jgrb17183-sup-0002-txts01

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Text S1
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Hu et al. (2009a, b) derived two fundamental elastic formulas to study the
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preseismic and coseismic stress fields based on the principle of virtual work. On the
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basis of the elastic formulas, we propose a quasi-static model of fault earthquake
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defined by domain V with boundary surface S (Figure 1). The domain consists of
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three regions: (1) the upper crust region, VI , excluding earthquake fault zones, which
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is isotropic elastic; (2) the earthquake fault zone, VII , in the upper crust, which is
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transversely elastic; (3) and the lower crust and upper mantle, VIII , which is
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viscoelastic according to the Maxwell model. The boundary surface is divided into
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two sub-boundaries, S1 and S 2 , on which the known displacement vector and
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traction qt are prescribed, respectively.
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Figure 1 The sketch map of the finite element model.
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The constitutive relationship of the material in VI is:
σ t  D Iε t ,
(1)
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where superscript t of σ and ε denote time, σ  [ xx  yy  zz  yz  xz  xy ]T and
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ε  [ xx  yy  zz  yz  xz  xy ]T are the stress and strain at time t, respectively,
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ux , u y and uz are displacement components in the directions of x, y and z, DI is the
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elastic material matrixes,


1  
 
1 



1 
 
E
DI 

(1   )(1  2 ) 

0


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ux 
 
u y  ,
u 
 z








0.5   
0
0.5  
0.5  
The constitutive relationship of the material in VII (Cai and Yin, 1997) in the
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
y 


x 


0

T


 x 0 0 0 z




ε t  Lut  0
0
0
y
z





0 0 z y x

material axis system ( x, y , z ) is:
σ  DII ε ,
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(2)
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where ε  [ xx  yy  zz  yz  xz  xy ]T , σ  [ xx  yy  zz  yz  xz  xy ]T are the strain
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and stress, respectively.
 a (1  a 22 )b a 2 (1   1 )b a ( 1  a 22 )b 0

(1   12 )b
a 2 (1   1 )b 0


a (1  a 22 )b 0
DII  
G2


sym.


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0
0
0
G1
0

0
0
.
0
0

G2 
E1
E2
,b 
, E1 , E2 ,1 , 2 , G2 are five independent parameters, and
E2
(1  1 )(1  1  2 22 a)
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a
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G1 
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0
E1
E2
, G2 
.
2(1  1 )
2(1  2 )
Equation (2) can be transferred into the global coordinate system (x, y, z):
σ t  D IIε t
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where DII  N T DII N and ε  Nε t , N is the transformation matrix between the
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material coordinate system ( x, y , z ) and global coordinate system (x, y, z) ,
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 l12
 2
 l2
 l2
N 3
 2l2l3
 2l l
 31
 2l1l2
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m12
n12
m1n1
l1n1
2
2
2
3
2
2
2
3


l2 m2 
l3m3 
,
l2 m3  l3m2 
l3m1  l1m3 

l1m2  l2 m1 
l1m1
m
n
m2 n2
l2 n2
m
n
m3n3
l3n3
2m2 m3
2n2 n3
m2 n3  m3n2
l2 n3  l3n2
2m3m1
2n3n1
m3n1  m1n3
l3n1  l1n3
2m1m2
2n1n2
m1n2  m2 n1
l1n2  l2 n1
l, m, n are directional cosines between the two coordinate systems (Table 1).
Table 1 Directional cosine between the two coordinate systems.
Axis
x
y
z
x
l1
m1
n1
y
l2
m2
n2
z
l3
m3
n3
The material in the earthquake fault zones VIII in the lower crust and upper
mantle is taken as Maxwell viscoelastic material. Its constitutive relationship is:
ε  DI 1σ  Q1σ ,
(3)
where Q is viscous material matrixes:
 1
 3

 1
 6

1
Q 1    1
 6





1
6
1
3
1

6

1
6
1

6
1
3

0
1
0
1






.




1

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After approximating the derivatives of the strain and stress by
εt 
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 εt  εt t
 σ t  σ t t


, σt 
,
t
t
t
t
Equation (3) is expressed by
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σ t  D IIIε t  σ 0 ,
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(4)
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where D III  (D I1  Q 1t ) 1 , and σ 0  D III D I1σ t t  D IIIε t t . It is found that the
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viscoelastic constitutive relation can be considered as an elastic one with initial
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stress σ 0 . Thus, the constitutive relations in the three regions can be expressed as
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integrate one:
σ t  Dε t  σ 0
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(5)
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where D  Di in Vi , i  I, II, III , σ 0  0 in VI and VII if no initial stresses, say, caused
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by heat, pore fluid pressure and so on.
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The strain and stress fields can be calculated by using ε t  Lut and
σ t  Dε t  σ 0 if ut is a solution of boundary value problem.
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Two basic equations can be obtained by following Hu et al. (2009b) on the basis
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of the principle of virtual work. One equation solves for preseismic displacement ut or
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strain ε t :
 ε Dε dV  
T
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V
t
V
uTf t dV   uTqt dS   εTσ0dV
S2
V
(6)
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where u T and ε T are the virtual displacement and virtual strain, respectively,
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σt  [ xx  yy  zz  yz  xz  xy ]T and εt  [ xx  yy  zz  yz  xz  xy ]T are the stress and
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strain at time t, respectively, f t and qt are body force and traction force,
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respectively, and D and σ 0 are the material matrix and initial or previous stresses,
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respectively.
The other equation solves the co-, and, postseismic displacement, u and
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strain ε , which are caused by an earthquake:

V
εT (D  D)εdV  εT D εt dV   εT σ0dV   uT (f )dV   uT (q)dS2 (7)
V
V
V
S2
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where ε  Lu is the co- or postseismic strain field in the domain V, and
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D , σ 0 , f , and q are the changes in the material matrix, stress matrix, body force,
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and traction force, respectively.
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The material change or weakening, D , is only limited to the fault zone during
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the coseismic interval. If fault healing is considered in the postseismic process,
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the D is a function of time. If f and q are much smaller than the contribution of the
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first term of right hand of Equation (7) during an earthquake sequence or a
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quasi-earthquake cycle, Equation (7) can be reduced to

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V
ε T (D  D)εdV   ε T D ε t dV   ε T σ 0 dV .
V
V
(8)
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After finite element discretization in V, Equations (6) is developed into the
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finite element formula to solve the preseismic displacement field U t caused by the
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body force in V and traction on the boundary S2:
KU t  F
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Ut
s1
(9)
 U s1
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where U s1 is the displacement vector specified on the boundary S1, and K and F are
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the preseismic global stiffness matrix and nodal load vector, respectively.
III
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Ni
K    e B Di BdV ,
T
i  I e 1
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Vi
e
III
Ni
F   (  e [HTf t  BTσ 0 ]dV e   e HTqt dS2e )
i  I e 1
Vi
s2
The summation symbol in the equation means assembling elements. H is the
shape function matrix, B  LH is a connection matrix between the displacement and
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strain, and Ni is the number of the elements in the region Vi .
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Equation (7) can be developed into the finite element formula for
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solving the co- and postseismic displacement field U , induced by material
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weakening under the control of the preseismic displacement field U t :
K c (D, D)U  F(Ut )  F(f t , qt , σ 0 )
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U
s1
(10)
 U s1
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where U s1 is the displacement change vector specified on the boundary S1, and
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K c    e BT (Di  Di )BdV e , F(Ut )    e BT Di BUt dVi e ,
Ni
III
i  I e 1
III
Vi
i  I e 1
III
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Ni
Vi
Ni
F(f , q , σ )   (  e [HT f t  BT σ 0 ]dV e   e HT qt dS2e ) .
t
t
0
i  I e 1
Vi
s2
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References
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Cai, Y., and Y. Yin (1997), The Finite Element Method and Program Design of
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Thermo-elastic Problem (in Chinese), Beijing, Peking University Press, 348p.
Hu, C., Y. Zhou, and Y. Cai (2009a), A new finite element model in studying
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earthquake triggering and continuous evolution of stress field, Science in China
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Series D: Earth Sciences, 52(7), 994-1004, doi:10.1007/S11430-009-0082-3.
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Hu, C., Y. Zhou, Y. Cai, and C.-Y. Wang (2009b), Study of earthquake triggering
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in a heterogeneous crust using a new finite element model, Seismological
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Research Letters, 80(5), 795-803, doi:10.1785/gssrl.80.5.799.
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