Physics · Book 4 · Bachelor Year 2

University Physics — Year 2

University Physics — Year 2 · Bachelor Year 2

7Sound Waves in Fluids

Count the seconds between the flash and the thunder and divide by three: that is the distance in kilometres. Sound crosses air at a third of a kilometre per second, water at a kilometre and a half, and an ultrasound scanner times the echoes from inside the body to a millionth of a second to draw its picture. This chapter applies the fluid mechanics of Chapters 3 and 2 to a fluid at rest disturbed by a small pressure ripple, and finds the d’Alembert equation again: the speed of sound, what carries the energy, how loud is loud, how sound spreads in space, and why a siren changes pitch as it passes.

7.1 The acoustic approximation

Definition 7.1 (Acoustic perturbation)

A fluid at rest, of uniform pressure P0P_0 and density ρ0\rho_0, is disturbed: P=P0+p(M,t)P = P_0 + p(M, t), ρ=ρ0+ρ1(M,t)\rho = \rho_0 + \rho_1(M, t), velocity v(M,t)\vect v(M, t). The acoustic approximation keeps only the first order in the small quantities pp (the overpressure, or acoustic pressure), ρ1\rho_1 and v\vect v: pP0|p| \ll P_0, ρ1ρ0|\rho_1| \ll \rho_0, vcv \ll c, and the transformation undergone by each fluid particle is so fast that it exchanges no heat: it is isentropic, with the compressibility χS=1ρ(ρP)S\chi_S = \frac1\rho\bigl(\frac{\partial\rho}{\partial P}\bigr)_S. Gravity is neglected.

Theorem 7.2 (Sound waves)

To first order, Euler’s equation, mass conservation and the isentropic law read

ρ0vt=gradp,ρ1t+ρ0divv=0,ρ1=ρ0χSp,\rho_0\frac{\partial\vect v}{\partial t} = -\operatorname{\vect{grad}}p , \qquad \frac{\partial\rho_1}{\partial t} + \rho_0\operatorname{div}\vect v = 0 , \qquad \rho_1 = \rho_0\chi_Sp ,

and together they give the wave equation for the overpressure,

Δp=1c22pt2,c=1ρ0χS,\Delta p = \frac1{c^2}\frac{\partial^2p}{\partial t^2} , \qquad c = \frac1{\sqrt{\rho_0\chi_S}} ,

(the same for ρ1\rho_1 and for v\vect v). For a perfect gas, χS=1/γP0\chi_S = 1/\gamma P_0 and

c=γP0ρ0=γRTM:c = \sqrt{\frac{\gamma P_0}{\rho_0}} = \sqrt{\frac{\gamma RT}{M}} :

343m/s343\,\mathrm{m}/\mathrm{s} in air at 20C20{}^{\circ}\mathrm{C}, rising by 0.6m/s0.6\,\mathrm{m}/\mathrm{s} per kelvin; 1000m/s1000\,\mathrm{m}/\mathrm{s} in helium; 1480m/s1480\,\mathrm{m}/\mathrm{s} in water (χS=4.5×1010Pa1\chi_S = 4.5 \times 10^{-10}\,\mathrm{Pa}^{-1}).

Proof. Euler: the convective term ρ(vgrad)v\rho(\vect v\cdot\operatorname{\vect{grad}})\vect v is second order, ρtvρ0tv\rho\,\partial_t\vect v \approx \rho_0\,\partial_t\vect v, and gradP=gradp\operatorname{\vect{grad}}P = \operatorname{\vect{grad}}p. Mass: tρ+div(ρv)tρ1+ρ0divv\partial_t\rho + \operatorname{div}(\rho\vect v) \approx \partial_t\rho_1 + \rho_0\operatorname{div}\vect v. Isentropic law:  ⁣dρ=ρχS ⁣dP\dd\rho = \rho\chi_S\,\dd P to first order. Take the divergence of the first equation and the time derivative of the second: ρ0tdivv=Δp=t2ρ1=ρ0χSt2p\rho_0\partial_t\operatorname{div}\vect v = -\Delta p = -\partial_t^2\rho_1 = -\rho_0\chi_S \partial_t^2p. For the perfect gas, PVγPV^\gamma constant along an isentropic transformation gives  ⁣dρ/ρ= ⁣dP/γP\dd\rho/\rho = \dd P/\gamma P, hence χS=1/γP\chi_S = 1/\gamma P, and P0/ρ0=RT/MP_0/\rho_0 = RT/M.

Remark 7.3 (Why isentropic)

Newton computed the speed of sound with the isothermal compressibility, P0/ρ0=290m/s\sqrt{P_0/\rho_0} = 290\,\mathrm{m}/\mathrm{s}, 15%15\% too low; Laplace saw that the compressions are too fast for heat to flow between the warm crests and the cool troughs — over one period, heat diffuses a few micrometres (Chapter 25), nothing compared with a wavelength — so the transformation is adiabatic and reversible, and γ\gamma appears. The speed of sound is thus a direct measurement of γ\gamma: 1.401.40 for air, 1.671.67 for argon.

Left: a slab of fluid displaced by (x, t) and pushed by the pressures on its faces; its compression sets the overpressure. Right: a plane sound wave — alternate zones of compression and rarefaction moving at c, the fluid itself oscillating back and forth along the direction of propagation (a longitudinal wave).
Left: a slab of fluid displaced by ξ(x,t)\xi(x, t) and pushed by the pressures on its faces; its compression sets the overpressure. Right: a plane sound wave — alternate zones of compression and rarefaction moving at cc, the fluid itself oscillating back and forth along the direction of propagation (a longitudinal wave).

7.2 Plane waves, impedance, intensity

Proposition 7.4 (Plane progressive sound wave)

For a plane wave p=f(xct)p = f(x - ct) travelling toward +x+x, the fluid velocity is along xx, in phase with the overpressure, and

p=Zv,Z=ρ0c=ρ0/χS,p = Z\,v , \qquad Z = \rho_0c = \sqrt{\rho_0/\chi_S} ,

where ZZ is the acoustic impedance of the medium (kgm2s1\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}): 410kgm2s1410\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1} for air, 1.5×106kgm2s11.5 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1} for water, 1.6×106kgm2s1\sim1.6 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1} for soft tissue, 4×107kgm2s14 \times 10^{7}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1} for steel. The wave carries the energy density and the intensity (power per unit area, toward +x+x)

e=12ρ0v2+12χSp2,I=pv,e = \tfrac12\rho_0v^2 + \tfrac12\chi_Sp^2 , \qquad I = p\,v ,

which obey te+xI=0\partial_te + \partial_xI = 0; for the progressive wave the two halves of ee are equal and I=p2/Z=Zv2I = p^2/Z = Zv^2. A sinusoidal wave of pressure amplitude pmp_m has the mean intensity I=pm2/2Z\langle I\rangle = p_m^2/2Z.

Proof. For p=f(xct)p = f(x - ct), ρ0tv=xp=f/cc\rho_0\partial_tv = -\partial_xp = f'/c\cdot c\dots: precisely, ρ0tv=f(xct)\rho_0\partial_tv = -f'(x - ct), and v=f(xct)/ρ0cv = f(x - ct)/\rho_0c satisfies it. The potential term of ee is the work stored in compressing the fluid (an isentropic compression of unit volume by  ⁣dV/V=χS ⁣dp\dd V/V = -\chi_S\,\dd p stores pχS ⁣dp=12χSp2\int p\,\chi_S\dd p = \tfrac12\chi_Sp^2); II is the work rate of the pressure force pSpS on the fluid ahead, moving at vv, per unit area. Balance: te=ρ0vtv+χSptp=vxppxv=x(pv)\partial_te = \rho_0v\partial_tv + \chi_Sp\partial_tp = -v\partial_xp - p\partial_xv = -\partial_x(pv) by the two linearized equations.

Definition 7.5 (Sound level)

The sound level of a wave of mean intensity II is

L=10log10II0 dB,I0=1×1012W/m2L = 10\log_{10}\frac I{I_0} \ \text{dB} , \qquad I_0 = 1 \times 10^{-12}\,\mathrm{W}/\mathrm{m}^{2}

— the threshold of hearing at 1kHz1\,\mathrm{kHz}, corresponding in air to the pressure amplitude p02×105Pap_0 \approx 2 \times 10^{-5}\,\mathrm{Pa} (rms) =2×1010= 2 \times 10^{-10} atmospheres. Doubling the intensity adds 3dB3\,\mathrm{dB}; ten times, 10dB10\,\mathrm{dB}; a hundred times the pressure amplitude, 40dB40\,\mathrm{dB}. Quiet room 30dB30\,\mathrm{dB}, conversation 60dB60\,\mathrm{dB}, busy street 80dB80\,\mathrm{dB}, rock concert 110dB110\,\mathrm{dB}, pain 120dB120\,\mathrm{dB} (I=1W/m2I = 1\,\mathrm{W}/\mathrm{m}^{2}, pm=29Pap_m = 29\,\mathrm{Pa}).

Example 7.6 (How small a sound is)

At the threshold, 1kHz1\,\mathrm{kHz}: pm=2.8×105Pap_m = 2.8 \times 10^{-5}\,\mathrm{Pa}, vm=pm/Z=7×108m/sv_m = p_m/Z = 7 \times 10^{-8}\,\mathrm{m}/\mathrm{s}, and the displacement amplitude ξm=vm/ω=1×1011m\xi_m = v_m/\omega = 1 \times 10^{-11}\,\mathrm{m} — a tenth of an atomic diameter: the eardrum detects motions smaller than an atom. At 120dB120\,\mathrm{dB}, ξm=11µm\xi_m = 11\,\text{µ}\mathrm{m}, still invisible, and pm/P0=3×104p_m/P_0 = 3 \times 10^{-4}: even the loudest sounds are tiny perturbations, which is why the linear theory works so well.

Left: in a plane progressive sound wave the overpressure and the fluid velocity are in phase, and the displacement lags by a quarter period. Right: the decibel scale — each 20\, dB step multiplies the intensity by a hundred and the pressure amplitude by ten. Left: in a plane progressive sound wave the overpressure and the fluid velocity are in phase, and the displacement lags by a quarter period. Right: the decibel scale — each 20\, dB step multiplies the intensity by a hundred and the pressure amplitude by ten.
Left: in a plane progressive sound wave the overpressure and the fluid velocity are in phase, and the displacement lags by a quarter period. Right: the decibel scale — each 20dB20\,\mathrm{dB} step multiplies the intensity by a hundred and the pressure amplitude by ten.

7.3 Spherical waves

Proposition 7.7 (Spherical waves and the inverse-square law)

A small source radiating equally in all directions produces the spherical wave

p(r,t)=Arf(trc),p(r, t) = \frac{A}{r}\,f\Bigl(t - \frac rc\Bigr) ,

whose amplitude falls as 1/r1/r and whose intensity falls as 1/r21/r^2: for a source of acoustic power P\mathcal P, I=P/4πr2I = \mathcal P/4\pi r^2, i.e. 6dB-6\,\mathrm{dB} each time the distance doubles. Far from the source the wave is locally plane, with v=p/Zv = p/Z radial.

Proof. In spherical coordinates, for a function of rr alone, Δp=1r2(rp)r2\Delta p = \frac1r\frac{\partial^2(rp)}{\partial r^2} (admitted; Chapter 11), so u=rpu = rp obeys the one-dimensional wave equation r2u=t2u/c2\partial_r^2u = \partial_t^2u/c^2, whence u=Af(tr/c)u = Af(t - r/c) for the outgoing wave. The power crossing a sphere of radius rr is 4πr2I4\pi r^2I, constant if nothing is absorbed.

Example 7.8 (A siren, a conversation)

A 10W10\,\mathrm{W} siren: I=10/4πr2I = 10/4\pi r^2, 0.8W/m20.8\,\mathrm{W}/\mathrm{m}^{2} at 1m1\,\mathrm{m} (119dB119\,\mathrm{dB}, pain), 79dB79\,\mathrm{dB} at 100m100\,\mathrm{m}, 59dB59\,\mathrm{dB} at 1km1\,\mathrm{km} — still audible over the city. A voice radiates about 10µW10\,\text{µ}\mathrm{W}: 60dB60\,\mathrm{dB} at 1m1\,\mathrm{m}, and 40dB40\,\mathrm{dB} at 10m10\,\mathrm{m}. Air absorbs sound too (more at high frequency, a few decibels per hundred metres at 10kHz10\,\mathrm{kHz}), which is why distant thunder rumbles low.

7.4 The Doppler effect

Theorem 7.9 (Doppler effect)

A source emits at frequency ff and moves at speed vsv_s along the line joining it to an observer who moves at vov_o, both speeds counted positive when they approach each other; the sound travels at cc in the air at rest. The observer receives the frequency

f=fc+vocvs.f' = f\,\frac{c + v_o}{c - v_s} .

A moving source crowds its wavefronts ahead of it (λ=(cvs)/f\lambda' = (c - v_s)/f) and spreads them behind; a moving observer meets wavefronts at the rate (c+vo)/λ(c + v_o)/\lambda. For vs,vocv_s, v_o \ll c both give Δf/f(vs+vo)/c\Delta f/f \approx (v_s + v_o)/c.

Proof. Moving source: the wavefronts emitted at tt and t+1/ft + 1/f are separated by c/fvs/fc/f - v_s/f in the direction of motion, so the wavelength ahead is λ=(cvs)/f\lambda' = (c - v_s)/f and the frequency received by a fixed observer is c/λc/\lambda'. Moving observer: the wavelength is λ=c/f\lambda = c/f but fronts pass at the relative speed c+voc + v_o. Combine.

Left: the wavefronts of a moving source crowd ahead and spread behind — higher pitch approaching, lower receding. Right: a source faster than sound leaves its wavefronts behind; their envelope is the Mach cone, heard on the ground as a boom.
Left: the wavefronts of a moving source crowd ahead and spread behind — higher pitch approaching, lower receding. Right: a source faster than sound leaves its wavefronts behind; their envelope is the Mach cone, heard on the ground as a boom.

Example 7.10 (Sirens, radar guns, red cells)

An ambulance siren at 700Hz700\,\mathrm{Hz} passing at 25m/s25\,\mathrm{m}/\mathrm{s}: 755Hz755\,\mathrm{Hz} approaching, 651Hz651\,\mathrm{Hz} receding — a drop of a sixth of an octave, the familiar "nee-naw" dip. A police radar gun measures the same effect on a 24GHz24\,\mathrm{GHz} radio wave reflected by a car (the wave is shifted twice, by the car receiving and re-emitting): Δf=2fv/c=4.8kHz\Delta f = 2fv/c = 4.8\,\mathrm{kHz} at 30m/s30\,\mathrm{m}/\mathrm{s}. An ultrasound probe at 5MHz5\,\mathrm{MHz} aimed at an artery hears the blood cells at Δf=2fvcosθ/c1.6kHz\Delta f = 2fv\cos\theta/c \approx 1.6\,\mathrm{kHz} for 0.5m/s0.5\,\mathrm{m}/\mathrm{s} at 6060{}^{\circ}: an audible whistle whose pitch is the blood speed. And the spectral lines of a receding galaxy are shifted red by Δλ/λ=v/c\Delta\lambda/\lambda = v/c — the formula holds for light at low speed, with the relativistic correction beyond.

Remark 7.11 (Supersonic)

When vs>cv_s > c the formula breaks down (f<0f' < 0 ahead): no sound precedes the source. The wavefronts emitted along the path have a conical envelope of half-angle θ\theta with sinθ=c/vs\sin\theta = c/v_s (the Mach cone); the pressure jump carried by the cone is the sonic boom, which reaches a listener on the ground only after the aircraft has passed — at Mach 22 and 10km10\,\mathrm{km} of altitude, θ=30\theta = 30{}^{\circ} and the boom arrives 10km/tanθ/vs25s10\,\text{km}/\tan\theta/v_s \approx 25\,\mathrm{s} after the overhead passage. A bullet’s crack and the tip of a whip are the same cone.

Method 7.12 (Orders of magnitude in acoustics)

Given a sound level LL: I=I010L/10I = I_0\,10^{L/10}; then pm=2ZIp_m = \sqrt{2ZI}, vm=pm/Zv_m = p_m/Z, ξm=vm/ω\xi_m = v_m/\omega; the power of a source is 4πr2I4\pi r^2I if it radiates in all directions (twice less over a hard floor, which reflects into a half-space). Going from r1r_1 to r2r_2 changes LL by 20log10(r1/r2)20\log_{10}(r_1/r_2). Adding nn incoherent equal sources adds 10log10n10\log_{10}n; two coherent sources in phase at a point add 6dB6\,\mathrm{dB}.

7.5 Exercises

Exercise 7.1

Speed of sound in air (γ=1.40\gamma = 1.40, M=29g/molM = 29\,\mathrm{g}/\mathrm{mol}) at 0C0{}^{\circ}\mathrm{C}, 20C20{}^{\circ}\mathrm{C} and at 50C-50{}^{\circ}\mathrm{C} (10km10\,\mathrm{km} altitude); in helium (γ=1.67\gamma = 1.67, M=4g/molM = 4\,\mathrm{g}/\mathrm{mol}) and carbon dioxide (γ=1.30\gamma = 1.30, M=44g/molM = 44\,\mathrm{g}/\mathrm{mol}) at 20C20{}^{\circ}\mathrm{C}. Why does a voice sound high-pitched after breathing helium?

Solution

Solution of Exercise 7.1.

c=γRT/Mc = \sqrt{\gamma RT/M}: 331m/s331\,\mathrm{m}/\mathrm{s}, 343m/s343\,\mathrm{m}/\mathrm{s}, 299m/s299\,\mathrm{m}/\mathrm{s}; helium 1010m/s1010\,\mathrm{m}/\mathrm{s}; CO2_2 268m/s268\,\mathrm{m}/\mathrm{s}. The vocal cords vibrate at the same frequency, but the resonances of the vocal tract (which shape the timbre) scale with cc and move up by a factor three: the voice sounds high-pitched.

Exercise 7.2

A conversation at 60dB60\,\mathrm{dB}, 500Hz500\,\mathrm{Hz}: intensity, pressure amplitude, velocity amplitude and displacement amplitude in air (Z=410kgm2s1Z = 410\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}). Same for 120dB120\,\mathrm{dB}. Level of two people talking at once; of a hundred.

Solution

Solution of Exercise 7.2.

60dB60\,\mathrm{dB}: I=1×106W/m2I = 1 \times 10^{-6}\,\mathrm{W}/\mathrm{m}^{2}, pm=2ZI=29mPap_m = \sqrt{2ZI} = 29\,\mathrm{mPa}, vm=pm/Z=7×105m/sv_m = p_m/Z = 7 \times 10^{-5}\,\mathrm{m}/\mathrm{s}, ξm=vm/ω=22nm\xi_m = v_m/\omega = 22\,\mathrm{nm}. 120dB120\,\mathrm{dB}: 1W/m21\,\mathrm{W}/\mathrm{m}^{2}, 29Pa29\,\mathrm{Pa}, 7cm/s7\,\mathrm{cm}/\mathrm{s}, 22µm22\,\text{µ}\mathrm{m}. Two: 63dB63\,\mathrm{dB}; a hundred: 80dB80\,\mathrm{dB}.

Exercise 7.3

A loudspeaker radiates 1.0W1.0\,\mathrm{W} of sound equally in all directions. Intensity and level at 1m1\,\mathrm{m}, 10m10\,\mathrm{m}, 100m100\,\mathrm{m}; distance at which the level falls to 60dB60\,\mathrm{dB}; power needed for 100dB100\,\mathrm{dB} at 30m30\,\mathrm{m} (an open-air concert).

Solution

Solution of Exercise 7.3.

I=1/4πr2I = 1/4\pi r^2: 0.080W/m20.080\,\mathrm{W}/\mathrm{m}^{2} (109dB109\,\mathrm{dB}), 89dB89\,\mathrm{dB}, 69dB69\,\mathrm{dB}; I=106I = 10^{-6} at r=1/4π106=280mr = \sqrt{1/4\pi10^{-6}} = 280\,\mathrm{m}; 100dB100\,\mathrm{dB} at 30m30\,\mathrm{m} needs 4π×900×102=110W4\pi \times 900 \times 10^{-2} = 110\,\mathrm{W} of sound.

Exercise 7.4

Thunder is heard 4.5s4.5\,\mathrm{s} after the flash: distance. A ship’s horn echoes off a cliff after 3.0s3.0\,\mathrm{s}: distance. Sonar: an echo from the sea floor returns after 2.4s2.4\,\mathrm{s} (c=1500m/sc = 1500\,\mathrm{m}/\mathrm{s}): depth. A 5MHz5\,\mathrm{MHz} ultrasound echo returns after 130µs130\,\text{µ}\mathrm{s} in tissue (1540m/s1540\,\mathrm{m}/\mathrm{s}): depth.

Solution

Solution of Exercise 7.4.

4.5×340=1.5km4.5 \times 340 = 1.5\,\mathrm{km}; 340×1.5=510m340 \times 1.5 = 510\,\mathrm{m}; 1500×1.2=1.8km1500 \times 1.2 = 1.8\,\mathrm{km}; 1540×65×106=10cm1540 \times 65 \times 10^{-6} = 10\,\mathrm{cm}.

Exercise 7.5 ★★

A train horn at 500Hz500\,\mathrm{Hz}; c=340m/sc = 340\,\mathrm{m}/\mathrm{s}. (a) Frequency heard by a person on the platform as the train approaches at 40m/s40\,\mathrm{m}/\mathrm{s}, and after it has passed. (b) The person is on a train moving toward the horn at 40m/s40\,\mathrm{m}/\mathrm{s}, the horn at rest; then both moving toward each other at 40m/s40\,\mathrm{m}/\mathrm{s}: compare with a relative speed of 80m/s80\,\mathrm{m}/\mathrm{s} and one body at rest. (c) Frequency heard by the driver of the horn’s train from the echo off a wall ahead.

Solution

Solution of Exercise 7.5.

(a) 500×340/300=567Hz500 \times 340/300 = 567\,\mathrm{Hz}; 500×340/380=447Hz500 \times 340/380 = 447\,\mathrm{Hz}. (b) 500×380/340=559Hz500 \times 380/340 = 559\,\mathrm{Hz}; both: 500×380/300=633Hz500 \times 380/300 = 633\,\mathrm{Hz}, against 654Hz654\,\mathrm{Hz} (source alone at 80m/s80\,\mathrm{m}/\mathrm{s}) or 618Hz618\,\mathrm{Hz} (observer alone): the air, not the relative speed, sets the result. (c) The wall receives 567Hz567\,\mathrm{Hz} and re-emits it at rest; the driver approaches at 40m/s40\,\mathrm{m}/\mathrm{s}: 567×380/340=633Hz567 \times 380/340 = 633\,\mathrm{Hz}.

Exercise 7.6 ★★

For a pressure amplitude of 1.0Pa1.0\,\mathrm{Pa} at 1kHz1\,\mathrm{kHz}, compute the velocity and displacement amplitudes, the intensity and the level in air, in water (Z=1.5×106kgm2s1Z = 1.5 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}) and in steel (4×107kgm2s14 \times 10^{7}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}). Same pressure, very different intensities: comment. (Underwater levels are quoted relative to 1µPa1\,\text{µ}\mathrm{Pa}: what is 1Pa1\,\mathrm{Pa} on that scale?)

Solution

Solution of Exercise 7.6.

vm=pm/Zv_m = p_m/Z: 2.4mm/s2.4\,\mathrm{mm}/\mathrm{s}, 0.67µm/s0.67\,\text{µ}\mathrm{m}/\mathrm{s}, 25nm/s25\,\mathrm{nm}/\mathrm{s}; ξm=vm/ω\xi_m = v_m/\omega: 390nm390\,\mathrm{nm}, 0.11nm0.11\,\mathrm{nm}, 4pm4\,\mathrm{pm}; I=pm2/2ZI = p_m^2/2Z: 1.2×103W/m21.2 \times 10^{-3}\,\mathrm{W}/\mathrm{m}^{2} (91dB91\,\mathrm{dB}), 3.3×107W/m23.3 \times 10^{-7}\,\mathrm{W}/\mathrm{m}^{2} (55dB55\,\mathrm{dB}), 1.3×108W/m21.3 \times 10^{-8}\,\mathrm{W}/\mathrm{m}^{2} (41dB41\,\mathrm{dB}). A stiff medium barely moves under a given pressure and carries little power. 1Pa1\,\mathrm{Pa} is 120dB120\,\mathrm{dB} re 1µPa1\,\text{µ}\mathrm{Pa}.

Exercise 7.7 ★★

(a) Newton’s isothermal speed P0/ρ0\sqrt{P_0/\rho_0} for air at 20C20{}^{\circ}\mathrm{C} (ρ0=1.20kg/m3\rho_0 = 1.20\,\mathrm{kg}/\mathrm{m}^{3}) and Laplace’s correction. (b) Measured: 343m/s343\,\mathrm{m}/\mathrm{s} in air, 323m/s323\,\mathrm{m}/\mathrm{s} in argon (M=40g/molM = 40\,\mathrm{g}/\mathrm{mol}) at 20C20{}^{\circ}\mathrm{C}: deduce γ\gamma for each; interpret with the number of degrees of freedom. (c) Estimate how far heat diffuses in one period at 1kHz1\,\mathrm{kHz} (thermal diffusivity of air 2×105m2/s2 \times 10^{-5}\,\mathrm{m}^{2}/\mathrm{s}) and compare with the wavelength.

Solution

Solution of Exercise 7.7.

(a) 1.013×105/1.2=290m/s\sqrt{1.013 \times 10^5/1.2} = 290\,\mathrm{m}/\mathrm{s}; ×1.4\times\sqrt{1.4}: 343m/s343\,\mathrm{m}/\mathrm{s}. (b) γ=c2M/RT\gamma = c^2M/RT: 1.401.40 for air, 1.711.71 for argon (5/35/3 within the rounding): three translational degrees of freedom (γ=1+2/3\gamma = 1 + 2/3) against five for a diatomic gas (1+2/51 + 2/5). (c) D/f=2×108=0.14mmλ=34cm\sqrt{D/f} = \sqrt{2 \times 10^{-8}} = 0.14\,\mathrm{mm} \ll \lambda = 34\,\mathrm{cm}: no heat flows between crests and troughs.

Exercise 7.8 ★★

Organ pipes. In a pipe the overpressure is zero at an open end and the velocity is zero at a closed end. (a) Standing waves in a pipe open at both ends: show the modes are fn=nc/2Lf_n = nc/2L; in a pipe closed at one end, fn=(2n1)c/4Lf_n = (2n - 1)c/4L. (b) Lengths for a 440Hz440\,\mathrm{Hz} fundamental in each case. (c) Which harmonics does each pipe contain? (d) The real open end sits about 0.60.6 radius beyond the pipe (end correction): for a 4cm4\,\mathrm{cm} pipe, the correction on LL and on ff.

Solution

Solution of Exercise 7.8.

(a) Open–open: p=pmsinkxcosωtp = p_m\sin kx\cos\omega t with kL=nπkL = n\pi; closed–open: p=pmcoskxcosωtp = p_m\cos kx\cos\omega t (velocity node, pressure antinode at the closed end) with kL=(2n1)π/2kL = (2n - 1)\pi/2. (b) L=c/2f=39cmL = c/2f = 39\,\mathrm{cm}; c/4f=19.5cmc/4f = 19.5\,\mathrm{cm}. (c) All harmonics; odd harmonics only (the clarinet’s hollow sound). (d) 0.6×2=1.2cm0.6 \times 2 = 1.2\,\mathrm{cm} per open end: Leff=41.4cmL_{\text{eff}} = 41.4\,\mathrm{cm}, f=414Hzf = 414\,\mathrm{Hz}, 6%6\% flat — the pipe must be cut to 36.6cm36.6\,\mathrm{cm}.

Exercise 7.9 ★★

A 2.0kW2.0\,\mathrm{kW} electric siren converts 20%20\% of its power into sound radiated into a half-space (it sits on a roof). (a) Intensity, level and pressure amplitude at 100m100\,\mathrm{m}. (b) Distance of the pain threshold (120dB120\,\mathrm{dB}); of the 70dB70\,\mathrm{dB} contour where it stops being alarming. (c) Air absorption adds 1dB1\,\mathrm{dB} per 100m100\,\mathrm{m} at its frequency: distance of the 70dB70\,\mathrm{dB} contour now (solve numerically). (d) How many such sirens cover a city of 10km10\,\mathrm{km} radius?

Solution

Solution of Exercise 7.9.

P=400W\mathcal P = 400\,\mathrm{W}, I=P/2πr2I = \mathcal P/2\pi r^2. (a) 6.4×103W/m26.4 \times 10^{-3}\,\mathrm{W}/\mathrm{m}^{2}, 98dB98\,\mathrm{dB}, pm=2.3Pap_m = 2.3\,\mathrm{Pa}. (b) r=400/2π=8mr = \sqrt{400/2\pi} = 8\,\mathrm{m}; 70dB70\,\mathrm{dB} at 2.5km2.5\,\mathrm{km}. (c) 9820log(r/100)(r100)/100=7098 - 20\log(r/100) - (r - 100)/100 = 70: r950mr \approx 950\,\mathrm{m}. (d) π(10)2/π(0.95)2110\pi(10)^2/\pi(0.95)^2 \approx 110 sirens.

Exercise 7.10 ★★★

Energy of a standing sound wave. In a closed tube of length LL the overpressure is p=pmcos(kx)cos(ωt)p = p_m\cos(kx)\cos(\omega t), k=nπ/Lk = n\pi/L. (a) Find v(x,t)v(x, t) from the linearized Euler equation. (b) Kinetic and potential energy densities; show that they oscillate in quadrature in time and are shifted by a quarter wavelength in space. (c) Total energy in the tube (section SS); check it is constant. (d) Mean intensity: zero everywhere — and yet the energy moves: describe how.

Solution

Solution of Exercise 7.10.

(a) ρ0tv=pmksinkxcosωt\rho_0\partial_tv = p_mk\sin kx\cos\omega t: v=(pm/Z)sinkxsinωtv = (p_m/Z)\sin kx\sin\omega t. (b) ek=12χSpm2sin2kxsin2ωte_k = \tfrac12\chi_Sp_m^2\sin^2kx\sin^2\omega t, ep=12χSpm2cos2kxcos2ωte_p = \tfrac12\chi_Sp_m^2\cos^2kx\cos^2\omega t: one is maximal when the other vanishes, in time and in space. (c) E=S0L(ek+ep) ⁣dx=14χSpm2SLE = S\int_0^L(e_k + e_p)\dd x = \tfrac14\chi_Sp_m^2SL, constant. (d) I=pv=(pm2/4Z)sin2kxsin2ωtI = pv = (p_m^2/4Z)\sin2kx\sin2\omega t: zero mean, but twice per period energy flows from the pressure antinodes to the velocity antinodes and back.

Exercise 7.11 ★★★

Sonic boom. An aircraft flies horizontally at v=1.6cv = 1.6\,c at altitude h=12kmh = 12\,\mathrm{km}, c=300m/sc = 300\,\mathrm{m}/\mathrm{s} there. (a) Derive the Mach angle from the envelope of the spherical wavefronts. (b) Time between the overhead passage and the boom on the ground (neglect the variation of cc with altitude). (c) Width on the ground of the strip that hears the boom as the aircraft flies by, if the cone’s trace is heard within ±30km\pm30\,\mathrm{km} of the track: why is supersonic flight over land banned? (d) A rifle bullet at 800m/s800\,\mathrm{m}/\mathrm{s}: Mach angle; what an observer standing 10m10\,\mathrm{m} from the trajectory hears, and in what order.

Solution

Solution of Exercise 7.11.

(a) The front emitted at t=0t = 0 has radius ctct when the source is vtvt away: the tangent cone has sinθ=c/v\sin\theta = c/v. (b) θ=39\theta = 39{}^{\circ}; the cone reaches the ground under the aircraft when it is h/tanθ=15kmh/\tan\theta = 15\,\mathrm{km} further: 15000/480=31s15000/480 = 31\,\mathrm{s} after the overhead passage. (c) A 60km60\,\mathrm{km}-wide carpet along the whole route hears the boom. (d) sinθ=340/800\sin\theta = 340/800, θ=25\theta = 25{}^{\circ}; the crack of the cone arrives first, the muzzle blast, travelling at cc from the gun, later.

Exercise 7.12 ★★★

Doppler ultrasound. A probe emits at f=5.0MHzf = 5.0\,\mathrm{MHz} into tissue (c=1540m/sc = 1540\,\mathrm{m}/\mathrm{s}); red cells move at vv along a vessel making the angle θ\theta with the beam. (a) Frequency received by a cell (moving observer). (b) It re-emits (scatters) this frequency as a moving source: frequency back at the probe; show Δf=2fvcosθ/c\Delta f = 2fv\cos\theta/c for vcv \ll c. (c) Δf\Delta f for v=0.50m/sv = 0.50\,\mathrm{m}/\mathrm{s}, θ=60\theta = 60{}^{\circ}; for θ=90\theta = 90{}^{\circ} — what does the operator do? (d) The probe can resolve 50Hz50\,\mathrm{Hz}: velocity resolution. Why is the Doppler signal made audible rather than displayed only?

Solution

Solution of Exercise 7.12.

(a) f1=f(c+vcosθ)/cf_1 = f(c + v\cos\theta)/c. (b) f2=f1c/(cvcosθ)=f(c+vcosθ)/(cvcosθ)f(1+2vcosθ/c)f_2 = f_1c/(c - v\cos\theta) = f(c + v\cos\theta) /(c - v\cos\theta) \approx f(1 + 2v\cos\theta/c). (c) 2×5×106×0.5×0.5/1540=1.6kHz2 \times 5 \times 10^6 \times 0.5 \times 0.5/1540 = 1.6\,\mathrm{kHz}; zero at 9090{}^{\circ}: tilt the probe. (d) Δv=50×1540/(2×5×106×0.5)=1.5cm/s\Delta v = 50 \times 1540/ (2 \times 5 \times 10^6 \times 0.5) = 1.5\,\mathrm{cm}/\mathrm{s}. The ear follows pitch and timbre in real time: a smooth whistle means laminar flow, a hiss means turbulence behind a narrowing.

An ultrasound scanner: a few megahertz of sound, timed echoes and the impedance mismatches between tissues draw the image; the gel removes the film of air that would reflect everything.
An ultrasound scanner: a few megahertz of sound, timed echoes and the impedance mismatches between tissues draw the image; the gel removes the film of air that would reflect everything.

7.6 Problem: From thunder to the echograph

Problem 7.1

Weekend problem — sound in the open air, in a concert hall, inside the body and from a passing siren

Air: γ=1.40\gamma = 1.40, M=29g/molM = 29\,\mathrm{g}/\mathrm{mol}, Z=410kgm2s1Z = 410\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1} at 15C15{}^{\circ}\mathrm{C}; R=8.31J/(molK)R = 8.31\,\mathrm{J}/(\mathrm{mol}\,\mathrm{K}).

Part I — The storm.

  1. Speed of sound at 15C15{}^{\circ}\mathrm{C} and at 30C30{}^{\circ}\mathrm{C}; justify the rule "three seconds per kilometre".
  2. Thunder arrives 4.0s4.0\,\mathrm{s} after the flash: distance of the strike. The thunder lasts several seconds although the flash is instantaneous: why?
  3. Near the strike the level reaches 120dB120\,\mathrm{dB}: pressure amplitude and velocity amplitude of the air.
  4. Energy received per square metre of wall during a thunderclap of 2s2\,\mathrm{s} at 120dB120\,\mathrm{dB}.
  5. On a clear night the ground cools and the air is colder below than above. Sound rays obey Snell’s law between layers, sini/c=\sin i/c = const: do rays launched upward bend down or up? Why are distant sounds heard so well at night and over water?
  6. By day, the reverse: a listener at 3km3\,\mathrm{km} hears nothing. Estimate the angle by which a horizontal ray has bent after 3km3\,\mathrm{km} if cc falls by 1%1\,\% per 500m500\,\mathrm{m} of altitude (treat the bending as uniform: the ray is a circle).
  7. Air absorbs high frequencies far more than low ones: why does distant thunder rumble while a nearby strike cracks?

Part II — The concert. A loudspeaker receives 100W100\,\mathrm{W} of electrical power and converts 2%2\% of it into sound, radiated equally into the half-space in front of it.

  1. Acoustic power; intensity and level at 10m10\,\mathrm{m}.
  2. Pressure amplitude there; velocity and displacement amplitudes at 100Hz100\,\mathrm{Hz}.
  3. Level at 1m1\,\mathrm{m} (is it safe?) and distance at which the music falls to 60dB60\,\mathrm{dB}.
  4. Ten identical loudspeakers spread around the stage, not in phase: level at 10m10\,\mathrm{m}. Two loudspeakers fed in phase, at the same distance from a listener on their axis: level there.
  5. The hall (volume 10000m310\,000\,\mathrm{m}^{3}) has 2000m22000\,\mathrm{m}^{2} of walls and audience that absorb 30%30\% of the sound hitting them: estimate the acoustic energy stored in the hall at equilibrium and the reverberation time (time for the level to drop 60dB60\,\mathrm{dB} after the music stops), using the balance between the power emitted and the power absorbed (Iwallce/4I_{\text{wall}} \approx ce/4 for a diffuse field, admitted).

Part III — The echograph. Soft tissue: c=1540m/sc = 1540\,\mathrm{m}/\mathrm{s}, Z=1.6×106kgm2s1Z = 1.6 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}; bone Z=7×106kgm2s1Z = 7 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}; air 400kgm2s1400\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}. At normal incidence the pressure amplitude reflected at an interface is r=(Z2Z1)/(Z2+Z1)r = (Z_2 - Z_1)/(Z_2 + Z_1) times the incident one (derived in Chapter 15); tissue attenuates sound by about 0.5dB0.5\,\mathrm{dB} per centimetre and per megahertz.

  1. Wavelength in tissue at 3MHz3\,\mathrm{MHz}, 5MHz5\,\mathrm{MHz}, 10MHz10\,\mathrm{MHz}; the smallest detail each can resolve is about one wavelength.
  2. Echo delay from an organ 12cm12\,\mathrm{cm} deep; maximum rate at which pulses can be sent without confusing echoes; time to build an image of 200200 lines.
  3. Fraction of the pressure, and of the energy, reflected at a tissue–air interface; at a tissue–bone interface; between fat (Z=1.38×106kgm2s1Z = 1.38 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}) and muscle (1.70×106kgm2s11.70 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}\,\mathrm{s}^{-1}). Why the gel, and why bones cast shadows?
  4. At 5MHz5\,\mathrm{MHz} the beam crosses 2cm2\,\mathrm{cm} of fat before meeting muscle: fraction of the emitted energy that comes back to the probe from that interface (reflection and round-trip attenuation), in decibels.
  5. Round-trip attenuation in decibels for the organ of question 12 at each of the three frequencies; if the scanner can handle 80dB80\,\mathrm{dB} of loss, which frequencies work? State the resolution versus depth trade-off.
  6. The probe emits pulses of 1µs1\,\text{µ}\mathrm{s} at 5MHz5\,\mathrm{MHz}: how many wavelengths long is a pulse, and how does that limit the depth resolution?
  7. Doppler mode at 5MHz5\,\mathrm{MHz} on an artery at 0.40m/s0.40\,\mathrm{m}/\mathrm{s}, beam at 6060{}^{\circ}: shift; what the operator hears.

Part IV — The siren.

  1. An ambulance passes at 90km/h90\,\mathrm{km}/\mathrm{h} with a 700Hz700\,\mathrm{Hz} siren: frequencies heard approaching and receding; the interval between them in semitones (a semitone is a ratio 21/122^{1/12}).
  2. The listener is in a car going at 15m/s15\,\mathrm{m}/\mathrm{s} toward the approaching ambulance: frequency heard.
  3. At what instant does a listener on the pavement hear exactly 700Hz700\,\mathrm{Hz}?
  4. The ambulance’s wavefronts ahead of it: wavelength; speed of the sound relative to the ambulance ahead and behind.
  5. A radar gun at 24GHz24\,\mathrm{GHz} reads a 3.2kHz3.2\,\mathrm{kHz} shift from a car: speed of the car (the wave is shifted twice).
  6. Sum up: the six speeds of this problem (sound in air, in tissue, the ambulance, the car, the red cells, light) and the one formula that handles them all.
Solution

Solution of Problem 7.1.

1. c=1.4×8.31×288/0.029=340m/sc = \sqrt{1.4 \times 8.31 \times 288/0.029} = 340\,\mathrm{m}/\mathrm{s}; 349m/s349\,\mathrm{m}/\mathrm{s} at 30C30{}^{\circ}\mathrm{C}. 1km1\,\mathrm{km} in 2.9s2.9\,\mathrm{s}.

2. 1.4km1.4\,\mathrm{km}. The channel is kilometres long; the sound of its different parts arrives over seconds, with echoes from clouds and ground.

3. I=1W/m2I = 1\,\mathrm{W}/\mathrm{m}^{2}: pm=2ZI=29Pap_m = \sqrt{2ZI} = 29\,\mathrm{Pa}, vm=7cm/sv_m = 7\,\mathrm{cm}/\mathrm{s}.

4. It=2J/m2It = 2\,\mathrm{J}/\mathrm{m}^{2}.

5. cc grows upward; sini/c\sin i/c constant makes ii grow, so the ray bends toward the horizontal and back down: sound is channelled along the ground and carries far. Over water the lowest air is cooled by the water: the same.

6. The rays bend upward, leaving a shadow zone. Radius of curvature R=c/( ⁣dc/ ⁣dz)=50kmR = c/(\dd c/\dd z) = 50\,\mathrm{km}: after 3km3\,\mathrm{km} the ray has turned by 3/50=0.06rad=3.43/50 = 0.06\,\mathrm{rad} = 3.4{}^{\circ} and risen 90m90\,\mathrm{m}: the listener is below it.

7. Absorption grows as f2f^2: the crack’s high frequencies are gone after a few kilometres, the low rumble remains.

8. P=2W\mathcal P = 2\,\mathrm{W}; I=2/2πr2=3.2×103W/m2I = 2/2\pi r^2 = 3.2 \times 10^{-3}\,\mathrm{W}/\mathrm{m}^{2} at 10m10\,\mathrm{m}: 95dB95\,\mathrm{dB}.

9. pm=2×410×3.2×103=1.6Pap_m = \sqrt{2 \times 410 \times 3.2 \times 10^{-3}} = 1.6\,\mathrm{Pa}; vm=3.9mm/sv_m = 3.9\,\mathrm{mm}/\mathrm{s}; ξm=vm/2πf=6µm\xi_m = v_m/2\pi f = 6\,\text{µ}\mathrm{m}.

10. +20dB+20\,\mathrm{dB}: 115dB115\,\mathrm{dB} at 1m1\,\mathrm{m} — damaging within minutes. 60dB60\,\mathrm{dB}: r=2/2π106=560mr = \sqrt{2/2\pi10^{-6}} = 560\,\mathrm{m}.

11. Ten incoherent: +10dB+10\,\mathrm{dB}, 105dB105\,\mathrm{dB}. Two in phase: the pressure doubles, +6dB+6\,\mathrm{dB}, 101dB101\,\mathrm{dB}.

12. Balance P=αAce/4\mathcal P = \alpha A\,ce/4: e=8/(0.3×2000×340)=3.9×105J/m3e = 8/(0.3 \times 2000 \times 340) = 3.9 \times 10^{-5}\,\mathrm{J}/\mathrm{m}^{3}, E=eV=0.4JE = eV = 0.4\,\mathrm{J}. After the stop,  ⁣dE/ ⁣dt=(αAc/4V)E\dd E/\dd t = -(\alpha Ac /4V)E: τ=4V/αAc=0.20s\tau = 4V/\alpha Ac = 0.20\,\mathrm{s}, and 60dB60\,\mathrm{dB} takes τln106=2.7s\tau\ln10^6 = 2.7\,\mathrm{s} (Sabine’s reverberation time).

13. λ=c/f\lambda = c/f: 0.51mm0.51\,\mathrm{mm}, 0.31mm0.31\,\mathrm{mm}, 0.15mm0.15\,\mathrm{mm}.

14. 2×0.12/1540=156µs2 \times 0.12/1540 = 156\,\text{µ}\mathrm{s}; 6.4kHz6.4\,\mathrm{kHz}; 200200 lines in 31ms31\,\mathrm{ms} (thirty images a second).

15. Tissue–air: r=0.9995r = -0.9995, 99.9%99.9\% of the energy reflected — hence the gel, which removes the air film. Tissue–bone: r=0.63r = 0.63, 40%40\% of the energy; the rest is absorbed by the bone, which casts a shadow. Fat–muscle: r=0.10r = 0.10, 1%1\% of the energy: the faint echoes the image is made of.

16. Reflected fraction 1.1%1.1\% (20dB-20\,\mathrm{dB}); round trip 4cm4\,\mathrm{cm} at 5MHz5\,\mathrm{MHz}: 10dB-10\,\mathrm{dB}; in all 30dB-30\,\mathrm{dB}, one thousandth.

17. Round trip 24cm24\,\mathrm{cm}: 36dB36\,\mathrm{dB}, 60dB60\,\mathrm{dB}, 120dB120\,\mathrm{dB}: 3MHz3\,\mathrm{MHz} and 5MHz5\,\mathrm{MHz} work, 10MHz10\,\mathrm{MHz} does not — deep organs are imaged at low frequency with coarse resolution, superficial ones at high frequency finely.

18. Five wavelengths, 1.5mm1.5\,\mathrm{mm} long: two interfaces closer than about 0.8mm0.8\,\mathrm{mm} (half the pulse) give overlapping echoes.

19. 2×5×106×0.4×0.5/1540=1.3kHz2 \times 5 \times 10^6 \times 0.4 \times 0.5/1540 = 1.3\,\mathrm{kHz}: a whistle whose pitch rises and falls with each heartbeat.

20. v=25m/sv = 25\,\mathrm{m}/\mathrm{s}: 700×340/315=756Hz700 \times 340/315 = 756\,\mathrm{Hz}, 700×340/365=652Hz700 \times 340/365 = 652\,\mathrm{Hz}; ratio 1.161.16, 12log21.16=2.612\log_21.16 = 2.6 semitones.

21. 700×355/315=789Hz700 \times 355/315 = 789\,\mathrm{Hz}.

22. At closest approach, when the ambulance’s velocity is perpendicular to the line of sight (strictly, when the sound now arriving was emitted at that point).

23. λ=(34025)/700=0.45m\lambda' = (340 - 25)/700 = 0.45\,\mathrm{m} (against 0.49m0.49\,\mathrm{m}); the sound recedes from the ambulance at 315m/s315\,\mathrm{m}/\mathrm{s} ahead and 365m/s365\,\mathrm{m}/\mathrm{s} behind.

24. v=cΔf/2f=3×108×3200/4.8×1010=20m/s=72km/hv = c\,\Delta f/2f = 3 \times 10^8 \times 3200/4.8 \times 10^{10} = 20\,\mathrm{m}/\mathrm{s} = 72\,\mathrm{km}/\mathrm{h}.

25. 340m/s340\,\mathrm{m}/\mathrm{s}, 1540m/s1540\,\mathrm{m}/\mathrm{s}, 25m/s25\,\mathrm{m}/\mathrm{s}, 20m/s20\,\mathrm{m}/\mathrm{s}, 0.4m/s0.4\,\mathrm{m}/\mathrm{s}, 3×108m/s3 \times 10^{8}\,\mathrm{m}/\mathrm{s}: f=f(c+vo)/(cvs)f' = f(c + v_o)/(c - v_s), applied once or twice, and for light at low speed.

Terms defined in this chapter

See all 393 terms in the glossary