Vibration Testing & Modal Identification Jean-Claude Golinval
Transcript of Vibration Testing & Modal Identification Jean-Claude Golinval
Vibr
ationTe
sting
& M
odal I
dent
ificat
ion
Vibration Testing & Modal Identification
Jean-Claude GolinvalReferences
• D. J. EWINS
Modal Testing : theory, practice and application
Second Edition, Research Studies Press LTD, 2000
ISBN 0 86380 218 4
• N. MAIA, J. SILVA
Theoretical and Experimental Modal Analysis
Research Studies Press LTD, 1997
ISBN 0 86380 208 7
2Two Routes to Vibration Analysis
Description of the structure in terms of its mass, stiffness and
damping properties
Theoretical Approach – Direct Problem
Experimental Approach – Inverse Problem
Structural Model Modal Model Response Model
Response Measurements
Modal Model (Identification) Structural Model
Natural frequencies, Modal damping factors,
Mode shapes
Frequency Response Functions, Impulse Response Functions
3
Définition
Développement d ’un modèle mathématique du comportement dynamique d ’une structure à partir de tests expérimentaux.
Relation fondamentale
Réponse Excitation Propriétés du système= ×
Bref historiqueAvant 1947 : mesures de la réponse seule
1947 : mesures de la réponse et de l ’excitation Kennedy, Pancu : mesures des fréquences de résonance et de l ’amortissement de structures d ’avions.
1960-70 : progrès techniques des moyens de mesures (capteurs, électronique, …) et d ’acquisition (analyseurs de spectre digitaux)
1965 : algorithme FFT (Cooley et Tukey)
Analyse et identification modale
4Single-Degree-Of-Freedom (SDOF) System
Governing equation of motion
the trial solution :
Roots :
)(tfxkxcxm =++
teXtx λ=)(
200
2
2,1 12
42
ζωωζλ −±−=−
±−= im
mkcmc
wheremm
k
00 2
candω
ζω ==
Natural frequency Viscous damping ratio
In case of no external forcing ( f(t) = 0,
leads to the requirement that : 02 =++ kcm λλ
5
Free vibration characteristic of damped SDOF system )1( <ζ
tit eeXtx2
00 1)( ζωζω −−=
Forced response to harmonic excitation: tieFtf ω=)(
)()()( ωωω FHX =
⎟⎠
⎞⎜⎝
⎛+⎟⎠
⎞⎜⎝
⎛ −=
+−=
020
22
21
11)()(
1)(
ωωζ
ωωωω
ωi
kcimkH
Frequency Response Function (FRF)
6
Alternative Forms of FRF
Force Structure Response
Displacement
Velocity
Acceleration
Standard FRF Inverse FRF
Displacement Receptance Admittance
Dynamic stiffness
Velocity Mobility Mechanical impedance
Acceleration Accelerance Inertance
Apparent mass
FRF = Response / Force
7
Graphical Displays of FRF Data
The FRF is a complex quantity.
))(())(( ωω HiHH ℑ+ℜ=Real Part Imaginary Part
Frequency
The most common forms of presentation are:
• Bode plot: Modulus and Phase of FRF vs. Frequency (2 graphs);
• Nyquist plot: Imaginary Part (of FRF) vs. en Real Part (of FRF) (a single graph which does not contain frequency information explicitely);
• Cartesian plots: Real Part (of FRF) vs. Frequency and Imaginary Part (of FRF) vs. Frequency (2 graphs);
8
• Bode Plot
Linear scales Log-Log scales
Receptance Mass Stiffness
)log()log(2)log())(log(/1/1)( 2
kmHkmH
−−−−
ωωωω
9
• Nyquist Plot
)(ωH
)(ωφ
• Cartesian Plots
Real Part
Imaginary Part
10
• Three-dimensional plot of SDOF system FRF
11Multi-Degree-Of-Freedom Systems
Governing equation of motion
)(tfqKqCqM =++
q = vector of displacements
f(t) = vector of forces
M = mass matrix
K = stiffness matrix
C = damping matrix
M, K and C constitute the Spatial Model.
12
Undamped MDOF SystemsFree Vibration Solution – The Modal Properties
The undamped system’s natural frequencies are the solutions of
and the corresponding mode shapes are the solutions of
02 =− MK ωdtm
( ) ( ) 02 =− rr ψMK ω
N eigensolutions
( ) ( ) ( )N
N
ψψψ 21
ωωω ≤≤≤ 21
0=+ xKxM
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[ ][ ]r
Tr
T
k
m
=
=
ΨKΨΨMΨ
Orthogonality properties:
Let us define
( ) ( ) ( )[ ][ ] [ ]22
221
221
Nr
N
diag ωωωω =
= ψψψΨ Modal matrix
Spectral matrix
[ ]2rωandΨ constitute the Modal Model.
Modal mass matrix
Modal stiffness matrix
[ ] [ ] [ ]rrr km 12 −=ωAnd thus
14
Orthogonality properties:
in which case, the mass-normalised eigenvectors are written as
( ) ( ) ( )[ ]NxxxX 21= Mass-normalised modal matrix
Remark :Mass-normalisation is the most relevant scaling in modal testing, i.e.
[ ] [ ]1=rm
[ ][ ]2
rT
T
ω=
=
XKX
1XMX
15
Forced Response Solution – The FRF Characteristics
tiet ωFfqKqM ==+ )(
Solution of the form: tie ωQq =
Modal transformation: ( ) aXxQ ==∑=
k
N
kka
1
The equations of motion then becomes: ( ) FaXMK =− 2ω
Premultiply both sides by to obtainTX
[ ] [ ]( ) FX1XQ Tr
122 −−= ωωwhich leads to
[ ] [ ] FXa1 Tr =⎟
⎠⎞
⎜⎝⎛ − 22 ωω
16
[ ] [ ]( ) Tr X1XH
122)(−
−= ωωω
From the definition of the FRF matrix, it follows that:
( ) ( )[ ]( )
( )⎥⎥⎥
⎦
⎤
⎢⎢⎢
⎣
⎡
⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢
⎣
⎡
−=
TN
T
rN
x
xxxH
1
2211
ωω
Hence the spectral representation of the FRF matrix:
( ) ( )∑= −
=N
k k
Tkk
122)(
ωωω
xxH
17
Any individual FRF coefficient linking coordinates r and s (called dynamic influence coefficient) is written:
( )( ) skrkkrs
N
k k
krsrs A
AH φφ
ωωω =
−= ∑
=with
122)(
Modal Constant (or Residue)
Natural Frequency
(Pole)
18
Damped Systems)(tfqKqCqM =++
Modal transformation: ( ) ( ) ηXxq == ∑=
k
N
kkt
1η
Modal matrix
Pre-multiplying the equation of motion by TX
[ ] ( ) [ ] )()()( ttkttm Tr
Tr fXηXCXη =++ η
Modal damping matrix
19
Proportional Damping
In this case, the matrix is diagonal
where [ck] = modal damping matrix.
[ ]kT c=XCX
Using the notation introduced above for the SDOF analysis, the damping coefficient of mode k is written in the form:
kkkk mc ωζ2=
The forced response to an harmonic excitation
tie ωFqKqCqM =++
is in the form:tie ωQq =
Modal transformation: ( ) aXxQ == ∑=
k
N
kka
1
20
Thus, the equation of motion takes the form:
( ) FaXCMK =+− ωω i2
Pre-multiplying par , we have:TX
[ ] [ ] [ ]( ) FX1XQ Tkkk i
122 2−
+−= ωζωωω
[ ] [ ] [ ] FXa1 Tkkk i =⎟⎠⎞
⎜⎝⎛ +− ωζωωω 222
[ ] [ ] [ ]( ) Tkkk i X1XH
122 2)(−
+−= ωζωωωωWe obtain:
and the expression of the FRF matrix is:
( ) ( )∑= +−
=N
k kkk
Tkk
i122 2
)(ωωζωω
ωxx
H
21
The receptance frequency response function (FRF) at coordinate r , resulting from a single force applied at coordinate s , is :
( )( ) ( ) ( )kskrkrs
N
k kkk
krsrs A
i
AH xx=
+−= ∑
=with
122 2
)(ωωζωω
ω
Example:
22
Particular form of proportional damping
MKC γβ +=
In this case, the eigenvalues and eigenmodes take the form:
undampeddamped
kkk
kkdk
XX =
⎟⎟⎠
⎞⎜⎜⎝
⎛+=
−=
ωγωβζ
ζωω
21
1 2 kζ
kω
0=β
0=γ
23
Viscous damping (General case)
In this case, the matrix is not diagonal anymore.
Consider the homogeneous system:
It can be shown that the eigensolutions of the appropriate equation
occur as complex conjugates.
XCXT
0qKqCqM =++
( ) 02 =++ QKCM λλ
( ) ( )Nk
kk
kk ,,1,
,*
*
=⎪⎭
⎪⎬⎫
ψψ
λλ
with: ⎟⎠⎞⎜
⎝⎛ −+−= 21 kkkk i ζζωλ
This approach is not particularly convenient for numerical application.
24
In the general case of viscous damping, it is better to recast the equations into the state-space form:
⎪⎩
⎪⎨⎧
=−=++
0qMqMFqKqCqM tie ω
or tie ω
⎭⎬⎫
⎩⎨⎧
=⎭⎬⎫
⎩⎨⎧
⎥⎦
⎤⎢⎣
⎡−
+⎭⎬⎫
⎩⎨⎧
⎥⎦
⎤⎢⎣
⎡0F
M00K
0MMC
A B+u u tie ωP=
A and B are real and symmetric matrices of dimension 2N x 2N.
25
Homogeneous equation:
Solution of the form:
Eigenvalue problem:
2N eigenvalues and eigenvectors verifying the orthogonality properties:
0uBuA =+
teλUu =
( ) 0zBA =+λ
kλ ( )kz
[ ][ ]k
Tk
T
b
a
=Β
=
ZZ
ZAZ
and which have the usual characteristic that
)2,,1(; Nkab
k
kk =−=λ
26
Forced response to harmonic excitationtie ωPuBuA =+
Development in the series of eigenmodes:
( )∑=
=N
kk
tik e
2
1zu ωη
Substituting into the state-space equation and pre-multiplying by we have:
( )Tkz
( ) )2,,1( Nkbai Tkkkkk ==+ Pzηηω
( ) )2,,1()(
Nkia kk
Tk
k =−
=λω
ηPz
Thus, the solution may be written as:
( ) ( ) tiN
k kk
Tkk e
iaω
λω∑= −
=2
1 )(Pzz
u
27
( ) ( ) ( ) ( ) Pzzzz
Q
Q
⎟⎟
⎠
⎞
−+
⎜⎜
⎝
⎛
−=
⎪⎭
⎪⎬
⎫
⎪⎩
⎪⎨
⎧
∑= )()(1 kk
TkkN
k kk
Tkk
iaiai λωλωω
However, because the eigensolutions occur in complex conjugate pairs, the solution may be rewritten as:
If we extract the response vector Q, we obtain the expression of the FRF matrix in the form:
( ) ( ) ( ) ( ))()(1 kk
TkkN
k kk
Tkk
iaia λωλω −+
−= ∑
=
zzzzH
28
A single response parameter takes the form:Modal constants
(Residues)
( ) ( ) ( ) ( )∑= −
+−
=N
k kk
kskr
kk
kskrrs iaia
H1 )()(
)(λωλω
ωzzzz
Poles (complex)
( ) ( ) ( ) ( ))()(1 kk
TkkN
k kk
Tkk
iaia λωλω −+
−= ∑
=
zzzzH
29
Complex Modes
Real mode: in-phase vibration, (standing wave)
Complex mode: out-of-phase vibration (travelling wave)
Measurement of modal complexity (complex mode shapes plotted on Argand diagrams)
30
Example:
31
a) Undamped systems
b) Damped systems (proportional damping)
c) Damped systems (general case of viscous damping)
( ) ( ) ( ) ( )∑=
−+
−=
N
k kk
kskr
kk
kskrrs iaia
H1
)()()(
λωλωω
zzzz
( )( ) ( ) ( )kskrkrs
N
k kkk
krsrs A
i
AH xx=
+−=∑
=
with1
22 2)(
ωωζωωω
( )( ) ( ) ( )kskrkrs
N
k k
krsrs A
AH xx=
−=∑
=
with1
22)(ωω
ω
The fundamental relations used for experimental modal analysis are:
Summary
32FRF Measurement TechniquesTest Planning
• Definition of the objectives
- estimation of vibration amplitude levels
- estimation of natural frequencies, mode shapes and damping factors
- model validation
• Selection of the frequency range
• Selection of measurement and excitation coordinates
• Selection of excitation devices and transducers
• Selection of the support points (to minimise external influence)
• Checking the quality of measured data
• Measured data consistency, including reciprocity
• Measurement repeatability
• Measurement reliability
33
General Layout of FRF Measurement System
Excitation mechanism
Transduction systemAnalyser
34
• Mechanical Exciters
- little flexibility or control
Excitation of the Structure
35
• Electrohydraulic Exciters
- substantial forces are generated
- possibility to apply simultaneously a static load to the dynamicvibratory load
- large displacement amplitudes
- limited frequency range
- hydraulic shakers are complex and expansive
36
• Electrodynamic Exciters
37
Characteristics of a shaker
38
Example of grounded structure
Examples of freely-supported structure
39
Exciter attachment Various mounting arrangements for exciter
(a) Ideal configuration
(b) Suspended shaker plus inertia mass
(c) et (d) Compromise configurations
(b) Unsatisfactory assembly
(c) et (d) Acceptable assembly
(e) Use of a push rod or stinger
40
Example of electrodynamic shaker used for environmental testing (qualification, fatigue)
Gearing & Watson V2664
Max. force = 26.6 kN(sinus et random) ;
Max. displ. = 50 mm(peak-peak) ;
Max. velocity = 1.52 m/s.
41
• Piezoelectric exciters
- Operational at high frequency range
- Low excitation amplitude
• Non-Contact Magnetic Excitation
- Electromagnetic force
- Measurement of the reaction force on the body of the magnet (not directly the force applied to the structure)
- Application to rotating machinery
42
• Hammer Excitation
Tip
Head
Force gauge
43
(I) Stiff tip (steel)
(II) Medium tip (vinyl)
(III) Soft tip (rubber)
Duration of the pulse
= cut-off frequency
Typical impact force pulse and spectrum
44
Use of different excitation devices
45
Consider a sinusoidal signal
tXxtXx
tXxtFf
ωωωω
ωω
sinsin
sinsin
2−=
===
Signal Response parameter
XX
XF
2ωω
Force
Displacement
Velocity
Acceleration
24
25
/10/smmsmm
μμ
1Hz15800101Hz0,5
onacceleratintdisplacemefrequency−
Example:
Not detectable
Transducers
46
Choice of the physical quantity to be measured
• Displacement : measurement of gaps, orbits of rotor inside journals, thermal dilatations, …
• Velocity : used in standards to characterise vibration intensity
• Acceleration : measurement of high frequency signals (shocks)
acceleration
Vibration amplitude
velocitydisplacement
frequency
47
Vibration Transducers
Definition
Physical quantity
(force, displacement, velocity, acceleration)
absolute or relative
TRANSDUCER
(sensitivity)
Electrical quantity
(voltage, current, charge)
Specifications• Measurement Range (e.g. 0 to 10 g,
-1 mm to +1mm)
• Frequency Range (e.g. 1hz to 1,5 kHz)
• Sensitivity (e.g. 10 pC/g, 300 mV/(cm/s))
• Transverse Sensitivity
• Environmental:
- Magnetic Sensitivity (e.g. 0,1 g/tesla)
- Acoustic Sensitivity (e.g. 0,01 pC/db)
- Temperature Transient Sensitivity
• Physical
- Weight, Dimensions
• Mounting Techniques
48
Vibration Transducer Basics
Governing equation of motion
)()()( tfyxkyxcxm =−+−+
In terms of relative displacement
)()( tRymtfzkzczm =−=++
The forced response to harmonic excitation applied to the body (with f(t)=0) is written in the form
tieYty ω=)(
titi
eZcimk
eYmtz ωω
ωωω =
+−= 2
2
)(
( )( ) ( )2
022
02
20
21 ωωζωωωω+−
=YZ
20
20
12tan
ωωωωζφ
−=
amplitude phase
)(tx)(tz
)(ty
m
k
c
49
Displacement transducer
(sismographs)
yzYZ
−=⇒⎪⎩
⎪⎨
⎧
→
∀→>
°180
1,4
0 φ
ζωω have we For
When , the amplitude peak disappears 707,0=ζ
50
Design requirement: <<<0ω
k low
m highTransducer is relatively large and heavy
Example: LVDT (Linear Variable Differential Transformer)
Frequency Range: < 500 Hz
51
Velocity Transducer (same working principles as for the displacement transducer)
Practical example
Advantages:
- reliability, robustness (no power supply needed)
- high sensitivity (e.g. 300 mV/(cm/s))
- low impedance (no conditioning amplifier needed)
Drawbacks: - heavy and large, frequency range < 2000 Hz
tU
te
∂∂=
∂∂−= λφ
Voltage Magnetic flux
52
Accelerometers
titi
eZcimk
eYmtz ωω
ωωω =
+−= 2
2
)(
( ) ( )20
220
22
20
21
1
ωωζωωωω
+−=
YZ
20
20
12tan
ωωωωζφ
−=
Amplitude
Phase
System response:
53
Measurement of the acceleration of the support
( )YkmYZ 2
20
2
0
,0 ωω
ωωω −=−→→ get we As
Acceleration of the supportAccelerometer
sensitivity
Design requirement: >>>0ω
k high
m small
Transducer is small and light
Sensitivity seismic mass÷
Optimise the choice for any
given application
( ) ( )20
220
22
20
21
1
ωωζωωωω
+−=
YZ
Amplitude:
54
Typical examples of piezoelectric accelerometers
yQ 1λ=
Sensitivity in pC/g
55
Advantages:
- high frequency range
- excellent linearity
- low sensitivity to environmental noises
- small size, lightness
Drawbacks:
- very high impedance
charge amplifier
Selection of accelerometers
56
Attachment and location of accelerometers
57
Force Transducers Impedance Heads
Combination of 2 transducers: force + acceleration
58
Laser Transducers
• Laser Doppler velocimeter (LDV)
− Characteristics for a typical device:
− Frequency range: 0-250 kHz
− Vibration velocity range: 0.01 - 20000 mm/s
− Target distance: 0.2 - 30 m
− Signal/noise: excellent (depends on target, type of scan and measurement range)
− Sensitivity: 1 - 1000 mm/s/V
• Holographic interferometry (ESPI, DSPI)
59Base excitation of mechanical systems
General case
)(2 tq
Partition of the DOF :
• n1 free displacements q1
• n2 imposed displacements q2
⎭⎬⎫
⎩⎨⎧=
⎭⎬⎫
⎩⎨⎧
⎥⎦
⎤⎢⎣
⎡+⎭⎬⎫
⎩⎨⎧
⎥⎦
⎤⎢⎣
⎡)(22
1
2221
1211
2
1
2221
1211
tr0
KKKK
MMMM
Equations of motion
60
The response takes the form
⎭⎬⎫
⎩⎨⎧
⎥⎦
⎤⎢⎣
⎡ −=
−
2
1121
11
0)(
qy
IKKI
q t
)()()( 212111 tt qMSMg +−=
(equivalent load)
= S (static condensation matrix at foundation level)
)(1111111 tgyKyM =+
Dynamic part of the response solution of
61
System submitted to global support acceleration
)(tϕu
)(2
11
2
1 tϕ⎭⎬⎫
⎩⎨⎧+
⎭⎬⎫
⎩⎨⎧=
⎭⎬⎫
⎩⎨⎧=
uu
0y
q
where ( ) )()( 2121111
2121
111
tt ϕuMuMguKKu
+−=−= −
Method of additional masses
⎭⎬⎫
⎩⎨⎧=
⎭⎬⎫
⎩⎨⎧
⎥⎦
⎤⎢⎣
⎡+⎭⎬⎫
⎩⎨⎧
⎥⎦
⎤⎢⎣
⎡+ )(2
1
2221
1211
2
10222221
1211
tf0
KKKK
MMMMM
Modification of the equations of motion
with M22 of high amplitude level 2022)( qMf ≅t
62
Effective modal masses
Governing motion equation for the unrestrained DOF
)(1111111 tgyKyM =+ )()()( 212111 tt qMSMg +−=
Normal equations
212112 )( qMSMXηηΩ +−=+ T
with
Γ = modal participation matrix of dimension n1 x n2
Concept of effective modal mass : Γ Γ T
( )∑
=
=−1
1
2n
j j
jiST mm
μeΓ
Total mass Mass associated with the support
Effective mass of mode j in direction i
63Digital Signal Processing
Different types of signals
64
Basic Theory of Fourier Analysis
A function x(t), periodic in time T, can be written in an infinite series of sinusoids:
( )( ( ))tnbtnaatx nn
n ωω sincos2
)(1
0 ++= ∑∞
=
( )Tπω 2=with
where ( )
( ) ),2,1(sin)(2
),2,1,0(cos)(2
0
0
==
==
∫
∫ndttntx
Tb
ndttntxT
a
T
n
T
n
ω
ω
Alternative forms
∑∞
−∞=
=n
tnin eXtx ω)( ∫ −=
T tnin dtetx
TX
0)(1 ωwhere
65
The Fourier Transform
A nonperiodic function x(t) which satisfies the condition
( ) ( )( ) ωωωωω dtBtAtx sin)(cos)()( += ∫∞
∞−
where ( )
( ) dtttxB
dtttxA
∫
∫∞
∞−
∞
∞−
=
=
ωπ
ω
ωπ
ω
sin)(1)(
cos)(1)(
Alternative form
ωω ω deXtx ti)()( ∫∞
∞−= ∫
∞
∞−
−= dtetxX ti ω
πω )(
21)(where
∞<∫∞
∞−dttx )(
can be represented by the integral
66
The Discrete Fourier Transform (DFT)
Let us consider a time signal which is digitised (by an A-D converter)
tΔ = time resolution
tf s Δ
= 1= sampling rate
tNT Δ= = sample length
Nf
Tf s==Δ 1
= frequency resolution
The Fourier series of the original signal (periodicity assumption) can be written:
∑∞
−∞=
=n
Ttni
n eXtxπ2
)( ∫−
=T
Ttni
n dtetxT
X0
2
)(1 π
with
1x2x
3x kx
)(tx
Nx
tNT Δ=
tk Δ t
67
If x(t) is discretised at evenly spaced time intervals , we can write at a particular time :tkti Δ=
∫−
=T
Ttni
n dtetxT
X0
2
)(1 π
Nkni
kT
tkniT
tni
k exetkxetxk πππ 222
)()(−Δ−−
=Δ=
In this case, the integral
is replaced by textN
X Nkni
k
N
kn Δ
Δ=
−
=∑
π2
1
1
The (complex) DFT is defined by
),,1(1 2
1
NnexN
X Nkni
k
N
kn ==
−
=∑
π
tΔ
68
The calculation of the DFT of a signal using the definition
requires N 2 complex multiplications (and additions)
time-consuming operation.
The basis of the FFT algorithm of radix 2 (N=2r where r is an integral number) is the partitioning of the full sequence of sample values into a number of shorter sequences:
The Fast Fourier Transform (FFT)
)1,,0(1 21
0
−==−−
=∑ Nnex
NX N
kni
k
N
kn
π
⎟⎟⎠
⎞⎜⎜⎝
⎛+=
+−
+
−
=
−−
=∑∑ N
kni
k
N
k
Nkni
k
N
kn exex
NX
)12(2
12
12
0
22
2
12
0
1 ππ
⎟⎟⎠
⎞⎜⎜⎝
⎛+=
−
+
−
=
−−−
=∑∑ 2
2
12
12
0
22
2
2
12
021
21 N
kni
k
N
k
NniN
kni
k
N
kn exeex
NX
πππ
69
( )
( ) ( ))1
2,,0(
)()(21
2
)()(21)(
−=⎪⎭
⎪⎬
⎫
−=+
+= NnnXWnXNnX
nXWnXnX
zn
y
zn
y
where Ni
eWπ2−
=
Thus the full FFT computation scheme becomes
Example of partitioning : N=8 samples
x0 x1 x2 x3 x4 x5 x6 x7x0 x2 x4 x6 x1 x3 x5 x7x0 x4 x2 x6 x1 x5 x3 x7x0 x4 x2 x6 x1 x5 x3 x7
1x 2x 3x
4x
5x 6x 7x0x
1x 3x2x
4x
6x0x
1x4x
0x
2x
6x
3x
7x
5x7x
5x
70
Random Vibration
Consider a random process represented by an infinite set of samples
∑=∞→
=n
k
k
nx txn
t1
1)(
1 )(1lim)(μ
)()(1lim),( 1)(
11
)(11 ττ +=+ ∑
=∞→txtx
nttR k
n
k
k
nxx
∫−∞→=
2
2
22 )(1limT
TTdttx
TXRoot Mean Square Value
Definitions
Mean Value
Autocorrelation Function
71
Classes of random process
Random Process
Steady-stateNon steady-state
Ergodic(is a type of random process which requires only a single
sample, albeit of considerable length, to portray all the
statistical properties required for its definition)
Non ergodic
)(),()(
11
1
ττμμ
xxxx
xx
RttRt
=+= independent of
t1
72
For an ergodic process, it follows that the Autocorrelation function is defined as the ‘expected’ (or average) value of the product (x(t).x(t+τ))
2)0( XRxx =
( ) ( ) ( )[ ]ττ += txtxERxx .
It can been seen that:
73
Power Spectral Density (PSD)
The Auto- or Power Spectral Density (PSD), Sxx(ω), of a signal x(t)is defined as the Fourier Transform of the Autocorrelation Function i.e.
∫∞
∞−
−= ττπ
ω τω deRS ixxxx )(
21)(
The Auto-Spectral Density is a real and even function of frequency, and does in fact provide a description of the frequency composition of the original signal. For an acceleration signal for example, it has units of (m/s2)2/(rad/s).
The inverse transformation gives:
∫∞
∞−= ωωτ τω deSR i
xxxx )()(
Thus, it comes: 2)()0( XdSR xxxx == ∫∞
∞−ωω
74
A similar concept can be applied to a pair of functions such as x(t)and f(t) to produce cross correlation and cross spectral density functions.
The cross correlation function, Rxf (t) , is defined as:
∫∞
∞−
−= ττπ
ω τω deRS ixfxf )(
21)(
( ) ( ) ( )[ ]ττ += tftxERxf .
and the cross spectral density is defined as its Fourier Transform:
75
Time Domain Autocorrelation function Power Spectral Density
sinus
Narrow bandprocess
Large bandprocess
White noise
76
System Response - Time / Frequency Duality
)()()( ωωω FHX =
∫ −=t
dthftx0
)()()( τττ
)(ωH
TransfertFunction (FRF)
)(th
Impulse Response)(tf
)(ωF
In the frequency domain, we can establish the following relations:
)()()()()()(
)()()( 2
ωωωωωω
ωωω
xfxx
fffx
ffxx
SHSSHS
SHS
=
=
=
Input Output
Property of the cross power spectral densities:
)()( * ωω fxxf SS =
77
Some Features of Digital Fourier Analysis
There are a number of features of digital Fourier analysis which, if not properly treated, can give rise to erroneous results. These are generally the result of the discretisation approximation and of the need to limit the length of the time history.
Specific features are:
• aliasing,
• leakage,
• windowing,
• filtering,
• zooming,
• averaging.
78
Aliasing
Aliasing results from the discretisation of the originally continuous time history.
High-frequency signal: the existence of high frequencies is misinterpreted if the sampling rate is too slow.
Thus, a signal of frequency ω and one of (ω s - ω) (where ω s is the sampling frequency) are indistinguishable when represented as a discretised time history.
Low-frequency signal
79
Alias distortion of spectrum by DFT
(a) True spectrum of signal
(b) Indicated spectrum from DFT: frequencies higher than ωS / 2are “folded back”
Nyquist sampling theorem
2sωω ≤ ==
2maxsωω Nyquist (cut-off) frequency
Practically, one often chooses : ωω 56.2=s
80
Solution : use an anti-aliasing filter which subjects the original time signal to a low-pass, sharp cut-off filter.
True spectrum of signal
Low-pass filter
Indicated spectrum from DFT
Because the filters are not perfect, it is necessary to reject the spectral measurements in a frequency range approaching the Nyquist frequency. It is for this reason that a 1024-point transform results in a 512-line spectrum and that only the first 400 lines are given on the analyser display.
81
Leakage
Leakage results from the need to take only a finite length of time history coupled with the assumption of periodicity.
(a) Ideal signal
(b) ‘Awkward’ signal
(a) The signal is perfectly periodic in the time window T(b) The periodicity assumption is not strictly valid (discontinuity
at the end of the sample)
82
Time domain Frequency domain
83
Windowing
)()()(' twtxtx =Analysed signal Window
)()()(' ωωω WXX ⊗=Convolution product
(a) Boxcar
(b) Hanning
(c) Cosine-taper
(d) Exponential
Different types of window
84
Frequency spectra of different windows
85
Filtering
Filtering is another signal conditioning process rather like windowing, except that it is applied in the frequency domain rather that the time domain.
)()()(' ωωω WXX = )()()(' twtxtx ⊗=
86
Improving Resolution
Inadequate frequency resolution (e.g. especially for lightly-damped systems) arises because of the constraints imposed by the DFT process i.e.
• the limited number of discrete points available (N);
• the maximum frequency range to be covered (ωs/2) and/or the length of time sample available.
Solutions to this problem are:
• Increasing transform size (but it may be counterproductive to increase the fineness of the spectrum overall)
• Zero padding
• Zoom
87
Results of using zero-padding
Zero padding: It consists in adding a series of zeroes to the short sample of actual data, to increase artificially the length of the sample.
(a) DFT of data between 0and T1
(b) DFT of data padded to T2
(c) DFT of full record 0 to T2.
It reveals the presence of 2 frequency components in the signal !
88
A method consists to apply a band-pass filter to the signal and to perform a DFT between 0 and
Zoom
The objective is to obtain a finer frequency resolution by concentrating all the spectral lines (400, 800, …) on the frequency range of interest (between f1 and f2 rather than between 0 and f2).
(a) Spectrum of the signal to be analysed
(b) Band-pass filter
( )12 ωω −
89
Then because of the aliasing phenomenon, the frequency components between f1 and f2 will appear aliased in the analysis range 0 to (f2-f1) with the advantage of a finer resolution.
In this example, the resolution is 4 times finer than in the original baseband analysis.
Effective frequency translation for zoom
90
Other methods to achieve a zoom measurement are based on effectively shifting the frequency origin by multiplying the original time history by a function and then filtering the higher of the two components thus produced.
Example : suppose the signal to be analysed is:
Multiplying this by yields:
If we filter out the second component, we are left with the original signal translated down the frequency range by . In this method, it is clear that sample times are multiplied by the zoom magnification factor.
( )t1cos ω
( )tAtx ωsin)( =( )t1cos ω
( ) ( ) ( ) ( )( )ttAttAtx 111 sinsin2
cossin)(' ωωωωωω ++−==
1ω
91
Averaging
Need to enhance the quality of the measurements in terms of reliability and accuracy. A high number of samples allows to remove spurious random noise from the signals.
There are several options which can be selected when setting an analyser into average mode (exponential, linear).
Different interpretations of multi-sample averaging
(a) Sequential
(b) Overlap
92Use of Different Excitation Signals
Classes of signal used for modal testing
Periodic excitation
• stepped sine
• slow sine sweep
• periodic
• pseudo-random
• periodic random
Transient excitation
• burst sine
• burst random
• chirp
• impulse
Random excitation
• (true) random
• white noise
• narrow-band random
93
Periodic Excitation
• Stepped-sine Testing
Features :
- Step-by-step variation of the frequency of the excitation signal;
- Need to ensure steady-state conditions before the measurements are made;
- The extent of the unwanted transient response will depend on:
the proximity of a natural frequency,
the lightness of the damping,
the abruptness of the changeover.
long measurement time.
Example of rapid coarse sweep with a large frequency increment, followed by a set of small fine sweeps localised around the resonances of interest.
94
• Slow Sine Sweep Testing
(= the traditional method of FRF measurement)
Features :
- Slow and continuous variation of the excitation frequency;
- Slow sweep rate to achieve steady-state conditions;
Prescriptions of the ISO Standard:
- Linear sweep:
- Logarithmic sweep:
Distorting effect of sweep rate
22max 216 rrS ζω< Hz/min
22max 310 rrS ζω< Hz/min
95
• Periodic, Pseudo-Random and Periodic Random Excitation
Features :
- Superposition of sinusoids;
or
- Generation of a random mixture of amplitudes and phases for the various frequency components and repetition of this sequence for several successive cycles.
Optimisation of the energy in the frequency range of interest.
Advantage:
- Exact periodicity of the excitation resulting in zero leakage errors
no need to use a window.
96
Random Excitation
FRF estimates using random excitation
The principle upon which the FRF is determined using random excitation relies on the following relations:
)()()()()()(
)()()( 2
ωωωωωω
ωωω
xfxx
fffx
ffxx
SHSSHS
SHS
=
=
=rather than )()()( ωωω FHX =
where Sxx (ω) , Sff (ω), Sxf (ω) are the autospectra of the response and excitation signals and the cross spectrum between these two signals, respectively.
97
The spectrum analyser has the facility to estimate these various Power Spectral Densities (PSD). Two estimates for the FRF can becomputed using these equations. We shall denote them:
Because we have used different quantities for these two estimates, we must be prepared for the eventuality that they are not identical (as, according to theory, they should be) and to this end we shall introduce the coherence function which is defined by:
)()(
)(1 ωω
ωff
fx
SS
H =)()()(2 ω
ωωxf
xx
SSH =and
)()(
2
12
ωωγ
HH= which can be shown to be always less or equal to 1.
98
Noisy Data
)(txStructure)(tf
Noise Noise
)(tm)(tnMeasured Excitation
)(~ tx)(~ tf
Measured Response
Measured excitation and response signals:
)()()(~ tntftf += )()()(~ tmtxtx +=
Assumption: m(t) and n(t) are not correlated with x(t) and f(t).0)()()( === ωωω xmfnnm SSS
Thus, it follows:
)()()(
)()()(
~~
~~
ωωω
ωωω
mmxxxx
nnffff
SSS
SSS
+=
+=)()(~~ ωω fxxf SS =and
99
)()()(
)(1 ωωω
ωnnff
fx
SSS
H+
=
)()()()(2 ω
ωωωxf
mmxx
SSSH +=
FRF estimates:
is used when noise degrades the response signal (better indicator near antiresonance)
is used when noise degrades the force signal (better indicator near resonance)
General Case: )()()( 21 ωωω HHH ≤≤
ω
)(1 ωH
)(2 ωHAlternative:
)()()( 21 ωωω HHHV =
)(ωH
100
Coherence estimation:
( ) ( )
⎟⎠
⎞⎜⎝
⎛ +⎟⎟⎠
⎞⎜⎜⎝
⎛+
=
++=
)()(1
)()(1
)(
)()()(
)()()(
2
2~~
ωω
ωω
ωγ
ωωω
ωωω
γ
xx
mm
ff
nn
fx
mmxx
xf
nnff
fxxf
SS
SS
SSS
SSS
)()(
2
12
ωωγ
HH=
12~~ ≤xfγ
Cases when
• There may be noise on one or other of the signals;
• The dynamic behaviour of the structure is nonlinear;
• The structure is excited by a non-recorded source of excitation (e.g. lateral coupling between the structure and the shaker).
12~~ ≤xfγ
101
Example of FRF measurement using random excitation
Coherence drop due to noise in the
response signal
Coherence drop due to noise in the excitation signal
102
Example of application
103
Transient Excitation
There are 3 types of transient excitation signals.
• Burst excitation signals
It consists of short sections of an underlying continuous signal(which may be a sine wave, a sine sweep or a random signal) followed by a period of zero input.
The duration of the burst is selected to allow the damping out of the response by the end of the measurement period (to avoid leakage errors).
104
• Rapid sine sweep or ‘chirp’
(short duration signal)
Good control of both the amplitude and the frequency content of the signal.
105
• Impulsive excitation
One practical difficulty encountered when using the hammer excitation is that of the double-hit (rebound).
- Impact from a hammer blow
- Impact controlled by a shaker attached to the structure
106
(a) Excitation pulse clearly satisfies the assumption
(b) The response history also satisfies the assumption
(c) The response history does not satisfy the assumption (for the period T selected)
(d) Exponential window
Periodicity assumption
107
(e) Results processed by exponential window
Impulsive excitation as pseudo-periodic function
108
Types of excitation
No single method is the ‘best’ and it is probably worth making use of several types in order to optimise time, effort and accuracy.
109Modal Identification Methods
1. FRF measurements
(e.g. 800 lines / spectrum)
2. Modal parameter extraction
data reduction
(e.g. 6 modes x 4 values = 24 values/spectrum)
3. Derivation of a mathematical model
(Spatial model, Modal Model)
( )∑= +−
=N
k kkk
krsrs i
AH
122 2
)(ωωζωω
ω
jkα
jkα
110
Classification of modal identification methods
Frequency Domain
(FRF’s)
Time Domain
(IRF’s or response histories)
SDOF methods MDOF methods
Single-FRF methods Multi-FRF methods
• modelling of damping effects,
• model order.
Difficulties :
111
SDOF Modal Identification Methods
SDOF means that just one resonance is considered at a time
Assumption: the modes must appear clearly separated so that theycan be analysed sequentially, one after the other.
( )( )krs
kkk
krsrs B
i
AH +
+−≅
ωωζωωω
2)( 22
( ) ( ) ( )∑∑≠== +−
++−
=+−
=N
kjj jjj
jrs
kkk
krsN
k kkk
krsrs i
A
i
A
i
AH
12222
122 222
)(ωωζωωωωζωωωωζωω
ω
!
rsH
( )333 ,, rsAζω
( )222 ,, rsAζω
( )111 ,, rsAζω
12
3
rsH
rsH
112
a) Peak-Amplitude Method (Peak-Picking)
Estimation of the damping ratio using the quality factor:
kba
kQζωω
ω2
1=−
=
rsH
rsH
kω aω bω
Half-Power points
2rsα
kω
113
b) Circle-Fit Method
Circle-fitting FRF plot in the vicinity of resonance
( ))2/tan()2/tan(2
22
bak
bak θθω
ωωζ+
−=
rωaω
bω
Effect of residual terms
aω
bω
bθaθ
rζ
detection of nonlinear behaviour
114
Concept of residual terms
To take into account the influence of modes which exist outside the frequency range of measurement and/or analysis, any FRF coefficient may be rewritten as:
rrr
jkrN
mr
m
mr
m
r
N
r rrr
jkrjk
iA
iA
ωωζωω
ωωζωωωα
2
2)(
221
1
1
122
2
2
1
1
+−⎟⎟⎠
⎞⎜⎜⎝
⎛++=
+−=
∑∑∑
∑
+==
−
=
=
High-frequency modes
Low-frequency modesModes actually identified
115
Contributions of low-, medium- and high frequency modes
( )Rrs
m
mk kkk
krsRrs
rs Ki
A
MH 1
21)(
2
1
222 ++−
+−= ∑= ωωζωωω
ω
Residual mass Residual stiffness
rsH
Rec
epta
nce
(log-
log
scal
e)
rsH
rsH
116
Examples of regenerated FRF’s
without residuals
with residuals
117
MDOF Modal Identification Methods
a) Least Squares Complex Exponential (LSCE)
Features:
• Time-domain technique
• Global estimation of natural frequency and damping of several modes simultaneously
Theoretical basis:
The general expression used for the FRF of a damped system in terms of modal parameters is:
( ) ( ) ( ) ( )
( ) ( )
)()(
)()()(
*
*
1
**
**
1
k
krsN
k k
krs
kk
kskrN
k kk
kskrrs
iA
iA
izz
izz
H
λωλω
λωρλωρω
−+
−=
−+
−=
∑
∑
=
=
118
Taking the inverse Fourier Transform, the expression for an Impulse Response Function (IRF) in terms of modal parameters writes:
( ) ( ) ( ) ⎟⎠
⎞⎜⎝
⎛=+= ∑∑==
N
k
tkrs
tkrs
N
k
tkrsrs
kkk eAeAeAth1
*
1Re2)(
* λλλ
Time sampling: tjt Δ=
( ) ⎟⎠
⎞⎜⎝
⎛=Δ ∑=
N
k
jkkrsrs ZAtjh
1Re2)(
tk
keZ Δ= λ defines the natural frequency and damping ratio of mode k (= global estimate)
( )krsA defines the displacement of point r in mode k (= local estimate)
119
The unknowns Zk may be considered as the roots of a polynomial of order 2N:
( ) ∑∏=
≠−=
=−=N
p
pp
N
kNk
k ZZZZP2
00
)( α
where the coefficients αp have to be estimated using data measured on the system.
( ) ⎟⎠
⎞⎜⎝
⎛=Δ ∑=
N
k
jkkrsrs ZAtjh
1Re2)(
For this purpose, let us consider the expression of the IRF
120
The IRF at a series of 2N equally spaced time intervals is:
( )
( )
( ) ⎟⎠
⎞⎜⎝
⎛=Δ×
⎟⎠
⎞⎜⎝
⎛=Δ×
⎟⎠
⎞⎜⎝
⎛=×
∑
∑
∑
=
=
=
N
k
NkkrsrsN
N
k
pkkrsrsp
N
kkkrsrs
ZAtNh
ZAtph
ZAh
1
22
1
1
00
Re2)2(
Re2)(
Re2)0(
α
α
α
( ) ⎟⎟⎠
⎞⎜⎜⎝
⎛=Δ ∑ ∑∑
= ==
N
k
pk
N
ppkrsrs
N
pp ZAtph
1
2
0
2
0Re2)( αα
= 0 from the definition
0)(2
0=Δ∑
=
tphrs
N
ppα
121
)2()(12
0tNhtph rsrs
N
pp Δ−=Δ∑
−
=
α
It follows that:
To estimate the coefficients αp in a least squares sense, let express this equation:
( )( ) ( )( )tNhtph rsrs
N
pp Δ+−=Δ+∑
−
=
212
0α
• for all possible time points:
• for all possible measured responses:
• for all possible excitation points: ),,1(),,1(
),,1,0()2(
i
o
t
nsnr
ntN
……
…
==
=Δ+
122
Thus the matrix:
( ) ( ) ( )( )( ) ( ) ( )
( ) ( )( ) ( )( )
( ) ( )( ) ( )( )
( ) ( )( ) ( )( )⎥⎥⎥⎥⎥⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢⎢⎢⎢⎢⎢
⎣
⎡
Δ−+Δ+Δ
Δ+−Δ+Δ
Δ−+Δ+Δ
ΔΔΔΔ−Δ
tNnhtnhtnh
tNhthth
tNnhtnhtnh
tNhththtNhthh
tnntnntnn
rsrsrs
ttt
ioioio121
121
121
22120
111111
111111
111111
=
⎪⎪⎭
⎪⎪⎬
⎫
⎪⎪⎩
⎪⎪⎨
⎧
−12
1
0
Nα
αα ( )
( )( )
( )( )
( )( )
( )( )⎪⎪⎪⎪⎪
⎭
⎪⎪⎪⎪⎪
⎬
⎫
⎪⎪⎪⎪⎪
⎩
⎪⎪⎪⎪⎪
⎨
⎧
Δ+−
Δ+−
Δ+−
Δ+−Δ−
tnNh
tNh
tnNh
tNhtNh
tnn
rs
t
io2
2
2
122
11
11
11
Overdetermined system: A x = b
which has the solution: ( ) bAAAx TT 1−=
123
The solution:
allows to reconstruct the polynomial:
and the roots:
gives the complex eigenvalues:
If the eigenvalues may be further expressed as follows:
we obtain the values of the natural frequency ωk and the damping
ratio ζk (in the assumption of proportional damping).
1210 −= NT αααx
∑=
=N
p
pp ZZP
2
0
)( αt
kkeZ Δ= λ
),,2,1( Nkk …=λ
( )21 kkkk i ζζωλ −+−=
124
Selection of the model order
By using a different number of poles (2N) and comparing the error between the regenerated FRF’s and the original measured data, it is possible to draw a so-called ‘stabilisation diagram’:
As the number of poles increases, a number of computational modes are created in addition to the genuine physical modes which are of interest.
125
b) Least Squares Frequency Domain (LSFD)
Features:
• Frequency domain technique
• Global estimation of residues (--> complex modes)
Theoretical basis:
FRF of a damped system in the frequency band [ωmin, ωmax]:
( ) ( )Rrsk
krsm
mk k
krsRrs
rs KiA
iA
MH 1
)()(1)( *
*
2
2
1
+⎟⎟⎠
⎞⎜⎜⎝
⎛
−+
−+−= ∑
= λωλωωω
126
( ) ( )
⎪⎭
⎪⎬⎫∗
Rrs
Rrs
krskrs
MK
AA
,
, are local estimates (which depend on the locations of the measurement point (r) and of the excitation point (s)
Receptance diagram (log-log scale) rsH R
rsK1
RrsM2
1ω
Lower residual
Upper residual
( ) ( )Rrsk
krsm
mk k
krsRrs
rs KiA
iA
MH 1
)()(1)( *
*
2
2
1
+⎟⎟⎠
⎞⎜⎜⎝
⎛
−+
−+−= ∑
= λωλωωω
127
Calculation of the residues and( )krsA ( )∗
krsAAssumption: the poles λk have been identified (LSCE method).
( ) ( ) ( )
( ) ( ) ( )⎪⎩
⎪⎨⎧
−=
+=∗
krskrskrs
krskrskrs
ViUA
ViUAWriting:
the FRF takes the form:
( ) ( ) Rrs
kkrs
m
mkkkrsR
rsrs K
QVPUM
H 1)()(1)(2
1
2 +⎟⎟⎠
⎞⎜⎜⎝
⎛++−= ∑
=
ωωω
ω
(2 m+2) unknowns with m = m2 - m1
We define the error as: ( ) 2)(
max
min
ωωω
ωω
EXPrsrs HHE −= ∑
=
Theoretical value Measured data
128
The error is minimised by differentiating its expression with respect to each unknowns in turn,
( ) ( )
0;0
),,(;0;0 21
=∂∂=
∂∂
==∂
∂=∂
∂
rsrs
krskrs
ME
KE
mmkV
EU
E …
thus generating a set of (2 m+2) equations with (2 m+2) unknowns (m = m2-m1).
129
Extraction of the (complex) eigenmodes.
For each identified pole k (k = 1,.., m) , we have:
( ) ( ) ( )
( ) ( ) ( )
( ) ( ) ( ) ( )
( ) ( )ksrnksn
kskskskss
kskks
kskksk
zzA
zzzA
zzAzzA
oo==
===
=
=
2
22
11,λ
( ) ( )kssks Az =
and thus:
( )( )
( )),,,1( srnr
zA
z oks
krskr ≠== …
A transducer should not be located where zs(k) = 0 (on a vibration node)
130
( )
⎥⎥⎥⎥⎥⎥
⎦
⎤
⎢⎢⎢⎢⎢⎢
⎣
⎡
=
iooo
i
i
nnsnn
rn
n
rs
s
r
HHH
H
H
H
H
H
H
1
11
1
11
ωH « roving hammer »
In practice:
131
Frequency band Partial fitting
As modes 1, 2, 3 have been identified (poles and residues), their participation in the frequency range [ωmin, ωmax] can be subtracted mathematically before identifying modes 4, 5 et 6.
FRF data associated with a bad coherence are not considered for identification
Used data
Rejected data
Remarks
rsH rsH
132
c) Ibrahim Time Domain Method (ITD, 1973-77)
Features :
• Time-domain method
• Global estimation of poles and residues
Theoretical basis:
The free response of a viscously-damped system is given by:
∑=
=n
k
tk
ket2
1)()( λzqFree response
vector
complex eigenvector z (k)(unscaled mode)
Number of modes in the response
133
Considering 2n time instants, the free response matrix is given by:
( ) ( )[ ] ( ) ( )
1 1 1 2
2 1 2 2
1 2 1 2
n
n n n
t t
n nt t
e et t
e e
λ λ
λ λ
⎡ ⎤⎢ ⎥
⎡ ⎤= ⎢ ⎥⎣ ⎦⎢ ⎥⎢ ⎥⎣ ⎦
q q z z… …
2n n×Q
2n n×Z
2 2n n×Λ=
134
( ) ( )[ ] ( ) ( )
1 1 1 2
2 1 2 2
1 2 1 2
n
n n n
t t
n nt t
e eˆ ˆt t t t
e e
λ λ
λ λ
⎡ ⎤⎢ ⎥
⎡ ⎤+ Δ + Δ = ⎢ ⎥⎣ ⎦⎢ ⎥⎢ ⎥⎣ ⎦
q q z z… …
Considering a second set of samples shifted by an interval of time Δtwith respect to the first set:
( ) ( )( )
( )2n 2nt t ttk j k jk
j k kk 1 k 1
t t e e eλ λλ+Δ Δ
= =+ Δ = =∑ ∑q z z
tΔQ Z Λ
tˆ
Δ =Q Z Λ
135
( ) ( )[ ] ( ) ( )
1 1 1 2
2 1 2 2
1 2 1 22 2
n
n n n
t t
n nt t
e eˆ ˆˆ ˆt t t t
e e
λ λ
λ λ
⎡ ⎤⎢ ⎥
⎡ ⎤+ Δ + Δ = ⎢ ⎥⎣ ⎦⎢ ⎥⎢ ⎥⎣ ⎦
q q z z… …
In the same way, for a time shift of 2 Δt
with ( ) ( )2 i t
i iˆ e λ Δ=z z
2 tˆ
Δ =Q Z Λ
136
Thus, we have:
2
ou
ou
t
t
t
ˆ
ˆˆˆ
ˆ
Δ
Δ
Δ
⎡ ⎤ ⎡ ⎤= =⎢ ⎥ ⎢ ⎥⎣ ⎦⎣ ⎦⎡ ⎤⎡ ⎤
= =⎢ ⎥⎢ ⎥⎢ ⎥⎣ ⎦ ⎣ ⎦
Q ZΛ Φ A Λ
Q Z
ZQΛ Φ A ΛQ Z
and
Eliminating Λ gives:
1i i
ˆ ˆ− =ΦΦ a a
1 ˆˆ − =ΦΦ A A
If we define:
We have:1 i t
i iˆ eλ Δ− =ΦΦ a a
Eigenvalue problem
The eigenvectors ai have their first n co-ordinates equal to the eigenmodes of the structure and λi are the complex eigenvalues.
or
or
[ ] [ ]nn aaAaaA ˆˆˆ11 …… == and
137
( ) 1i tT T
i iˆ eλ− Δ⎡ ⎤ =⎣ ⎦Φ Φ Φ Φ a a
If the number of time samples is greater than the number of modes excited, then matrices Φ are rectangular and the eigenvalue problem is transformed into:
138
Since the order of matrix may exceed the number of modes excited, it remains to separate the structural modes from the numerical modes.
For this purpose, let us write the response of the real stationsdelayed by a time-interval Δτ : i.e.
Modal Confidence Factor
( ) 1T Tˆ −⎡ ⎤⎣ ⎦Φ Φ Φ Φ
( ) ( )( )
( ) ( )2 2 2
1 1 1
k k k kn n n
t t tk k k
k k k' t e e e ' eλ τ λ τ λ λ+Δ Δ
= = == = =∑ ∑ ∑q z z z
( ) ( )t ' tτ+ Δ =q q
If zi(k) is the i th deflection of the k th mode at the real station, then the value at the assumed station delayed by Δτ is expected to be:
( ) ( )τλ Δ= kekiki zz expected,
139
The Modal Confidence Factor (MCF) is defined as:
and should be near 1.( )
( )ki
ki
',
zz expectedMCF =
140
d) Stochastic Subspace Identification Method
Features:
• Time-domain method
• Global estimation of poles and residues
Theoretical background: Stochastic model in the state-space.
Given a n-dimensional time series q[k] = q(tk), the dynamic behavior of the system may be described by the state space model
[ ] [ ] [ ][ ] [ ] [ ]1k k kk k k
+r = A r + wq = B x + v
State matrix
Output matrix
State vector
Process noise
Assumption: w and v are zero-mean Gaussian white noise.
Measurement noise
141
The covariance matrices of w and v are:
[ ][ ] [ ] [ ]( ) ( )T Tk
E k t k t tk
δ⎡ ⎤⎛ ⎞ ⎛ ⎞+ + =⎢ ⎥⎜ ⎟ ⎜ ⎟
⎝ ⎠⎝ ⎠⎣ ⎦
w Q Sw v
v S R
The output covariance matrices are defined as
Expectation
[ ] [ ]
[ ] [ ]
0T
Ti
E k k
E k i k
⎡ ⎤= ⎣ ⎦⎡ ⎤= +⎣ ⎦
Λ q q
Λ q q
Covariance matrices
142
As w[k] and v[k] are independent of the state vector r[k], the following properties can be established:
[ ] [ ]
[ ] [ ]
0
0
0 01
1
T T
T T
T
ii
E k k
E k k
−
⎡ ⎤ = +⎣ ⎦⎡ ⎤+ = = +⎣ ⎦
= +
=
r r A Σ A Q
r r G A Σ B S
Λ B Σ B R
Λ B A G
where Σ0 is the state covariance matrix and G is referred as the next state-output covariance matrix.
143
Covariance-Driven Stochastic Subspace Method
Let us construct the Hankel matrix with p block rows and q block columns of the output covariance matrix Λi
1 2
2 3 1
1 1
q
qp,q
p p p q
+
+ + +
⎡ ⎤⎢ ⎥⎢ ⎥= ⎢ ⎥⎢ ⎥⎢ ⎥⎣ ⎦
Λ Λ Λ
Λ Λ ΛH
Λ Λ Λ
( )q p≥
The pth-order observability and controllability matrices are respectively:
1
1
Tpp
−
−
⎡ ⎤= ⎣ ⎦⎡ ⎤= ⎣ ⎦
O B B A B A
C G A G A G
144
p,q p q=H O C
1ii
−=Λ B A GThe previous relationship
leads to the following factorisation property
Let W1 and W2 be two user-defined invertible weighting matrices
of dimension p x m and q x m respectively. Performing the following singular value decomposition gives:
[ ] [ ]1 , 2 1 2 1 2 11
1 10
0 0T T
p q⎡ ⎤= =⎢ ⎥⎣ ⎦
W H W U U U SS
V V V
S1 contains 2 Nm non-zero singular values where Nm is the number of system modes.
145
It follows that the observability and controllability matrices can be recovered as
1 21 1
1 211
p
Tq
=
=
O U S
C S V
Let us write
2 11
Tpp p↑ −
−⎡ ⎤= =⎣ ⎦O B A B A B A O A
may be determined by making use of Op matrix
Matrices A and B then the eigenvalues and eigenvectors of the system may be easily computed.
146
Comparison and Correlation Techniques
• Visual inspection experimental / calculated mode-shapes.
• Visual inspection of regenerated / predicted FRFs.
• Use of mathematical tools.
Let us note:
xX an experimental (complex) eigenvector;
xA an analytical eigenvector (predicted by a model);
147Modal Scale Factor (MSF)
TX ATA A
MSF = x xx x
orTX ATX X
MSF = x xx x
depending upon which mode-shape is taken as the reference one.
148
Graphical representations
Modal Assurance Criterion (MAC)
( )10 ≤≤ MAC)()(
2
ATAX
TX
ATX
MACxxxx
xx=
149
Causes of bad correlation:
• presence of non-linearities, noisy data
• bad modal identification
• inappropriate choice of measurement coordinates
• modelling uncertainties (physical parameters, geometry)
• modelling errors (FEM)