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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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<strong>Internal</strong> wave generation. 1. Green’s function 58<br />

Figure 9. Po<strong>in</strong>ts of contact T + and T – of the uppermost and lowermost tangents from a<br />

po<strong>in</strong>t r to the sphere.<br />

Figure 10. Bouss<strong>in</strong>esq <strong>in</strong>ternal wave field of a monochromatically pulsat<strong>in</strong>g sphere. <strong>Wave</strong>s<br />

are conf<strong>in</strong>ed <strong>in</strong> regions III and V, bounded by characteristic cones of semi-angle<br />

θ 0 = arc cos (ω/N). There, coord<strong>in</strong>ates σ ± describe transverse distances, with<br />

which the phase variates.<br />

Figure 11. Bouss<strong>in</strong>esq <strong>in</strong>ternal wave field of an impulsively pulsat<strong>in</strong>g sphere. Out of the<br />

characteristic torus of radius Nta gravity waves, whose surfaces of constant phase<br />

are conical (cf. figure 2), dom<strong>in</strong>ate. Inside the torus they give way to buoyancy<br />

oscillations, whose phase is constant.<br />

Figure 12. Orig<strong>in</strong>al <strong>in</strong>tegration path (dotted l<strong>in</strong>e), and steepest descent contours (heavy<br />

l<strong>in</strong>es), for the asymptotic expansion of (D12). The saddle po<strong>in</strong>ts ω 1 and ω 2 are<br />

situated a distance (α/2t) 2/3 from the orig<strong>in</strong> ω 3 = 0 which makes no contribution to<br />

the expansion.

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