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Title: CIDER


1
CIDER08-Seismology Lectures
  • Lecture 1 Equations and Waves (BR)
  • Lecture 2 Numerical Simulations (JT)
  • Lecture 3 Surface waves (GM)
  • Lecture 4 Geophysical Inverse Problem (GM)
  • Lecture 5 Receiver Functions (AL)
  • Lecture 6 Array Techniques (AL)

2
Equations and Waves
  • Barbara Romanowicz
  • U.C. Berkeley
  • KITP

CIDER Summer08
3
Seismology and the earths interior
  • Snapshot of present structure of the earth
  • Defined the 1D layering of the earth
  • 3D variations of seismic parameters as proxies
    for lateral variations of temperature and
    composition
  • Isotropic velocities
  • Anisotropy
  • Anelastic attenuation

4
x (Vsh/Vsv)2
Montagner, 2002
5
Motivation for seismic Q tomography
Faul and Jackson, 2005
6
From Stein and Wysession, 2003
7
From Stein and Wysession, 2003
8
Rayleigh
SS
P
S
9
Seismic wave equation
  • We apply F ma
  • Stresses
  • Force on plane normal to x1
  • -Total force due to stresses

10
Seismic wave equation
  • We apply F ma
  • Stresses
  • Force on plane normal to x1
  • -Total force due to stresses

11
Body forces F(2)
Mass is
ma F is then
i1,2,3
In general, body forces include source term and
gravity term
12
Body forces F(2)
Mass is
ma F is then
i1,2,3
In general, body forces include source term and
gravity term
13
Body forces F(2)
Mass is
ma F is then
i1,2,3
In general, body forces include source term and
gravity term
14
Elasticity Linear stress-strain relationship
  • cijkl is the elastic tensor
  • 21 independent elements (symmetries)
  • Isotropic material properties are the same in
    all directions
  • there are only 2 independent elements, l and m
    (Lamé Parameters)

Hookes law Strains lt10-4
15
Elasticity Linear stress-strain relationship
  • cijkl is the elastic tensor
  • 21 independent elements (symmetries)
  • Isotropic material properties are the same in
    all directions
  • there are only 2 independent elements, l and m
    (Lamé Parameters)

Hookes law Strains lt10-4
16
Isotropic medium
Described by distribution of (r, l, m) or (r,
k, m) or (r ,a ,b)
Shear modulus m
Bulk modulus
P velocity
S velocity
l, m, k have units of stress
17
Isotropic medium
Described by distribution of (r, l, m) or (r,
k, m) or (r ,a ,b)
Shear modulus m
Bulk modulus
P velocity
S velocity
Bulk sound velocity
18
Isotropic medium
Described by distribution of (r, l, m) or (r,
k, m) or (r ,a ,b)
Shear modulus m
Bulk modulus
P velocity
S velocity
Bulk sound velocity
19
Isotropic medium
Described by distribution of (r, l, m) or (r,
k, m) or (r ,a ,b)
Shear modulus m
Bulk modulus
P velocity
S velocity
Bulk sound velocity
20
Homogeneous wave equation for Isotropic medium
(no body forces)
Substituting expression of stress as a function
of Lame parameters
Gradients of structure, non zero for
inhomogeneous medium
?If structure depends only on radius Consider
a stack of homogeneous layers linked through
reflection/transmission coefficients
homogeneous layer methods ?gradient terms vary
as 1/ ?, where ? is angular frequency -gt neglect
them at high frequency ray methods ,
infinite frequency approximation (f gt1 hz)
21
Homogeneous wave equation for Isotropic medium
(no body forces)
Substituting expression of stress as a function
of Lame parameters
Gradients of structure, non zero for
inhomogeneous medium
?If structure depends only on radius Consider
a stack of homogeneous layers linked through
reflection/transmission coefficients
homogeneous layer methods ?gradient terms vary
as 1/ ?, where ? is angular frequency -gt neglect
them at high frequency ray methods ,
infinite frequency approximation (f gt1 hz)
22
Homogeneous wave equation for Isotropic medium
(no body forces)
Substituting expression of stress as a function
of Lame parameters
Gradients of structure, non zero for
inhomogeneous medium
?If structure depends only on radius Consider
a stack of homogeneous layers linked through
reflection/transmission coefficients
homogeneous layer methods ?gradient terms vary
as 1/ ?, where ? is angular frequency -gt neglect
them at high frequency ray methods ,
infinite frequency approximation (f gt1 hz)
23
Homogeneous wave equation for Isotropic medium
(no body forces)
Substituting expression of stress as a function
of Lame parameters
Gradients of structure, non zero for
inhomogeneous medium
?If structure depends only on radius Consider
a stack of homogeneous layers linked through
reflection/transmission coefficients
homogeneous layer methods ?gradient terms vary
as 1/ ?, where ? is angular frequency -gt neglect
them at high frequency ray methods ,
infinite frequency approximation (f gt1 hz)
24
  • In a homogeneous medium (or high frequency
    approximation)
  • Taking divergence and curl, the equation of
    motion separates in two parts

S waves
a2
P waves
Note
25
  • In a homogeneous medium(or high frequency
    approximation)
  • Taking divergence and curl, the equation of
    motion separates in two parts

S waves
a2
P waves
Note
26
  • In a homogeneous medium(or high frequency
    approximation)
  • Taking divergence and curl, the equation of
    motion separates in two parts

S waves
a2
P waves
Note
27
Solutions are waves u(x,t) f(xvt) where v
velocity In Cartesian coordinates, plane
waves
k is the wave number
(Figures from Stein and Wysession, 2003)
In spherical coordinates
Amplitudes decay as 1/r geometrical spreading
28
Solutions are waves u(x,t) f(xvt) where v
velocity In Cartesian coordinates, plane
waves
k is the wave number
(Figures from Stein and Wysession, 2003)
In spherical coordinates
Amplitudes decay as 1/r geometrical spreading
29
Solutions are waves u(x,t) f(xvt) where v
velocity In Cartesian coordinates, plane
waves
k is the wave number
(Figures from Stein and Wysession, 2003)
In Spherical coordinates
Amplitudes decay as 1/r geometrical spreading
30
Polarisation of P and S waves
31
From Stein and Wysession, 2003
32
Example Particle motion plots for SKSSKKS and
Sdiff
From Stein and Wysession, 2003
33
Ray theory
  • Simple and fast
  • Used extensively in earthquake location, focal
    mechanisms, inversion for structure in crust and
    mantle
  • Shortcomings
  • High frequency approximation fails at long
    periods
  • Does not predict non geometrical effects i.e.
    diffracted waves, head waves
  • Limitations in predicting effects of
    heterogeneity on waveforms

34
?x
p ray parameter apparent horizontal slowness
35
Snells law
At the interface between two media
v1 lt v2
Ray angle at the interface must change to
preserve the timing of the wavefronts across the
interface
p sin ?1/v1 sin ?2/ v2
?Ray parameter is a constant of the ray
?Ray bottoms for a critical incidence angle
no transmitted wave for larger incidence angles
(post-critical or total reflection)
36
In general, some of the energy is transmitted,
some reflected, and, in the P-SV case, some
converted
SH case
P-SV case
Angles of reflection/transmission depend only on
velocities Amplitudes depend on impedance (? v)
37
Ray paths in spherical geometry, when velocity
increases with depth
38
Steep gradients, such as upper-mantle
discontinuities, create triplications
39
Low velocity layers create shadow zones
40
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41
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42
Van der Hilst et al., 1998
P wave tomography
43
P travel time (tranmission) tomography
Courtesy of D. Vasco
44
Travel time kernels
D 60o T 20 s
P waves
S waves
Montelli et al., 2006
45
Montelli et al., 2004
46
Karason and van der Hilst, 2000
47
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48
Astiz, Earle and Shearer, 1996
49
Predictions from IASP91 model
Shearer, 1996
50
Shallow earthquake
From Stein and Wysession, 2003
51
Surface waves
  • Arise from interaction of body waves with free
    surface.
  • Energy confined near the surface
  • Rayleigh waves interference between P and SV
    waves exist because of free surface
  • Love waves interference of multiple S
    reflections. Require increase of velocity with
    depth
  • Surface waves are dispersive velocity depends on
    frequency (group and phase velocity)
  • Most of the long period energy (gt30 s) radiated
    from earthquakes propagates as surface waves

52
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53
After Park et al, 2005
54
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55
Sumatra 12/26/04
(0.8 to 2.2 mHz)
CAN
1S5
3S2
1S4
UNM
0S9
0S12
0S8
0S7
0S10
0S11
0S0
0S5
1S3 /3S1
0S6
Frequency
Fourier spectrum200 hours starting 10 hours
before origin time
56
Free oscillations
57
The kth free oscillation
satisfies
SNREI model Solutions of the form
k (l,m,n)
58
The kth free oscillation
satisfies
SNREI model Solutions of the form
k (l,m,n)
59
Free Oscillations (standing waves)
gt Frequency domain
The kth free oscillation
satisfies
SNREI model Solutions of the form
k (l,m,n)
60
Free Oscillations (standing waves)
The kth free oscillation
satisfies
SNREI model Solutions of the form
k (l,m,n)
61
Free Oscillations (standing waves)
The kth free oscillation
satisfies
SNREI model Solutions of the form
k (l,m,n)
62
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63
oS2
oSo
oS3
After Park et al, 2005
(53.9 min) (25.7 min) (20.5
min)
64
Seismograms by mode summation
? Mode Completeness
? Orthonormality (L is an adjoint operator)
65
Seismograms by mode summation
? Mode Completeness
? Orthonormality (L is an adjoint operator)
66
Seismograms by mode summation
? Mode Completeness
? Orthonormality (L is an adjoint operator)
67
The solution for the displacement then has the
form
Where Fk is the distribution of body forces, and
H(t) is the Heaviside function, and we
assume that the motion is zero before t0.
In terms of moment tensor
Where M is moment Tensor, e strain tensor At the
source
68
The solution for the displacement then has the
form
Where Fk is the distribution of body forces, and
H(t) is the Heaviside function, and we
assume that the motion is zero before t0.
In terms of moment tensor
Where M is moment Tensor, e strain tensor At the
source
69
The solution for the displacement then has the
form
r0source location
Where Fk is the distribution of body forces, and
H(t) is the Heaviside function, and we
assume that the motion is zero before t0.
In terms of moment tensor
Where M is Moment Rate Tensor, e strain
tensor eval. at the source
70
Spheroidal modes Vertical Radial component
Toroidal modes Transverse component
n0
n1
n T l
l angular order, horizontal nodal planes n
overtone number, vertical nodes
71
Normal mode summation 1D
  • A excitation
  • w eigen-frequency
  • Q Quality factor ( attenuation )

72
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73
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74
From ray theory to finite frequency effects
  • Goal is to use as much information as
  • possible from seismograms

75
Standard tomographic ingredients
  • Body waves
  • Travel times of well separated phases
  • Ray theory
  • Surface waves
  • Group/phase velocities or waveforms
  • Path average approximation (PAVA)

76
  • c is the phase velocity velocity at which the
    peaks and troughs travel
  • Energy travels with group velocity (along the
    actual ray paths)

77
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78
Towards Waveform Tomography
observed
synthetic
79
SS
Sdiff
PAVA
NACT
Ray theory versus two approximations to first
order perturbation theory In the 2D vertical
plane
Li and Romanowicz, 1995
80
Yoshizawa and Kennett, 2004
Looking from the top (horizontal plane)
81
After Montelli et al., 2006
82
Fundamental Mode Surface waves
Body waves
Overtone surface waves
Ritsema et al., 2004
83
Towards Waveform Tomography
observed
synthetic
84
Preliminary Level 4 radially anisotropic model
courtesy of Ved Lekic
85
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86
Seismic Wave attenuation
  • Amplitudes of seismic waves are affected by
  • Geometrical spreading
  • Scattering/focusing (total energy in the
    wavefield conserved)
  • Intrinsic attenuation (energy loss due to
    friction on anelastic processes).

87
Intrinsic attenuation is described by the
quality factor Q
E peak strain energy ?E energy loss, per cycle
In ray theory
hence
88
Intrinsic attenuation is described by the
quality factor Q
E peak strain energy ?E energy loss per cycle
In ray theory
hence
89
Intrinsic attenuation is described by the
quality factor Q
E peak strain energy ?E energy loss per cycle
In ray theory
hence
90
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91
Examples of focusing
92
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93
  • Dispersion due to attenuation
  • Causality
  • Physical mechanisms for attenuation
  • In a frequency band where Q is constant

94
Romanowicz and Gung, 2002
95
Anisotropy
  • In general elastic properties of a material vary
    with orientation
  • Anisotropy causes wave splitting

From E. Garneros website
96
SKS Splitting Observations
Interpreted in terms of a model of a layer of
anisotropy with a horizontal symmetry axis
Dt time shift between fast and slow
waves Yo Direction of fast velocity
axis
Montagner et al. (2000) show how to relate
surface wave anisotropy and shear wave splitting
Huang et al., 2000
97
Types of anisotropy
  • General anisotropic model 21 independent
    elements of the elastic tensor cijkl
  • Long period waveforms sensitive to a subset, to
    first order (13) of which only a small number can
    be resolved
  • Radial anisotropy
  • Azimuthal anisotropy

98
Radial Anisotropy
  • Love/Rayleigh wave discrepancy
  • Vertical axis of symmetry
  • A,C,F,L,N (Love, 1911)
  • Long period S waveforms can only resolve
  • L r Vsv2
  • N r Vsh2
  • gt x (Vsh/Vsv) 2
  • dln x 2(dln Vsh dlnVsv)

99
Azimuthal anisotropy
  • Horizontal axis of symmetry
  • Described in terms of y, azimuth with respect to
    the symmetry axis in the horizontal plane
  • 6 Terms in 2y (B,G,H) and 2 terms in 4y (E)
  • Cos 2y -gt Bc,Gc, Hc
  • Sin 2y -gt Bs,Gs, Hs
  • Cos 4y-gt Ec
  • Sin 4y -gt Es
  • long period waveforms can resolve Gc and Gs

100
  • Vectorial tomography
  • Combination radial/azimuthal (Montagner and
    Nataf, 1986)
  • Radial anisotropy with arbitrary axis orientation
    (cf olivine crystals oriented in flow)
    orthotropic medium
  • L,N, Y, Q

101
  • Azimuthal anisotropy

102
Study of Structure near the CMB
From Ed Garneros website
103
Sharp boundary of the African Superplume
Ni et al., 2002
104
Indian Ocean Paths - Sdiffracted
Toh et al.,2005
2sec, 5sec, 18 sec (corner
frequencies)
105
Toh et al., EPSL, 2005
106
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