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WAVES AND VIBRATIONS IN INHOMOGENEOUS STRUCTURES ...

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The above expressions provide instantaneous values<br />

of the power flow. The energy transported during a<br />

single period of excitation T is defined as:<br />

<br />

W = ˆPdt (25)<br />

T<br />

This measure of the energy transported by a travelling<br />

wave is considered as the optimization objective in our<br />

second application example. In the case of a standing<br />

wave considered in the first example, W vanishes since<br />

no energy is transported in this case.<br />

The time-dependence of the solution from (6)–(8) is<br />

inserted into (23)–(24) and the integration is performed<br />

to yield the expressions<br />

<br />

Wx = π Dℜ i ˜ψx,x + ν ˜ψy,y ˜ψ ∗ <br />

x<br />

+ 1 − ν<br />

<br />

π Dℜ i ˜ψx,y + ˜ψy,x ˜ψ<br />

2 ∗ <br />

y<br />

<br />

− πkGhℜ i ˜ψx −˜w,x ˜w ∗<br />

(26)<br />

Wy =<br />

1 − ν<br />

<br />

π Dℜ i ˜ψx,y + ˜ψy,x ˜ψ<br />

2 ∗ <br />

x<br />

<br />

<br />

+π Dℜ i ν ˜ψx,x + ˜ψy,y ˜ψ ∗ <br />

y<br />

<br />

−πkGhℜ i ˜ψy −˜w,y ˜w ∗<br />

(27)<br />

where the asterisk is used to denote the complex<br />

conjugate.<br />

4 Discretized problem<br />

A standard Galerkin FE approach is used to set up a set<br />

of discretized equations based on (9)–(11):<br />

2<br />

−ω M + iωC + K d = f (28)<br />

in which M, C and K are the mass-, damping- and<br />

stiffness matrices, respectively, d is a vector containing<br />

the complex nodal variables and f is a load vector. The<br />

matrices M, C and K are collected in the system matrix<br />

S =−ω 2 M + iωC + K.<br />

M and K are assembled from the local element matrices<br />

in the usual way. These are based on the local<br />

shape functions defined as:<br />

⎧<br />

⎨<br />

⎩<br />

⎫<br />

˜w ⎬<br />

˜ψx<br />

⎭<br />

˜ψy<br />

= Nde ⎡<br />

= ⎣<br />

NT 1<br />

NT 2<br />

NT 3<br />

⎤<br />

⎦ d e<br />

(29)<br />

and from the B matrix defined as:<br />

⎧<br />

⎫<br />

˜ψx,x<br />

⎪⎨ ˜ψy,y ⎪⎬<br />

˜ψx,y + ˜ψy,x = ∂Nd<br />

˜ψx ⎪⎩<br />

−˜w,x ⎪⎭<br />

˜ψy −˜w,y<br />

e = Bd e ⎡<br />

⎢<br />

= ⎢<br />

⎣<br />

A.A. Larsen et al.<br />

N T 2,x<br />

N T 3,y<br />

N T 2,y + NT 3,x<br />

N T 2 − NT 1,x<br />

N T 3 − NT 1,y<br />

⎤<br />

⎥ d<br />

⎥<br />

⎦<br />

e<br />

(30)<br />

In all examples presented in this paper we use rectangular<br />

4-noded bilinear elements with dimensions<br />

2a by 2b.<br />

Damping is not defined in the continuous problem<br />

but included in the discretized version in the form of<br />

proportional (Rayleigh) damping:<br />

C = αM + βK (31)<br />

where α and β is the mass- and stiffness-proportional<br />

damping coefficients.<br />

The load is specified in the examples and the load<br />

vector is assembled in the usual way.<br />

Inserting the discretized displacements into the<br />

formulas for the energy transport we obtain<br />

<br />

Wx = πℜ i d eT e e<br />

Qx d ∗ <br />

(32)<br />

<br />

Wy = πℜ i d eT e e<br />

Qy d ∗ <br />

(33)<br />

in which Qe x and Qey are local element matrices defined<br />

in terms of the shape functions and their derivatives as:<br />

Q e x = D(N2,x + νN3,y)N T 1 − ν<br />

2 +<br />

2 D(N2,y + N3,x)N T 3<br />

−kGh(N2 − N1,x)N T 1<br />

(34)<br />

Q e y = D(νN2,x + N3,y)N T 1 − ν<br />

3 +<br />

2 D(N2,y + N3,x)N T 2<br />

−kGh(N3 − N1,y)N T 1<br />

(35)<br />

The energy transport in the x− and y−direction<br />

through a single element is given as:<br />

W e x =<br />

<br />

Wxdy, W e y =<br />

<br />

Wydx (36)<br />

e<br />

e<br />

By assuming uniform energy transport through an element<br />

we approximate this as<br />

W e x =<br />

<br />

πℜ i<br />

e<br />

d eT e e<br />

Qx d ∗ <br />

dy<br />

<br />

≈ 2bπℜ i d eT <br />

˜Q e e<br />

x d ∗ <br />

(37)<br />

W e y =<br />

<br />

πℜ i<br />

e<br />

d eT e e<br />

Qy d ∗ <br />

dx<br />

<br />

≈ 2aπℜ i d eT <br />

˜Q e e<br />

y d ∗ <br />

(38)

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