Geology Reference
In-Depth Information
The law of conservation of energy equates the gain of energy within the surface
S
, given by the sum of (6.118), (6.120) and (6.121), to the energy entering the
system (6.123). Since the volume is arbitrary, integrands are equated, giving
ρ T s
s
1
2 ρv k v k
2 ρv k v k
+
t
+
x j
1
t +
v
·∇
p
∇·
v
v j ·
k T
x j
x j τ ji v i
x j
ρ f j v j
=
+
H .
(6.124)
Expanding derivatives, this equation can be rearranged to
ρ T s
s
2 v k v k ∂ρ
x j ρv j
+ ρv k ∂v k
1
t + v j ∂v k
t +
v
·∇
p
∇·
v
+
t +
x j
k T
x j
v i ∂τ ji
x j τ ji ∂v i
x j
ρ f j v j
x j =
+
H .
(6.125)
It can be further simplified using the mass conservation equation (6.90) and the
equation of motion (6.103) to give
ρ T s
s
k T
x j
x j
+ τ ji ∂v i
t +
v
·∇
=
+
H
+
p
∇·
v
x j .
(6.126)
The left side of the equation of energy conservation (6.126) can be further trans-
formed using a Tds equation from thermodynamics,
α
ρ
Tds
=
c p dT
Tdp ,
(6.127)
where c p is the specific heat at constant pressure and
∂ρ
T
1
ρ
α =−
(6.128)
p
is the volume coe
cient of thermal expansion. Then, we have
ρ T s
·∇ s
= ρ c p T
·∇ T
α T p
·∇ p
t +
v
t +
v
t +
v
.
(6.129)
For an isotropic viscous fluid, the viscous stress resisting deformation is given
by (6.115), and we have
∂v j
x i +
j
j
τ ji ∂v i
∂v i
x j
∂v i
x j
2
3 ∇·
i
j
i
i
x j =
p δ
+ η
v δ
+ ζ ∇·
v δ
∂v j
x i +
j
+ η ∂v i
x j
∂v i
x j
2
3 ∇·
i
v ) 2
=−
p
∇·
v
v δ
+ ζ (
∇·
.
(6.130)
 
Search WWH ::




Custom Search