson,1,2 Martin Smith,3 John Scales,1 and Brian Zadler4 1 Department of Physics, Colorado School of Mines, Golden, Colorado 80401-1887, USA Systems Biology, Harvard Medical School, 200 Longwood Ave, Warren Alpert 536, Boston, Massachusetts 02115, USA 3 Blindgoat Geophysics, 2022 Quimby Mtn. Rd., Sharon, Vermont 05065, USA 4 Applied Research Associates, Inc., 7921 Shaffer Parkway, Littleton, Colorado 80127, USA 2 (Received 16 November 2011; accepted 14 May 2012; published online 26 June 2012) We have designed and built an ultrasonic parametric array with an emphasis on creating an intense, collimated beam of low frequency sound. With this device, we can insonify a small area of ground or a small target at range and induce vibrations. These vibrations can be synchronously detected with any stand-off device such as a laser-Doppler vibrometer or the millimeter wave vibrometer we describe in Smith et al. [J. Appl. Physics 108, 024902 (2010)]. Despite nonlinear conversion losses, the array produces sound pressure levels in excess of 90 dB at 1 kHz, 1.5 m in C 2012 American Institute of Physics. front of the array using 25 low-cost 40 KHz transducers. V [http://dx.doi.org/10.1063/1.4729265] INTRODUCTION The goal of this work is to produce an intense, collimated beam of low-frequency (200 Hz 1000 Hz) sound that can be used to insonify (i.e., couple sound into) as small a target area as possible. One approach to producing such a beam is to use a linear array of low-frequency sources in an end-fire configuration. The angular width, d, of a monochromatic beam is approximately2 k d¼ ; L (1) where k is wavelength and L is the length of the array. Assuming a speed of sound around 343 m=s, a 5 beamwidth we would need an array about 11k long. At 1000 Hz, a 5 array would be 3.8 m long, while at 500 Hz, it would be 7.5 m long. A linear array larger than 3 m would be cumbersome, space-consuming, and difficult to manipulate. A lighter, more compact system would allow the array to be mounted on the front of a vehicle where it may, for example, be used in land mine detection. Such a system could exploit parametric array technology3–5 which allows the replacement of a physical array by a virtual array created by nonlinear downconversion of intense sonic beams. Stepping through an example, Figure 1 diagrams the process approximately as it occurs in the specific parametric array used in this project. The array emits two co-propagating beams whose difference frequency is the desired low-frequency. When the signals are of high enough amplitude, their propagation in the interaction zone is non-linear. This is described by the Khokhlov-Zabolotskaya-Kuznetsov (KZK) equation, which takes into account nonlinearity, absorption, and diffraction.6 In first-order nonlinearity, the output signals consist of the two input signals, their sum and difference, and harmonics 0021-8979/2012/111(12)/124910/4/$30.00 of the two input signals. The output frequencies include x1 ; x2 ; ðx1 x2 Þ; ðx1 þ x2 Þ; 2x1 ; 2x2 , etc. The distribution of output energy over the various frequency components is sensitive to the drive level, with higher harmonics growing in amplitude as drive increases. In our tests, we used a source waveform constructed from two sinusoidal terms. The drive level was kept below the level at which higher harmonics (see Figure 7 below) predominate and the drive duration was kept short enough to avoid excessive transducer heating, typically a few seconds of signal. (In Ref. 1, we show that our millimeter wave interferometer can achieve 1 lm resolution given 1 s of signal.) In our work, the drive frequencies were 40.5 kHz and 41.5 kHz leading to an acoustic difference frequency of 1 kHz. The low-frequency energy is generated throughout the interaction volume and has precisely the phase distribution needed to function as an end-fire array along the axis of the interaction zone. This results in the ability to use a physically compact source element, the ceramic transducer array, to generate a collimated, low-frequency sonic beam that would otherwise require a much larger source element. The principal downside of the parametric array process is the typically low nonlinear conversion efficiency.6 In order to achieve as large an interaction zone as possible, the transducers must be driven as efficiently as possible at high power levels. We used an array of 25 medium-power (Airmar AR41) air-coupled transducers, each driven by a separate 60 W amplifier (Marchand PM221) through a handwound matching transformer tuned for each transducer (Amidon Ferrite Pot Core PC-1107-77). Figure 2 shows photos of the system during indoor testing. The amplifier bank is mounted below the transducer array along with the power control unit. The transducer= transformer units are connected to the amplifiers via a patch panel, making it easy to replace transducers. Transformers 111, 124910-1 C 2012 American Institute of Physics V Downloaded 01 Sep 2012 to 138.67.128.67. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions 124910-2 Gibson et al. FIG. 1. In this system, each ultrasonic transducer is a cylindrical element 92 mm in diameter which produces an ultrasonic beam in the vicinity of its broad resonance. The nominal beam width of one transducer at 40 kHz is 14 . The transducer is driven with the sum of 40.5 kHz and 41.5 kHz sinusoidal signals. The transducer produces two ultrasonic beams, one at each frequency, of similar spatial characteristics. The zone where both beams have high intensity is shown as an elongated oval. mounted on the back of the transducers are used to obtain maximum power transfer from the amplifier to the transducer by matching the real component of the transducer’s electrical impedance (from 40:5 kHz to 41:5 kHz) to the amplifier’s ideal load of 4 X. The transducer behaves inductively at those frequencies, so capacitance is added to the circuit to minimize complex impedance in the amplifier’s load. TESTING First, in the lab, the amplitude of the difference frequency of 1 kHz was measured in a plane in front of the parametric array using an audio microphone. The input voltage to the amplifiers was kept constant at 1 V peak to peak. J. Appl. Phys. 111, 124910 (2012) FIG. 3. A thermal image of the parametric array in operation. The difference in temperature between the working transducers is likely attributable to imperfections in electrical impedance matching between the amplifiers and the transducers, as well as small differences in the transducers themselves. At this input voltage, the amplifiers draw approximately 5 A total. A thermal infrared image of the system in action is shown in Figure 3. The interaction zone of the ultrasonic frequencies can be characterized by the amplitude of the 1 kHz waveform along the axis of propagation. This was sampled in variable increments of distance in front of the array, ranging from 1 cm, where the slope of the amplitude is relatively high, to 150 cm, where the amplitude changes little with distance. The result is shown in Figure 4. The beam spreading is characterized by the angle of a 6 dB (full width at quarter maximum (FWQM)) contour in the direction transverse to propagation. FWQM ¼ ðPeak Amplitude 6 dBÞ: FIG. 2. Parametric array and millimeter wave interferometer on mobile, battery-powered cart. (2) FIG. 4. Amplitude of 1 kHz waveform as a function of position relative to the center of the parametric array. The peak amplitude is reached around 100 cm, were it stays relatively constant. Using a sound pressure level meter, we measured the 1 kHz sound pressure level (SPL) at 150 cm to be over 90 dB. In this plot, the measurements were made with a flat response microphone but with no absolute power capability. Thus, the vertical scale is relative to an arbitrary but fixed reference voltage. Downloaded 01 Sep 2012 to 138.67.128.67. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions 124910-3 Gibson et al. J. Appl. Phys. 111, 124910 (2012) FIG. 7. Far-field beam divergence measured outdoors at 10 m distance from the array. The resulting beam divergence is consistent with the near field measurements made in the laboratory. FIG. 5. Beam intensity in a horizontal plane in front of the array. The average beam width, 18 , is shown by blue lines. The data for a given distance in the direction of propagation (Figure 5) are interpolated via cubic splines, then solved for the FWQM. These are divided by two to give the average distance off-axis, and fit using a linear, least squares regression to give beam width as a function of axial distance. The slope of this result, m, is used to calculate the beam spreading havg ¼ 2 arctanðmÞ; which is shown as lines in a contour plot of the beam intensity as a function of distance. The beam spreading is approximately 18 (i.e., beam divergence approximately 9 ). Even though this result is measured in the near field, it is consistent with a coarse scan made at 10 m in field tests. This angle is larger than we had hoped for but still gives an array size roughly half that associated with a linear transducer array. Repeated measurements of the same spatial location varied within 1 dB, which is taken to be the precision of the measurement. The measurements far off-axis varied on a shorter timescale (that of the oscilloscope averaging time) as a result of low signal to noise ratio at low amplitude. We looked at the presence of higher order term in the response as the drive voltage increased (i.e., term associated with cubic, quartic, etc., nonlinearities). As can be seen in Fig. 6, the beat frequency is overtaken as higher harmonics begin to dominate the signal. These can be heard as distortion of the beat note. The transducers themselves can withstand much higher driver levels provided the duty cycle is short enough. Thus, in short burst mode, higher harmonics could be exploited to produce a variety of beat frequencies (the acoustic analog of 3-photon and higher processes.) Finally, we performed a coarse beam divergence measurement at 10 m distance (Figure 7). This far field measurement is in reasonable agreement with the beam width inferred from the detailed amplitude map shown in Figure 5 measured in the laboratory. CONCLUSION We have constructed an ultrasonic parametric array which provides a collimated beam of low-frequency sound from a compact device. Results demonstrate a nonlinear interaction zone of approximately 1 m within which the lowfrequency beat note is produced from the modulated ultrasonic signal, which is the sum of two nearby sinusoidal signals. Apart from the matching transformers, the system was built with off the shelf components and can be readily expanded to increase the total acoustic power. Field tests show that the array is still easily audible at over 100 m distance, while at 1:5 m the measured sound pressure level is over 90 dB. ACKNOWLEDGMENTS FIG. 6. Beat tone (i.e., second harmonic) generation is overtaken by higher harmonics which grow as powers greater than 2 of the driving amplitude. This is a field test of harmonic line strength at 10 m distance from the array. This work was partially supported under two grants from the Army Research Office (W911NF-07-1-0478 and W911NF-09-1-0533) and the U.S. Office of Naval Research as a Multi-disciplinary University Research Initiative on Downloaded 01 Sep 2012 to 138.67.128.67. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions 124910-4 Gibson et al. Sound and Electromagnetic Interacting Waves under Grant No. N00014-10-1-0958. 1 M. L. Smith, J. A. Scales, M. Weiss, and B. Zadler, J. Appl. Phys. 108, 024902 (2010). 2 J. E. Barger, in Handbook of Acoustics, edited by M. J. Crocker (Wiley, Hoboken, NJ, 1998). View publication stats J. Appl. Phys. 111, 124910 (2012) 3 P. Westervelt, J. Acoust. Soc. Am. 35, 535 (1963). M. Yoneyama, J. Fujimoto, Y. Kawamo, and S. Sasabe, “The audio spotlight: An application of nonlinear interaction of sound waves to a new type of loudspeaker design,” J. Acoust. Soc. Am. 73, 1532–1536 (1983). 5 F. J. Pompei, “The audio spotlight: Put sound wherever you want it,” J. Audio Eng. Soc. 47, 726–731 (1999). 6 R. T. Beyer, Nonlinear Acoustics (Naval Sea Systems Command, U.S., 1974). 4 Downloaded 01 Sep 2012 to 138.67.128.67. Redistribution subject to AIP license or copyright; see http://jap.aip.org/about/rights_and_permissions