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Eduardo Kausel-Fundamental solutions in elastodynamics_ a compendium-Cambridge University Press (2006)

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10.4 Stiffness matrix method for layered spheres 181<br />

such that<br />

⎧<br />

⎨ ξ<br />

˜F m = Q m F m =<br />

⎩<br />

⎧<br />

⎨ ξ<br />

˜H m = Q m H m =<br />

⎩<br />

1<br />

1<br />

⎫ ⎧<br />

⎫<br />

⎬ ⎨ f 11 f 12 0 ⎬<br />

f<br />

⎭ ⎩ 21 f 22 0<br />

⎭<br />

1 0 0 f 33<br />

⎫ ⎧<br />

⎫<br />

⎬ ⎨ h 11 h 12 0 ⎬<br />

h<br />

⎭ ⎩ 21 h 22 0<br />

⎭<br />

1 0 0 h 33<br />

(10.158)<br />

(10.159)<br />

which implies<br />

ū = T n L n m Q−1 m Q m H m c<br />

= T n L n m Q−1 ˜H m m c<br />

and<br />

¯p = T n L n m Q−1 m Q m F m c<br />

= T n L n m Q−1 ˜F m m c<br />

⇒<br />

⇒<br />

ū = T n L n m Q−1 m ũ (10.160)<br />

¯p = T n L n m Q−1 m ˜p<br />

= T n L n m Q−1 ˜K m ũ<br />

(10.161)<br />

For example, for an exterior region, the scaled, symmetric impedance matrix would be<br />

˜K =−R 2 ˜F m<br />

(<br />

˜H m<br />

) −1<br />

⇒ ˜K = Q m KQ −1<br />

m (10.162)<br />

which relates the scaled force and displacement amplitudes vectors at the <strong>in</strong>terface of the<br />

outer region. More generally, <strong>in</strong> the case of a system of layers, we obta<strong>in</strong> a symmetric<br />

global system matrix. However, to avoid proliferation of symbols, we cont<strong>in</strong>ue label<strong>in</strong>g<br />

the scaled vectors for the system as we did for any <strong>in</strong>dividual layer, and write the system<br />

equation simply as<br />

˜p = ˜K ũ ⇒ ũ = ˜K −1 ˜p (10.163)<br />

In this equation, every third (SH) degree of freedom is uncoupled from the preced<strong>in</strong>g<br />

two (SV-P) degrees of freedom, so they should be solved separately. The advantage of<br />

us<strong>in</strong>g a symmetric stiffness matrix lies <strong>in</strong> the sav<strong>in</strong>g <strong>in</strong> computational effort, which is a<br />

factor of two. For notational transparency, however, we present the ensu<strong>in</strong>g examples <strong>in</strong><br />

the standard, non-symmetric form.<br />

10.4.3 Expansion of source and displacements <strong>in</strong>to spherical harmonics<br />

The stiffness matrix method described here<strong>in</strong> is based on a formulation <strong>in</strong> the frequency–<br />

spheroidal-wavenumber doma<strong>in</strong>. Thus, the sources p = p(R,φ,θ,ω), if any, must be<br />

expressed <strong>in</strong> terms of spheroidal harmonics of order m,n, i.e., ˜p ≡ ˜p mn (R,ω)<br />

Let p be the 3 × 1 vector of external tractions per solid angle at a given frequency, which<br />

we assume to be def<strong>in</strong>ed over a spherical surface of constant radius R. Expansion <strong>in</strong>to<br />

spheroidal harmonics yields<br />

∞∑ m∑<br />

p = T n L n m ˜p mn (10.164)<br />

m=0 n=0

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