Mathematical Physics - Volume II - Numerical Methods
Chapter 3. Comparison of finite element method and finite difference method
76
e Ω
y
T e
x
η
(1,1)
(-1,1)
ξ
Ω ^
(1,-1)
(-1,-1)
Figure 3.17: Local to global transformation.
Partial derivative matrix of the 2 × 2 order is called the transformation Jacobian and is denoted by J . In order for the inverse transformation to hold, it is obvious that | J |̸ = 0. In this case, we have that: d ξ d η = J − 1 d x d y = 1 | J | ∂ y ∂η ∂ x ∂η − ∂ y ∂ ξ ∂ x ∂ ξ d x d y , (3.123)
thus
ξ = ξ ( x , y ) η = η ( x , y )
(3.124)
Defines the inverse transformation. Considering the below expression, analogous to (3.122)
d η = ∂ ξ ∂ x ∂η ∂ x
∂ ξ ∂ y ∂η ∂ y
d ξ
d x d y
(3.125)
it is clear that the following holds: ∂ ξ ∂ x = 1 | J | ∂ y ∂η ,
∂ ξ ∂ y
∂ x ∂η , ∂ x ∂ ξ .
1 | J | 1 | J |
= −
(3.126)
∂η ∂ x
∂ y ∂ ξ ,
∂η ∂ y
1 | J |
= −
=
Now we can define the conditions necessary for a function in order to be used as a transformation function: 1. Within each element, functions ξ = ξ ( x , y ) and η = η ( x , y ) must be invertible and continu ously differentiable in order for the relation (3.126) to be applicable to them. 2. Mesh generated using a series of transformations [ T e ] must not contain overlapping elements and empty spaces between them.
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