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Zienkiewicz O.C., Taylor R.L. Vol. 3. The finite - tiera.ru

Zienkiewicz O.C., Taylor R.L. Vol. 3. The finite - tiera.ru

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54 Convection dominated problems<br />

This can be written in a compact matrix form similar to Eq. (2.93) as<br />

in which, with<br />

M ~ ˆÿ t‰…C ‡ K u ‡ K† ~ ‡ fŠ n<br />

@<br />

Gi ˆÿkij @xj …2:129a†<br />

we have (on omitting the third derivative terms and the e€ect of S) matrices of the<br />

form of Eq. (2.94), i.e.<br />

…<br />

C ˆ N T @N<br />

Ai d<br />

@xi … T<br />

@N<br />

Ku ˆ<br />

@xi AiAj t<br />

2<br />

@N<br />

d<br />

@xj … T<br />

@N<br />

K ˆ<br />

…<br />

f ˆ<br />

…<br />

M ˆ<br />

@x i<br />

@N<br />

d<br />

kij @xj N T ‡ t<br />

2 A @N<br />

i<br />

T<br />

@xi N T N d<br />

Q d ‡ boundary terms<br />

…2:129b†<br />

With ˆ 1 3 it can be shown that the order of approximation increases and for this<br />

scheme a simple iterative solution is possible. 71 We note that with the consistent<br />

mass matrix M the stability limit for ˆ 1<br />

3 is increased to C ˆ 1.<br />

Use of ˆ 1<br />

3 apparently requires an implicit solution. However, similar iteration to<br />

that used in Eq. (2.104) is rapidly convergent and the scheme can be used quite<br />

economically.<br />

2.10.2 Two-step predictor±corrector methods. Two-step<br />

<strong>Taylor</strong>±Galerkin operation<br />

<strong>The</strong>re are of course various alternative procedures for improving the temporal<br />

approximation other than the <strong>Taylor</strong> expansion used in the previous section. Such<br />

procedures will be particularly useful if the evaluation of the derivative matrix A<br />

can be avoided. In this section we shall consider two predictor±corrector schemes<br />

(of Runge±Kutta type) that avoid the evaluation of this matrix and are explicit.<br />

<strong>The</strong> ®rst starts with a standard Galerkin space approximation being applied to the<br />

basic equation (2.1). This results in the form<br />

M d~<br />

dt M _~ ˆ P C ‡ P D ‡ f ˆ w …2:130†

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