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holographic loudspeaker testing assessing radiated sound in 3 d space fundamentals applications The complex transfer function H(f,r) relating loudspeaker input u(t) to sound pressure p(r) at a particular point r under free field conditions, is described by the sum of orthonormal basis func- tions B(f,r) and it’s weighting complex coefficients C(f). Spherical Wave Expansion measurement The basis functions B(f,r) are general solutions of the wave equation in spherical coordinates, comprising Hankel functions of the second kind h n (2) and spherical harmonics Y n m . The coeffi- cients c nm (f) and the maximum order N of the expansion depend on the properties of the speci- fic loudspeaker being tested. Coefficients Basis functions Orthogonal Decomposition The decomposition into orthogonal basis functions B(f,r) provides a comprehensive re- presentation of the 3D output without redun- dancy. The maximum required order N of the expansion depends on the complexity of the directivity pattern generated by the loud- speaker. The total sound power generated by a compact sound source at low frequencies can be described by a low order of expansion (N=3) where the monopole (n=0), dipoles (n=1) and quadrupoles (n=2) are dominant. Total sound power and contribution of nth-order terms in wave expansion The sound field is measured using two cylindrical or hemispherical surfaces in the device’s near field. While still generating the same angular resolution of the directivity pattern, the hologra- phic approach requires a lower number of measurement points than traditional techniques. Near Field Scanning Number of points 1 100 1000 5000 Application on axis response sound power directivity professional systems Compact source Transducer in a baffle Line source The measurement of sound pressure in the near field, provides accurate amplitude and phase in- formation with a high signal to noise ratio (SNR) by minimizing the impact of air convection and temperature variation on the propagating sound wave. To ensure constant interaction between the loudspeaker and the room, the microphone is moved around the loudspeaker on two cylin- drical scanning surfaces, instead of rotating the loudspeaker on a turntable. This is required in order to separate the direct sound from the room reflections and will simplify the measurement of heavy loudspeakers. Microphone R-Axis Z-Axis Phi-Axis Parameter Identification + - + u(f) H(f,r i ) p meas (r i ) e Wave Expansion p mod (r i ) order of expansion N B 1 (r i ) B 2 (r i ) B n (r i ) C 1 C 2 C n Double layer scanning produces redundant data, which is used to check the accuracy of the mea- surements. The fitting error E fit evaluates the similarity between measured pressure p meas (r i ) and modeled pressure p mod (r i ) at all measurement points r i . A fitting error below 1% (-20dB) indicates good results. At high frequen- cies where this threshold is not met, a higher expansion order may be needed. Outside the loudspeaker’s passband (f < 30 Hz) the fitting error is caused by a poor signal to noise ratio (SNR) . Accurate far field data can be determined by only performing a single measurement and by using correction curves. For any loudspeaker (1) correction curves can be easily generated by comparing the total sound pressure (direct sound and room) at the microphone position r 0 and the direct sound pressure (no room effects) calculated using the full scan data and holographic processing. The correction curve can be applied to other loudspeakers (2) of similar geometry with the same loudspeaker and microphone position in the room. Single Point SPL Measurement f in Hz sound power in dB Total Sound Power Higher orders n=0 n=1 n=2 n=3 90 80 70 60 50 40 30 20 10 0 100 1k KLIPPEL N=0 N=1 N=2 N=3 N=5 N=10 Fitting error f in Hz error in dB Noise Floor -20dB =1% 5 0 -5 -10 -15 -20 -25 -30 -35 -40 -45 -50 -55 -60 100 1k 10k Far Field Characteristics The frequency response of the loudspeaker at any point in the far field can be extrapolated from near field data. On Axis 30° Off Axis 60° Off Axis f in Hz sound power in dB SPL in dB directivity index in dB f in Hz f in Hz Frequency Response Sound Power Directivity Index 85 80 75 70 65 60 55 50 45 40 35 110 105 100 95 90 85 80 75 70 65 60 14 12 10 8 6 4 2 0 100 1k 10k 100 1k 10k Traditional directional characteristics are calculated based on the wave expansion and can be exported to external sound field simulation software with any desired angular resolution (e.g. 1°). 3D Directivity -180° -160° -140° -120° -100° -80° -60° -40° -20° 20° 40° 60° 80° 100° 120° 140° 160° 180 ° 100 1k 10k f in Hz theta in degree Contour Plot Polar Plot Directivity Balloon Coverage Angle Near Field Characteristics Near field characteristics are especially relevant for studio monitors, smart phones, laptops and other personal audio devices. An observation plane can be positioned in 3D space to investigate the spatial SPL distribution in the near field of the audio device. The holographic measurement provides accurate phase information to compute the wave propa- gation into the far field, helping visualize the binaural perception of sound. Magnitude Phase 3kHz 3kHz Sound pressure distribution Wave front propagation Simplified Interpretation The CEA 2034 standard specifies meaningful loudspeaker responses at specific points, for home applications. This is helpful when considering the interaction with a room and when comparing loudspeakers regarding their performance at defined listening positions. Listening Window Early Reflections CEA 2034 Characteristics f in Hz SPL in dB 110 105 100 95 90 85 80 75 70 65 60 100 1k 10k dB Directivity Index 15 10 5 0 Testing personal audio devices, the IEC 62777 standard specifies the meaningful characteristics in personal acoustic zones in the near field of the sound source. IEC62777 – Personal Acoustic Zones f in Hz SPL in dB 105 100 95 90 85 80 75 70 65 60 55 50 100 1k 10k PF (Front) Distributed Sound Sources The directivity of distributed sound sources (line arrays, sound bars) can be determined by measuring each individual transducer of the loudspeaker system. Thereby, the measured cha- racteristic of each transducer also includes shadowing and diffraction effects of the loudspea- ker cabinet. After holographic processing, the total radiated sound pressure is calculated by superimposing the individual sound sources. By applying separate filters on each transducer (e.g. delay, gain), the directivity of the active system can easily be controlled (beam steering). -180° -160° -140° -120° -100° -80° -60° -40° -20° 20° 40° 60° 80° 100° 120° 140° 160° 180 ° 100 1k 10k theta -6dB -12dB -18dB 30 40 50 60 70 80 90 100 100 1k 10k Near Field DUT + Room Direct Sound Near Field Direct Sound Far Field 100 1k 10k KLIPPEL -30 -28 -26 -24 -22 -20 -18 -16 100 1k 10k -15 -10 -5 0 5 10 15 25 30 35 40 45 50 55 60 65 70 75 100 1k 10k 50 55 60 65 70 75 80 85 90 95 100 100 1k 10k 50 55 60 65 70 75 80 85 90 95 100 100 1k 10k Single Measurement (non anechoic) Near Field Response (Free Field) Far Field Response (Free Field) Room correction curve Near Field correction curve Reference Measurement Speaker 2 Speaker 1 + 1. Scanning each transducer output 2. Separate wave expansions 3. Superposition of all expansions On Axis PU (Front-Upper) PB (Rear) PD (Front-Lower) PL (Front-Left) PR (Front-Right) Sound Power Early Reflections Sound Power DI Multiplexer + + + ... ... + REFERENCES Earl G. Williams: Fourier Acoustics – Sound Radiation and Nearfield Acoustical Holography, 1999 Academic Press, ISNG 0-12-753960-3 IEC (E) 60268-Xa Draft: Part A - Acoustical Measurements, 2015 International Electrotechnical Commission IEC 62777 Ed.1: Quality Evaluation Method for the Sound Field of Directional Loudspeaker Array System, 2014 International Electrotechnical Commission www.klippel.de f in Hz f in Hz f in Hz f in Hz f in Hz f in Hz f in Hz SPL in dB SPL in dB SPL in dB SPL in dB SPL in dB SPL in dB Sound Separation Higher-order terms are required to model the directivity at higher frequencies in order to achieve sufficient angular resolution and accuracy. target N=0 N=1 N=2 N=5 N=10 Target directivity of a loudspeaker at f=2kHz (left) approximated by wave expansions truncated at maximum order N=10 Measurements of the sound pressure gene- rated by a loudspeaker in a non-anechoic environment show interference between the direct sound component and the reflections produced by the room (e.g. walls). At high fre- quencies the direct sound can be isolated by windowing the impulse response. At low fre- quencies the windowing technique requires a large distance between the speaker and the reflecting boundaries in order to provide suf- ficient spectral resolution. 100 1k 10k Sound Separation by time windowing f in Hz SPL in dB Sound Separation by holographic processing Room Reflections Measured Sound Direct Sound Reflection Free Frequency Holographic processing of the sound pressure data, scan- ned in two layers, separates the radiated direct sound w rad from the reflections w in , w trans and w scat . Sound Field Extrapolation Apparent sound power of the spherical waves of order n>0 decreases in the near field and stays constant in the far field of the sound source. near field far field holographic extrapolation H(f,r)=C(f) B(f,r) 115 110 105 100 95 90 85 80 75 70 65 100 1k 10k distance sound power in dB 0.1m 1m 10m n=0 n=3 n=5 n=7 n=10 n=9 n=8 monopole order n of the spherical waves Near Field Far Field 300 250 200 150 100 50 0 -50 0.1m 1m 10m In the near field the 1/r law is not valid due to the phase shift between the sound pressure and velocity, which increases the apparent sound power for small values of r. The spherical wave expansion can describe the sound pressure at any point in 3D space outside the scanning surface (near and far field). In the far field, the sound pressure p is directly pro- portional to the distance r and can be calculated using the 1/r law: „Doubling the distance reduces the sound pressure level by 6dB“. r r far a p ~ 1/r 100 1k 10k Reference Measurement (Full Scan) CEA-2034: Standard Method of Measurement for In-Home Loudspeakers, 2013 Consumer Electronics Association G. Weinreich, E. B. Arnold: Method for measuring acoustic radiation fields, J. Acoust. Soc. Am., 68 (2), 404–411, 1980 M. Melon, C. Langrenne, A. Garcia: Measurement of subwoofers with the field separation method: comparison of p- p and p-v formulations, C.-X. Bi, D.-Y. Hu, L. Xu and Y.-B. Zhang: Recovery of the free field using the spherical wave superposition method, Acoustics 2012 Nantes, 1781-1786, 2012 Z. Wang, S. F. Wu: Helmholtz equation-least-squares method for reconstructing the acoustic pressure field, J. Acoust. Soc. Am., 102 (4), 2020-2032, 1997S. Wu, H. Lu, S. Wu, D. B. Keele: High-Accuracy Full-Sphere Electro Acoustic Polar Measurements at High Frequencies using the HELS Method, Audio Eng. Soc. October 2006, Convention Paper 6881 D. B. Keele: Low Frequency Loudspeaker Assessment by Nearfield Sound- Pressure Measurement, J. of the Audio Eng. Soc., April 1974, Vol. 22, No. 3 C. Bellmann, W. Klippel, D. Knobloch: Holographic loudspeaker measurement based on near field scanning, DAGA 2015 - 41th Convention, DEGA e.V. Near Field Scanner 3D (NFS), Specification C8, 2015 Klippel GmbH, www.klippel.de Cone Vibration and Radiation Diagnostics, Application Note AN 31, 2012 Klippel GmbH, www.klippel.de
Transcript

holographic loudspeaker testingassess ing radiated sound in 3d space

fundamentals appl icat ions

The complex transfer function H(f,r) relating loudspeaker input u(t) to sound pressure p(r) at a particular point r under free field conditions, is described by the sum of orthonormal basis func-tions B(f,r) and it’s weighting complex coefficients C(f).

Spherical Wave Expansion

measurement

The basis functions B(f,r) are general solutions of the wave equation in spherical coordinates, comprising Hankel functions of the second kind hn

(2) and spherical harmonics Ynm. The coeffi-

cients cnm (f) and the maximum order N of the expansion depend on the properties of the speci-fic loudspeaker being tested.

Coefficients Basis functions

Orthogonal Decomposition

The decomposition into orthogonal basis functions B(f,r) provides a comprehensive re-presentation of the 3D output without redun-dancy. The maximum required order N of the expansion depends on the complexity of the directivity pattern generated by the loud-speaker. The total sound power generated by a compact sound source at low frequencies can be described by a low order of expansion (N=3) where the monopole (n=0), dipoles (n=1) and quadrupoles (n=2) are dominant.

Total sound power and contribution of nth-order terms in wave expansion

The sound field is measured using two cylindrical or hemispherical surfaces in the device’s near field. While still generating the same angular resolution of the directivity pattern, the hologra-phic approach requires a lower number of measurement points than traditional techniques.

Near Field Scanning

Numberof points

1

100

1000

5000

Application

on axis response

sound power

directivity

professional systems Compact source Transducer in a baffle Line source

The measurement of sound pressure in the near field, provides accurate amplitude and phase in-formation with a high signal to noise ratio (SNR) by minimizing the impact of air convection and temperature variation on the propagating sound wave. To ensure constant interaction between the loudspeaker and the room, the microphone is moved around the loudspeaker on two cylin-drical scanning surfaces, instead of rotating the loudspeaker on a turntable. This is required in order to separate the direct sound from the room reflections and will simplify the measurement of heavy loudspeakers.

Microphone

R-Axis

Z-Ax

is

Phi-Axis

Parameter Identification

+-

+

u(f)

H(f,ri)pmeas(ri) e

Wave Expansion

pmod(ri)

order ofexpansion N

B1(ri)

B2(ri)

Bn(ri)

C1

C2

Cn

Double layer scanning produces redundant data, which is used to check the accuracy of the mea-surements. The fitting error Efit evaluates the similarity between measured pressure pmeas(ri) and modeled pressure pmod(ri) at all measurement points ri.

A fitting error below 1% (-20dB) indicates good results. At high frequen-cies where this threshold is not met, a higher expansion order may be needed. Outside the loudspeaker’s passband (f < 30 Hz) the fitting error is caused by a poor signal to noise ratio (SNR) .

Accurate far field data can be determined by only performing a single measurement and by using correction curves. For any loudspeaker (1) correction curves can be easily generated by comparing the total sound pressure (direct sound and room) at the microphone position r0 and the direct sound pressure (no room effects) calculated using the full scan data and holographic processing. The correction curve can be applied to other loudspeakers (2) of similar geometry with the same loudspeaker and microphone position in the room.

Single Point SPL Measurement

f in Hz

soun

d po

wer

in d

B

Total Sound Power

Higher orders

n=0

n=1n=2

n=3

90

80

70

60

50

40

30

20

10

0100 1k

KLIPPEL

-60

-55

-50

-45

-40

-35

-30

-25

-20

-15

-10

-5

0

5

100 1k 10k

N=0

N=1

N=2N=3N=5

N=10

Fitting error

f in Hz

erro

r in

dB

Noise Floor

-20dB

=1%

5

0

-5

-10

-15

-20

-25

-30

-35

-40

-45

-50

-55

-60

100 1k 10k

Far Field Characteristics

The frequency response of the loudspeaker at any point in the far field can be extrapolated from near field data.

On Axis

30° Off Axis

60° Off Axis

f in Hz

soun

d po

wer

in d

B

SPL

in d

B

dire

ctiv

ity in

dex

in d

B

f in Hz f in Hz

Frequency Response Sound Power Directivity Index

85

80

75

70

65

60

55

50

45

40

35

110

105

100

95

90

85

80

75

70

65

60

14

12

10

8

6

4

2

0

100 1k 10k 100 1k 10k

Traditional directional characteristics are calculated based on the wave expansion and can be exported to external sound field simulation software with any desired angular resolution (e.g. 1°).

3D Directivity

-180°

-160°

-140°

-120°

-100°

-80°

-60°

-40°

-20°

20°

40°

60°

80°

100°

120°

140°

160°

180°

100 1k 10k

f in Hz

thet

a in

deg

ree

Contour Plot Polar Plot Directivity Balloon Coverage Angle

Near Field Characteristics

Near field characteristics are especially relevant for studio monitors, smart phones, laptops and other personal audio devices. An observation plane can be positioned in 3D space to investigate the spatial SPL distribution in the near field of the audio device.The holographic measurement provides accurate phase information to compute the wave propa-gation into the far field, helping visualize the binaural perception of sound.

Magnitude Phase

3kHz 3kHz

Sound pressure distribution Wave front propagation

Simplified Interpretation

The CEA 2034 standard specifies meaningful loudspeaker responses at specific points, for home applications. This is helpful when considering the interaction with a room and when comparing loudspeakers regarding their performance at defined listening positions.

ListeningWindow

EarlyReflections

CEA 2034 Characteristics

f in Hz

SPL

in d

B110

105

100

95

90

85

80

75

70

65

60100 1k 10k

dB D

irec

tivity

Inde

x

15

10

5

0

Testing personal audio devices, the IEC 62777 standard specifies the meaningful characteristics in personal acoustic zones in the near field of the sound source.

IEC62777 – Personal Acoustic Zones

f in Hz

SPL

in d

B

105

100

95

90

85

80

75

70

65

60

55

50

100 1k 10k

PF (Front)

Distributed Sound Sources

The directivity of distributed sound sources (line arrays, sound bars) can be determined by measuring each individual transducer of the loudspeaker system. Thereby, the measured cha-racteristic of each transducer also includes shadowing and diffraction effects of the loudspea-ker cabinet. After holographic processing, the total radiated sound pressure is calculated by superimposing the individual sound sources. By applying separate filters on each transducer (e.g. delay, gain), the directivity of the active system can easily be controlled (beam steering).

-180°

-160°

-140°

-120°

-100°

-80°

-60°

-40°

-20°

20°

40°

60°

80°

100°

120°

140°

160°

180°

100 1k 10k

thet

a

- 6 dB

-12dB

-18dB

30

40

50

60

70

80

90

100

100 1k 10k

Near Field DUT + Room

Direct Sound Near Field

Direct Sound Far Field

100 1k 10k

KLIPPEL

-30

-28

-26

-24

-22

-20

-18

-16

100 1k 10k-15

-10

-5

0

5

10

15

25

30

35

40

45

50

55

60

65

70

75

100 1k 10k50

55

60

65

70

75

80

85

90

95

100

100 1k 10k50

55

60

65

70

75

80

85

90

95

100

100 1k 10k

Single Measurement (non anechoic) Near Field Response (Free Field) Far Field Response (Free Field)

Room correction curve Near Field correction curve

Reference Measurement

Speaker 2

Speaker 1

+

1. Scanning each transducer output 2. Separate wave expansions 3. Superposition of all expansions

On Axis

PU (Front-Upper)

PB (Rear)

PD (Front-Lower)

PL (Front-Left) PR (Front-Right)

Sound Power

Early Reflections

Sound Power DI

Mul

tiple

xer

+

+

+

......

+

RefeRences

Earl G. Williams: Fourier Acoustics – Sound Radiation and Nearfield Acoustical Holography, 1999 Academic Press, ISNG 0-12-753960-3

IEC (E) 60268-Xa Draft: Part A - Acoustical Measurements, 2015 International Electrotechnical Commission

IEC 62777 Ed.1: Quality Evaluation Method for the Sound Field of Directional Loudspeaker Array System, 2014 International Electrotechnical Commission

www.klippel.de

f in Hz

f in Hz

f in Hzf in Hz

f in Hz f in Hz f in Hz

SPL

in d

B

SPL

in d

B

SPL

in d

B

SPL

in d

B

SPL

in d

B

SPL

in d

B

Sound Separation

Higher-order terms are required to model the directivity at higher frequencies in order to achieve sufficient angular resolution and accuracy.

target N=0 N=1 N=2 N=5 N=10

Target directivity of a loudspeaker at f=2kHz (left) approximated by wave expansions truncated at maximum order N=10

Measurements of the sound pressure gene-rated by a loudspeaker in a non-anechoic environment show interference between the direct sound component and the reflections produced by the room (e.g. walls). At high fre-quencies the direct sound can be isolated by windowing the impulse response. At low fre-quencies the windowing technique requires a large distance between the speaker and the reflecting boundaries in order to provide suf-ficient spectral resolution.

65

70

75

80

85

90

95

100

105

110

115

100 1k 10k

Sound Separation by time windowing

f in Hz

SPL

in d

B

Sound Separation by holographic processing

Room Reflections

Measured Sound

Direct Sound

Refle

ctio

n Fr

ee F

requ

ency

Holographic processing of the sound pressure data, scan-ned in two layers, separates the radiated direct sound wrad from the reflections win, wtrans and wscat.

Sound Field Extrapolation

Apparent sound power of the spherical waves of order n>0 decreases in the near field and stays constant in the far field of the sound source.

near field far field

holographic extrapolation

H(f,r)=C(f) B(f,r)

115

110

105

100

95

90

85

80

75

70

65

100 1k 10k

distance

soun

d po

wer

in d

B

-50

0

50

100

150

200

250

300

0.1m 1m 10m

n= 0n= 3n= 5

n= 7

n=10n= 9n= 8

monopole

order n of thespherical waves

Near Field Far Field

300

250

200

150

100

50

0

-50

0.1m 1m 10m

In the near field the 1/r law is not valid due to the phase shift between the sound pressure and velocity, which increases the apparent sound power for small values of r. The spherical wave expansion can describe the sound pressure at any point in 3D space outside the scanning surface (near and far field).

In the far field, the sound pressure p is directly pro-portional to the distance r and can be calculated using the 1/r law: „Doubling the distance reduces the sound pressure level by 6dB“.

rrfara

p~1/r

100 1k 10k

Reference Measurement (Full Scan)

CEA-2034: Standard Method of Measurement for In-Home Loudspeakers, 2013 Consumer Electronics Association

G. Weinreich, E. B. Arnold: Method for measuring acoustic radiation fields, J. Acoust. Soc. Am., 68 (2), 404–411, 1980

M. Melon, C. Langrenne, A. Garcia: Measurement of subwoofers with the field separation method: comparison of p- p and p-v formulations,

C.-X. Bi, D.-Y. Hu, L. Xu and Y.-B. Zhang: Recovery of the free field using the spherical wave superposition method, Acoustics 2012 Nantes, 1781-1786, 2012

Z. Wang, S. F. Wu: Helmholtz equation-least-squares method for reconstructing the acoustic pressure field, J. Acoust. Soc. Am., 102 (4), 2020-2032, 1997S. Wu,

H. Lu, S. Wu, D. B. Keele: High-Accuracy Full-Sphere Electro Acoustic Polar Measurements at High Frequencies using the HELS Method, Audio Eng. Soc. October 2006, Convention Paper 6881

D. B. Keele: Low Frequency Loudspeaker Assessment by Nearfield Sound-Pressure Measurement, J. of the Audio Eng. Soc., April 1974, Vol. 22, No. 3

C. Bellmann, W. Klippel, D. Knobloch: Holographic loudspeaker measurement based on near field scanning, DAGA 2015 - 41th Convention, DEGA e.V.

Near Field Scanner 3D (NFS), Specification C8, 2015 Klippel GmbH, www.klippel.de

Cone Vibration and Radiation Diagnostics, Application Note AN 31, 2012 Klippel GmbH, www.klippel.de

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