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Universität Karlsruhe (TH) - am Institut für Baustatik

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3 Finite Element Equations<br />

3.1 Interpolation of the initial and current reference surface<br />

In this section the finite element equations for quadrilaterals are specified applying the isopar<strong>am</strong>etric<br />

concept. The local numbering of the corner nodes and midside node can be seen in<br />

Fig. 1.<br />

4<br />

D<br />

3<br />

X 3<br />

h<br />

A p<br />

3<br />

<br />

C<br />

h<br />

1 midsurface ( =0)<br />

B<br />

2<br />

<br />

X 2 X 1 Figure 1: Quadrilateral shell element<br />

A map of the coordinates {ξ,η} ∈[−1, 1] from the unit square to the midsurface in the initial<br />

and current configuration is applied. Thus the position vector and the director vector of the<br />

reference surface are interpolated with bi–linear functions<br />

4∑<br />

4∑<br />

X h = N I X I D h = N I D I N I = 1<br />

I=1<br />

I=1<br />

4 (1 + ξ Iξ)(1 + η I η) (12)<br />

with ξ I ∈ {−1, 1, 1, −1} and η I ∈ {−1, −1, 1, 1}. The superscript h denotes the<br />

characteristic size of the element discretization and indicates the finite element approximation.<br />

The nodal position vectors X I and local cartesian basis systems [A 1I , A 2I , A 3I ] are generated<br />

within the mesh input. Here, D I = A 3I is perpendicular to Ω and A 1I , A 2I are constructed in<br />

such a way that the boundary conditions can be accommodated. With (12) 2 the orthogonality<br />

is only given at the nodes.<br />

For each element a local cartesian basis t i is evaluated<br />

¯d 1 = X 3 − X 1 ̂d 1 = ¯d 1 /|¯d 1 |<br />

¯d 2 = X 2 − X 4 ̂d 2 = ¯d 2 /|¯d 2 |<br />

t 1 = (̂d 1 + ̂d 2 )/|̂d 1 + ̂d 2 |<br />

t 2 = (̂d 1 − ̂d 2 )/|̂d 1 − ̂d 2 |<br />

t 3 = t 1 × t 2 .<br />

(13)<br />

One could also use the so-called l<strong>am</strong>ina basis according to [26] where the base vectors t α lie<br />

6

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