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May 22-23, 2011 Active Noise Control: Is it Good for Anything? Scott D. Sommerfeldt Acoustics Research Group Dept. of Physics & Astronomy Brigham Young University April 2, 2012

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Page 1: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Active Noise Control: Is it Good for Anything?

Scott D. Sommerfeldt Acoustics Research Group

Dept. of Physics & Astronomy

Brigham Young University

April 2, 2012

Page 2: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Physics and Astronomy Department Size

32 Faculty Members

325 Undergraduates

35 Graduate Students

Acoustics AMO Astronomy/Astrophysics Condensed Matter Plasma Theoretical Physics

Page 3: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Acoustics Research Group

• Interdisciplinary Group – currently primarily Physics and ME

• Physics: 4 full-time faculty (Sommerfeldt, Leishman, Gee, Thomas), one part-time faculty (Neilsen)

• ME: 2 faculty (Blotter, Thomson)

• Typically ~15 grads and ~ 25 undergrads involved from Physics, ME, few from EE

• ARG meets weekly to discuss acoustics topics – typical attendance is about 30

• External funding for group ~ $400k/year

• Strong student chapter of Acoustical Society of America

• Program recognized widely nationally

Page 4: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Outline

• History and background

• Principles of active control

• Local vs global control

• Global control for free-field radiation

• Global control in an enclosed field

• Conclusions

Page 5: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Brief History

• Active control began in 1930’s, with work of Paul Lueg

• Major drawback:

- acoustic feedback

- only worked at certain frequencies

- drifting electronics

A

λ/2

Page 6: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

History (cont.)

• Brief revival in 1950’s – Harry Olson

• Development of digital signal processing led to explosion of research beginning around 1980.

• Number of papers increased nearly exponentially for couple of decades – appears to be leveling off some now.

Page 7: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Active Control Principles

• Most acoustics applications involve linear systems – principle of superposition holds.

• How well must the fields match?

• Phase errors: Magnitude errors: For -20 dB, θ = 5.7° For -20 dB, amp. ratio = 1.0 dB -30 dB, θ = 1.8° For -30 dB, amp. ratio = 0.3 dB

Page 8: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Mechanisms of Active Control

I. Destructive Wave Interference

• Interference between waves leads to "zone of silence."

• Size of zone of silence - 0.1 λ.

• Global energy in the field increases. May not be a problem if the increase in energy is localized to areas of little concern.

Page 9: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Mechanisms of Active Control (cont.)

II. Mutual Coupling • Closely spaced sources modify each other's

radiation impedance. • Possible to achieve global attenuation of sound or

vibration field. (Ex. dipole vs. monopole) • Power radiated by two closely spaced sources

proportional to 1 - sin(kd)/(kd). Thus, sources must be closely spaced.

• For enclosed fields, sources may be remote from each other, but still coupled through the modes of the enclosure.

Page 10: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Adaptive Minimization

• Schematic of control system

• Error given by: 1

0

)()()(N

n

n ntxwtdte

Page 11: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Adaptive Minimization (cont.)

• Update coefficients using negative gradient

• Result:

)()()()1( tentxtwtw nn

Page 12: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Global ANC

• Suppression vs. interference

Mutual coupling of sources affects radiation resistance, power radiated

• Multi-channel systems often required for three-dimensional sound fields

• Global control requires “small” separation between noise and control sources

• Choose error sensor locations and types which result in global attenuation

Page 13: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Difficulty of ANC Problems

13

Page 14: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Cooling Fan Noise

• Axial fans used to cool computers, projectors, etc.

• Spectrum dominated by tonal noise (BPF and harmonics)

• Tonal noise result of unsteady loading on the fan blades

Page 15: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Previous Research and Objectives

• Previous: Single channel efforts

Error microphone usually in far field

Significant global attenuation for BPF (~12 dB), less for harmonics

• Objectives: Multi-channel ANC to achieve global tonal

attenuation

Error microphones in “practical” near field locations

Page 16: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Theoretical Analysis

• Determine:

“good” near field error microphone locations for given control source configuration

appropriate number of control sources

• Model fan/control sources as ideal point sources

• Calculate control source strengths that minimize radiated power

• Plot 2-D pressure and find potential microphone locations

Page 17: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Theoretical Analysis Results

Page 18: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Theoretical Analysis Results

Page 19: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Experimental Apparatus

• 80 mm (3.25”) seven-bladed fan Mounted on face of “CPU-like” enclosure

1” wide rectangular obstruction to create unsteady loading on fan inlet

BPF maintained at 370 Hz

• Four 1 1/8” loudspeakers mounted around fan

• Error microphones located on surface of enclosure

• Nonacoustic reference sensor Infrared emitter/detector

Voltage waveform with BPF and harmonics

• Multi-channel filtered-x LMS algorithm

Page 20: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Experimental Apparatus

Page 21: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Reference Signal Power Spectrum

Page 22: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

ANC at Error Microphone

Page 23: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

2 x 2 ANC—Ideal

7.1 dB 13.5 dB

5.6 dB 5.4 dB

Mean-Square

Pressure Reduction

Page 24: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

4 x 4 ANC—Ideal

8.4 dB

15.5 dB 14.3 dB

18.5 dB

Page 25: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Cooling Fan Control System

• Previous System

– 80 mm fan

– 32 mm loudspeakers

– 370 Hz BPF

• Modifications

– 60 mm fan

– 20 mm loudspeakers

– 600 Hz BPF

– Increase fan speed

Page 26: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

60 mm Fan Results

Page 27: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Global Comparison

80 mm 60 mm Ideal

kd MPR kd MPR kd MPR

BPF 0.4 10.1 dB 0.5 13.6 dB 0.5 ~30 dB

2 x BPF 0.8 16.1 dB 1.0 17.6 dB 1.0 22 dB

3 x BPF 1.2 12.8 dB 1.5 10.5 dB 1.5 14 dB

Mean-square pressure reduction (MPR)

Page 28: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Optimizing the Source Configuration

• Symmetric source configuration shown was assumed to be optimal

• Configuration can be optimized through use of a genetic algorithm

• Four control sources assumed

Page 29: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Optimizing the Source Configuration

Page 30: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Symmetric vs. Linear Configuration

Page 31: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Fan-Noise Findings

• Multi-channel ANC for cooling fan successfully demonstrated

• Point source modeling yields consistently good near field locations for error microphones

• Fan is complex noise source at higher harmonics—need multiple control channels for global reductions

• With better loudspeakers, can achieve more attenuation for BPF

80 mm fan 60 mm fan

Page 32: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Active Control of Energy Density in a Vehicle Cabin

Page 33: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011 The operator’s head does not necessarily stay in a fixed location

during typical operation.

Page 34: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Energy Density vs Pressure2

• Squared Pressure (SP) – More spatial variation

– Control can yield low pressure but potentially high velocity

– Control tends to be more local

• Energy Density (ED) – Less spatial variation

– Control requires both pressure and velocity to be minimized

– Control tends to be more global

Page 35: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

• Kinetic Energy

• Potential Energy

• Total Energy

• Instantaneous Energy Density

Acoustic Energy Density

Page 36: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Spatial Dependence for a Rectangular Enclosure

Page 37: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

SP Nodal Structure

Page 38: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

ED Nodal Structure

Page 39: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

2D Sensor

•2D Sensor Effective When Placed Near

Wall or Ceiling

•Computationally More Efficient

Page 40: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

The Enclosure

•Potential

Application: Cab

Noise

•Enclosure Fairly

Representative of

Small Equipment

Cab

Page 41: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Sensor and Mic Placement

•ED Control Has Less Dependence on

Sensor Location

Page 42: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Noise Source and Subwoofer

Page 43: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

110 Hz Tone @ Sensor

Page 44: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

110 Hz @ Ear Location

Page 45: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Engine Tone Attenuation (dB)

46 Hz 90 Hz 110 Hz 120 Hz

12-Mic Avg 33.47 16.55 23.97 20.62

Right Ear 34.95 22.24 30.48 30.60

Left Ear 35.02 19.41 23.68 26.72

Sensor 34.49 22.58 32.92 32.05

Page 46: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Sound Level Reduction (dBA)

46 Hz 90 Hz 110 Hz 120 Hz

12-Mic Avg 4.11 0.39 6.12 2.77

Right Ear 3.84 0.60 8.71 4.75

Left Ear 4.27 0.57 8.70 4.69

Sensor 2.6 0.36 7.68 4.48

Page 47: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Cab Noise Findings

• Engine tones can be attenuated drastically

• Attenuation is achieved throughout cabin

• Significant reduction in total sound level is possible, even with A weighting

• Much can still be done with respect to performance optimization

50 Hz

Page 48: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Examples

• Heavy Equipment (Caterpillar)

– Wheel Loader Cab

– Focused on tonal noise at engine firing frequency

48

Page 49: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

49

Hardware Configuration

• Sub-woofer used for low frequencies

• Smaller drivers (10 cm) used for higher frequencies

• ED sensor mounted in convenient location

Page 50: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

50

Cab Response – Engine Sweep

• Results measured at nominal operator head location

Relative Lp

Relative Lp

50

25

0

50

25

0

Page 51: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

51

Control Results – Engine Sweep

Relative Lp

50

25

0

Relative Lp

50

25

0 0

Page 52: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

52

Engine Firing Freq – Engine Sweep

972H prototype - firing frequency Lp at left ear

40

50

60

70

80

90

100

950

1150

1350

1550

1750

1950

2150

rpm

Lp

(d

B)

ANC OFF

ANC ON

10 d

B/d

iv

Page 53: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

53

Cab Results – Global Response

-3.4 -2.2 0.1

-6.3 -6.4 -5.0

-8.1 -7.5 -5.2

operator

head

upper plane

front

0.2 0.9 -1.1

-2.5 -3.9 -1.3

-5.7 -5.0 -5.2

lower plane

Page 54: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Conclusions

• Active noise control is a viable solution for certain applications.

• Need to be careful in applying technology in order to achieve desired results.

• Good understanding of physics of application necessary for proper implementation.

• Technology starting to find its way into real applications – cost is still an issue but it has come way down.

Page 55: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Current Applications

• Honda 2005 Odyssey and Accord Hybrid

• Lexus

• Accura

• Saab commuter jet

• Active headsets

• BMW working on implementing an ANC system

Page 56: Active Noise Control: Is it Good for Anything? · Dept. of Physics & Astronomy Brigham Young University April 2, 2012 . May 22-23, 2011 Physics and Astronomy Department Size 32 Faculty

May 22-23, 2011

Special Thanks To . . .

• Kent Gee

• Ben Faber

• Brian Monson

• Connor Duke

• Ben Shafer

• Jared Thomas

• Stephan Lovstedt

• The BYU Acoustics Research Group