Geoscience Reference
In-Depth Information
The following difference schemes for the first and second derivatives of f can be
derived from Eq. (4.96) (Wu, 1996b):
9
9
f
f
x =
a k f k ,
y =
b k f k
(4.97)
k
=
1
k
=
1
9
9
2 f
2 f
=
c k f k ,
=
d k f k
(4.98)
x 2
y 2
k
=
1
k
=
1
where a k , b k , c k , and d k are coefficients:
1 ∂ϕ
1 ∂ϕ
2 ∂ϕ
2 ∂ϕ
k
∂ξ + α
k
∂η
k
∂ξ + α
k
∂η
1
2
1
2
a k = α
, b k = α
,
1
1
∂ξ + α
1
1
∂η
2
2
2
1 ∂α
1 ∂α
1
ϕ
1
ϕ
1
ϕ
∂ϕ
k
k
∂ξ∂η + α
k
k
∂ξ
1
1
1
1
1
2
2
1
2
1
2
c k
= α
α
+
2
α
α
α
+
α
2
2
∂ξ
∂η
α
2
1
∂ξ + α
2
1
∂η
1 ∂α
1 ∂α
∂ϕ k
∂η
1
2
+
,
and
α
2
2
2
1
2
1
2
∂η
2
ϕ k
∂ξ
2
ϕ k
∂ξ∂η + α
2
ϕ k
∂η
2 ∂α
2 ∂α
∂ϕ k
∂ξ
1
2
1
1
2
2
2
2
2
1
2
d k = α
α
+
2
α
α
α
+
∂ξ + α
2
2
2
2
2
2
∂η
2 ∂α
2 ∂α
∂ϕ k
∂η
1
2
+
α
∂ξ + α
.
Eqs. (4.97) and (4.98) can be applied to any point in the local element. For example,
for the central point 5, one can obtain a k , b k , c k , and d k by specifying
0.
The isoparametric interpolation formula (4.96) can be extended to the 3-D case using
the interpolation functions (4.88) based on the 27-point element shown in Fig. 4.9, and
similar difference schemes for the 3-D first and second derivatives can be easily derived.
Note that the difference schemes (4.97) are similar to the central difference scheme
(4.13); thus, they are not as adequate for strong convection problems as the exponen-
tial difference scheme (4.95) and the upwind interpolation method introduced in the
next subsection.
ξ = η =
4.2.4.2 Upwind interpolation method on fixed grids
Wang and Hu (1993) analytically solved the following convection-diffusion equation
with constant velocity, diffusivity, and source term in the 1-D local element shown
in Fig. 4.12:
d 2 f
d
u df
d
S
ˆ
ξ = ε ξ
2 +
(4.99)
ξ
and derived the upwind interpolation functions:
 
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