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PHYS 536 R. J. Wilkes Session 17 1. Guest speaker: Bob Odom, UW Applied Physics Lab 2. Thomas Loop, Distinction between sound, noise & music 3. Regular lecture: Underwater acoustics 3/7/2019

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Page 1: PHYS 536 - University of Washington

PHYS 536 R. J. Wilkes

Session 17 1. Guest speaker: Bob Odom, UW Applied Physics Lab 2. Thomas Loop, Distinction between sound, noise & music 3. Regular lecture: Underwater acoustics

3/7/2019

Page 2: PHYS 536 - University of Washington

Course syllabus and schedule –second part

2

See : http://courses.washington.edu/phys536/syllabus.htm

Tonight 18 7-Mar GuestLecturer:BobOdom,UWAppliedPhysicsLab19 12-Mar Studentreport2presentaEons

20 14-Mar Studentreport2presentaEons.TAKE-HOMEFINALEXAMISSUED

-- 18-Mar FINALEXAMANSWERSDUEby5PM

Page 3: PHYS 536 - University of Washington

Announcements

End of term is almost here – topic 2 reports due next week •  Everyone gives a brief (15 min max) presentation in class describing what

you learned •  You do not need to submit a formal paper, but should email me

your slides including notes (can be a simple text file accompanying slides, or notes inside a ppt file) •  Slides and notes must be sent by 6 pm on night you present

•  Time slots assigned over the 2 nights next week (next slide) Thanks to those who signed up for Tuesday night

•  Don’t forget: 15 minutes max, including 1~ 2 min for questions •  Practice your talk to make sure you can finish in time

•  Don’t spend time repeating things already discussed in class, just refer to them if needed – focus on the new information you learned

•  Guest speaker: Tonight: Bob Odom, Sr. Principal Physicist, UW Applied Physics Lab (see

), Prof. Emeritus of Earth Sciences

Page 4: PHYS 536 - University of Washington

Presentation schedule

Time Thurs 3/7 Topic 8:00 Thomas Loop Distinction between sound, noise and music

Time Tues 3/12 Topic (Thanks volunteers!) 7:00 James Sayre Features of Medical Ultrasound Transducers 7:15 Jon Julius brass instruments 7:30 Martin Caspe temperament from a Physics and historical context 7:45 Kristina Gill Absorption of sound; how anechoic chambers work 8:00 Rana Levy LIGO sound 8:15 Pankaj Karna Architectural Acoustics of Closed Spaces 8:30 Sean Douglass acoustic holography 8:45 Roger Vargas Wave Field Synthesis and its applications

Time Thurs 3/14 Topic 7:00 Evan Bluhm guitar soundboard at hi-f with FEA 7:15 Steven Canning distinguishing music from speech II 7:30 Lazouich Ford woodwind instruments 7:45 Michael Greiner acoustics of the Puget sound 8:00 Manny Mercado analytical comparison of two concert halls 8:15 Michael Stullick applications of acoustic tweezers 8:30 Jermaine Wegner Acoustical levitation and its biological applications 8:45 4

Tonight

Page 5: PHYS 536 - University of Washington

Guest Speaker Thursday

5

Bob Odom, Sr. Principal Physicist, UW Applied Physics Lab (see www.apl.washington.edu ), Prof. Emeritus of Earth Sciences

Page 6: PHYS 536 - University of Washington

Sound absorption underwater

•  Loss of intensity in water is related to shear and bulk viscosity –  Shear viscosity: due to relative motion between water layers

•  Usually less important than bulk viscosity –  Bulk viscosity: due to molecular effects during a sound wave cycle

•  Relaxation time = characteristic time τ for molecular effect –  Small effects unless τ ~ T = 1/f –  Main culprits are MgSO4 and boric acid B(OH)3

•  Loss rate depends on temperature, seawater pressure and salinity –  SPL in a plane wave decreases as

6

dpdx

≈ −αexpp→ p(x) = p0 exp(−αexpx)→ ln pp0

⎝⎜

⎠⎟= −αexpx

αexp = exponential attenuation rate

dB loss = −20 log10pp0

⎝⎜

⎠⎟=αexpx 20 log10 (e)[ ] = 8.66αexpx

Attenuation coefficient α = dB loss x( )→ dB loss =αx

Page 7: PHYS 536 - University of Washington

Sound absorption underwater

•  Attenuation coefficients for relevant components of seawater –  Frequency dependent

7

For plane→ spherical waves, replace x→ R− R0( ), p0 → p0R0 / Rp = p0 R0 / R( )exp −αexp R− R0( )⎡⎣ ⎤⎦

Transmission loss TL = −20 log10pp0

⎝⎜

⎠⎟

TL = 20 log10RR0

⎝⎜

⎠⎟+α R− R0( ), dB

→ (spherical spreading) + (absorption)

distance R where loss rate ddR⎛

⎝⎜

⎠⎟

due to absorption term exceeds rate

due to spreading Rt =8.68α

Page 8: PHYS 536 - University of Washington

Sonar equation

•  Sonar equation gives intensity vs distance, after all quantities are made dimensionless by ratios with reference values:

SPL = SL – TL SPL = dB at distance R = 10 log(P/Pref)2 dB re Pref SL=source level= 10 log(P0/Pref)2 dB re Pref TL =transmission loss (as discussed previously)P

Here dB = “underwater dB” à P=rms sound pressure, with Pref = 1 µPa –  This is the sonar equation for passive sonar (1-way, only receiving)

where the signal is ~ monofrequency tone (narrow bandwidth source) –  SL can be obtained from power output of source:

8

Total power from source over spherical surface is

Π= I R2 dΩ∫ =4π p02 R0

2

ρ c⎛

⎝⎜

⎠⎟

R0 = spherical source reference radius (1 m is conventional)p0 = sound p at source; usually dB are taken re 1µPaρ =water density (1026 kg/m3 for seawater), c = sound speedso SL = 10 log Π+171 dB re 1µPa

Page 9: PHYS 536 - University of Washington

Sonar equation

•  Receivers with significant bandwidth have to take into account ambient noise spectra: Noise Spectrum Level NSL = noise spectral density (dB re 1 µPa per Hz)

9

Detected noise level DNL = NSL + (10 logw)−DIDI = directivity index

Sound source spectrum: SSL =10 log10s ⋅1HzIREF

⎝⎜

⎠⎟=αexpx 20 log10 (e)

s( f ) = source spectral density at frequency f (intensity per Hz)

for s( f ) ~ const over bandwidth (w, Hz), SL =10 log s ⋅wIREF

⎝⎜

⎠⎟,

w

s(f)

Page 10: PHYS 536 - University of Washington

Defining source characteristics

•  Directivity D : how concentrated is a source’s angular distribution, relative to simple isotropic source?

–  Directivity index: DI = 10 log D

10

Angular variation of P(θ,φ) = H (θ ) = 2J1(v)v

, with v = kasinθ

Intensity ≈ H 2 →Directivity D =IAXIAL (r)ISIMPLE (r)

:

intensity of given source / that of simple (spherical pattern) source

IAXIAL (r)ISIMPLE (r)

=P2AXIAL (r)

P2SIMPLE (r)

→D =4π

H 2 (θ )Ω

,

where H 2 (θ )Ω= average over solid angle Ω

From lecture 9

Page 11: PHYS 536 - University of Washington

Sonar equation

•  Taking into account noise, the sonar equation becomes SNR (dB) = SL -TL – DNL SNR = signal to noise ratio, SPL/DNL SPL = dB level at given location = 10 log(P/Pref)2 dB re Pref

(SL=source level, TL =transmission loss, DNL=detected noise level) –  Example (similar to Kinsler sect 15.10) Source is stationary, emits 120 dB around 1 kHz in 13 kt winds (so sea state 3), NSL=62 dB / Hz, DI=20 dB Receiver has w=100 Hz width filter at 1 kHz How far away can the source be heard with SNR = 0 dB (signal level same as noise)? DNL = NSL+10log(100w)-DI = 62 +20 -20 = 62 dB TL = SL – DNL – SNR=120 – 62 – 0 à must have TL < 78 dB TL = 20 log r + ar, for seawater, a=0.86α=0.07 dB/km

78 dB = 20 log r + 0.07 r à from fig in Kinsler, r~ 10 km 11

Page 12: PHYS 536 - University of Washington

12

•  Unlike light, sound has a preferred reference frame: the medium •  If sound source and observer are in relative motion, observed

frequency will differ from source’s frequency •  For observer moving relative to medium with speed u, apparent

propagation speed c’ will be different:

–  Wavelength cannot change – source is producing waves of constant length in the medium, and same length in moving coordinate system (motion does not change lengths except near light speed!)

–  Observed frequency has to change, to match apparent speed and fixed wavelength:

–  So if observer is moving (speed u) relative to source at rest in medium, apparent frequency f’ is:

c = λ f

f ' = c '

λ

c ' = c ± u(sign depends on relative direction of u )

Another issue: Doppler Effect for moving source/receiver

12

f ' = c 'λ=c+u( )c / f( )

= fc+u( )c

= f 1+ uc

⎝⎜

⎠⎟

+ sign if u is toward source, Minus sign if away from source

Page 13: PHYS 536 - University of Washington

13

Doppler effect: •  If source is moving (speed u) relative to observer at rest in medium,

then –  Frequency remains constant (same time interval between wavefront

emissions from source) –  But source now chases its own waves (or runs away from them):

wavelength in the medium is shorter or longer •  Wave speed = c •  Time between successive peaks = T •  Distance between peaks = cT – uT = wavelength •  Frequency of wave in medium (and for observer):

•  Notice the central role of the medium in both cases

f ' = c

λ '=

cc − u( )T

=c

c − u( )f = f 1

1− u / c⎛

⎝⎜⎞

⎠⎟

minus sign if toward observer, + sign if away from observer. Notice: different f for observers on opposite sides of the source!

13

Page 14: PHYS 536 - University of Washington

14

Doppler effect summary: •  General case

–  For either source or observer (or both) moving relative to medium,

c = speed of sound in medium u = speed of source/observer in the medium (both are unsigned = always taken as positive) Use upper sign if source and observer move toward each other, lower sign if source and observer move away from each other

f ' = f1± uOBS

c

⎝⎜

⎠⎟

1+ uSRCc

⎝⎜

⎠⎟+

Page 15: PHYS 536 - University of Washington

15

Examples •  Car moving with u=18 m/s sounds horn with f=550 Hz, in still air at 20C. What f’ is heard by observer on sidewalk?

Moving source, observer at rest in air: Car toots again while at stop sign. What f’ is heard by bicyclist with u=7.2 m/s

toward the car? Moving observer, source at rest in air: Road-raging driver toots horn yet again, when car is again moving with u=18 m/

s. Now what f’ is heard by bicyclist?

f ' = f 1

1− u / c⎛

⎝⎜⎞

⎠⎟= 550Hz 1

1− 18m/s / 343m/s( )⎛

⎝⎜

⎠⎟ = 550Hz 1.055( ) = 580Hz

f ' = f 1+ u

c⎛

⎝⎜⎞

⎠⎟= 550Hz 1+ 7.2m/s

343m/s⎛

⎝⎜⎞

⎠⎟= 550Hz 1.02( ) = 562Hz

f ' = f1+

uOBS

c⎛

⎝⎜⎞

⎠⎟

1−uSRC

c⎛

⎝⎜⎞

⎠⎟

= 550Hz1+ 7.2m/s / 343m/s( )( )1− 18m/s / 343m/s( )( )

= 550Hz 1.07( ) = 590Hz

Source and observer both in motion relative to air, approaching each other

Page 16: PHYS 536 - University of Washington

Announcements (repeat)

End of term is almost here – topic 2 reports due next week •  Everyone gives a brief (15 min max) presentation in class describing what

you learned •  You do not need to submit a formal paper, but should email me

your slides including notes (can be a simple text file accompanying slides, or notes inside a ppt file) •  Slides and notes must be sent by 6 pm on night you present

•  Time slots assigned over the 2 nights next week (next slide) Thanks to those who signed up for Tuesday night

•  Don’t forget: 15 minutes max, including 1~ 2 min for questions •  Practice your talk to make sure you can finish in time

•  Don’t spend time repeating things already discussed in class, just refer to them if needed – focus on the new information you learned

•  Guest speaker: Tonight: Bob Odom, Sr. Principal Physicist, UW Applied Physics Lab (see

), Prof. Emeritus of Earth Sciences

Page 17: PHYS 536 - University of Washington

Presentation schedule

Time Thurs 3/7 Topic 8:00 Thomas Loop Distinction between sound, noise and music

Time Tues 3/12 Topic (Thanks volunteers!) 7:00 James Sayre Features of Medical Ultrasound Transducers 7:15 Jon Julius brass instruments 7:30 Martin Caspe temperament from a Physics and historical context 7:45 Kristina Gill Absorption of sound; how anechoic chambers work 8:00 Rana Levy LIGO sound 8:15 Pankaj Karna Architectural Acoustics of Closed Spaces 8:30 Sean Douglass acoustic holography 8:45 Roger Vargas Wave Field Synthesis and its applications

Time Thurs 3/14 Topic 7:00 Evan Bluhm guitar soundboard at hi-f with FEA 7:15 Steven Canning distinguishing music from speech II 7:30 Lazouich Ford woodwind instruments 7:45 Michael Greiner acoustics of the Puget sound 8:00 Manny Mercado analytical comparison of two concert halls 8:15 Michael Stullick applications of acoustic tweezers 8:30 Jermaine Wegner Acoustical levitation and its biological applications 8:45 17

Tonight