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Universität Karlsruhe (TH) - am Institut für Baustatik

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as close as possible to the coordinates ξ and η. Hence the Jacobian matrix J is defined<br />

with<br />

⎡<br />

J = ⎣ Xh , ξ ·t 1 X h ⎤<br />

, ξ ·t 2<br />

⎦ (14)<br />

X h , η ·t 1 X h , η ·t 2<br />

X h , ξ = G 0 ξ + η G 1 G 0 ξ = 1 4∑<br />

ξ I X I<br />

4<br />

I=1<br />

X h , η = G 0 η + ξ G 1 G 0 η = 1 4∑<br />

η I X I<br />

4<br />

I=1<br />

G 1 = 1 4∑<br />

ξ I η I X I .<br />

4<br />

I=1<br />

One can prove that t 3 · G 0 ξ =0andt 3 · G 0 η = 0 holds which shows that t 3 is normal vector at<br />

the element center. Thus t 1 and t 2 span a tangent plane at the center of the element. Now<br />

we are able to express the local cartesian derivatives of the shape functions using the inverse<br />

Jacobian matrix J. The tangent vectors X, α and the derivatives of the director vector D, α<br />

are computed considering (12) as follows<br />

X h , α =<br />

4∑<br />

I=1<br />

N I , α X I D h , α =<br />

4∑<br />

I=1<br />

(15)<br />

[ ] [ ]<br />

NI ,<br />

N I , α D 1<br />

I = J −1 NI , ξ<br />

. (16)<br />

N I , 2 N I , η<br />

For arbitrary warped elements one obtains X h , α = t α at the element center, which can be<br />

shown using above orthogonality conditions. This is important in the context of the present<br />

mixed interpolation. Furthermore a local cartesian system is advantageous to verify complicated<br />

nonlinear constitutive equations. At other points of the element the vectors X h , α are<br />

only approximately orthogonal.<br />

The current shell middle surface is approximated in the s<strong>am</strong>e way<br />

x h =<br />

x h , α =<br />

4∑<br />

N I x I d h =<br />

I=1<br />

4∑<br />

N I , α x I d h , α =<br />

I=1<br />

4∑<br />

N I d I<br />

I=1<br />

4∑<br />

N I , α d I ,<br />

I=1<br />

(17)<br />

where x I = X I + u I describes the current nodal position vector and d I = a 3I is obtained<br />

by an orthogonal transformation a kI = R I A kI , k =1, 2, 3. The rotation tensor R I is a<br />

function of the par<strong>am</strong>eters organized in the vector ω I =[ω 1I ,ω 2I ,ω 3I ] T and is computed via<br />

Rodrigues’ formula<br />

R I = 1 + sin ω I<br />

ω I<br />

Ω I + 1 − cos ω I<br />

Ω 2<br />

ωI<br />

2 I Ω I =skewω I =<br />

⎡<br />

⎤<br />

0 −ω 3I ω 2I<br />

ω<br />

⎢ 3I 0 −ω 1I<br />

⎥<br />

⎣<br />

⎦<br />

−ω 2I ω 1I 0<br />

Representation (18) is singularity free for ω I = |ω I | < 2π which can always be fulfilled if after<br />

a certain number of load steps a multiplicative update of the total rotation tensor is applied.<br />

7<br />

(18)

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