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Internal Wave Generation in Uniformly Stratified Fluids. 1 ... - LEGI

Internal Wave Generation in Uniformly Stratified Fluids. 1 ... - LEGI

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5. EXACT GREEN’S FUNCTION<br />

5.1. Monochromatic Green’s function<br />

For ω > N, rescal<strong>in</strong>g the coord<strong>in</strong>ates accord<strong>in</strong>g to<br />

rh' = ω<br />

N rh and z' = ω2 – N2 1/2<br />

N<br />

z (5.1)<br />

reduces equation (3.15) for the monochromatic Green’s function G(r, ω) to a Helmholtz-like<br />

equation, whose Green’s function is given for <strong>in</strong>stance by Bleiste<strong>in</strong> (1984 p. 177). Return<strong>in</strong>g<br />

to the orig<strong>in</strong>al coord<strong>in</strong>ate system described <strong>in</strong> figure 5 yields<br />

G(r, ω) = 1<br />

4πr<br />

1/2<br />

–<br />

e<br />

βr<br />

2 ω2 – N2 cos2θ ω2 – N2 ω2 – N2 1/2<br />

ω2 – N2 cos2θ 1/2 . (5.2)<br />

As implied by the Pierce-Hurley radiation condition, the analytic cont<strong>in</strong>uation of this result over<br />

the lower half of the complex ω plane provides the value of the Green’s function on the whole<br />

real ω axis. The branch cuts emanat<strong>in</strong>g from the branch po<strong>in</strong>ts ± N, ± N⏐cos θ⏐ are taken as<br />

extend<strong>in</strong>g vertically upwards, as shown <strong>in</strong> figure 6. Thus, the phase of complex square roots<br />

of the form (ω 2 – ω 0 2 ) 1/2 has the follow<strong>in</strong>g behaviour on the real axis:<br />

ph ω 2 – ω 0 2 1/2 = 0 ω > ω0 , (5.3a)<br />

= – π/2 ω < ω0 , (5.3b)<br />

= – π ω < – ω0 . (5.3c)<br />

Denot<strong>in</strong>g from now on complex square roots, def<strong>in</strong>ed by (5.3), as powers 1/2 and real<br />

square roots by a square root symbol, we obta<strong>in</strong> for the Green’s function at every real<br />

frequency<br />

G(r, ω) = 1<br />

4πr e<br />

– βr ω<br />

2<br />

2 – N2 cos2θ ω2 – N2 ω2 – N2 ω2 – N2 cos2θ = i<br />

<strong>Internal</strong> wave generation. 1. Green’s function 15<br />

sgn ω<br />

4πr e<br />

– i βr<br />

2<br />

ω 2 – N 2 cos 2 θ<br />

N 2 – ω 2<br />

N 2 – ω 2 ω 2 – N 2 cos 2 θ<br />

sgn ω<br />

ω > N , (5.4a)<br />

N cos θ < ω < N , (5.4b)

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