14.12.2012 Views

GUIDE WAVE ANALYSIS AND FORECASTING - WMO

GUIDE WAVE ANALYSIS AND FORECASTING - WMO

GUIDE WAVE ANALYSIS AND FORECASTING - WMO

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

the energy flux is c gH 2 . This is a constant. Hence the<br />

shoaling factor depends on the ratio between the deepwater<br />

group velocity c g0 and the group velocity c g at<br />

depth h, and is given by:<br />

<strong>WAVE</strong> <strong>FORECASTING</strong> BY MANUAL METHODS 53<br />

(4.10)<br />

where c 0 is the phase velocity in deep water (√g/k 0),<br />

k 0 is the wavenumber in deep water and H 0 is the wave<br />

height in deep water. Since the group velocity c g is given<br />

by:<br />

c<br />

g<br />

K<br />

H cg<br />

= = =<br />

H c<br />

g<br />

1 ⎛ kh ⎞<br />

= β tanh kh , β = ⎜ + ⎟ ,<br />

k<br />

2 ⎝ sinh kh⎠<br />

1<br />

2<br />

2<br />

the shoaling factor can also be expressed as:<br />

10<br />

1<br />

0.1<br />

0.01<br />

s<br />

0<br />

1 c<br />

c<br />

0 0<br />

g 2 g<br />

,<br />

c/c0 . λ/λ0<br />

K = 2 β tanh kh .<br />

s<br />

– 1/ 2<br />

(4.11)<br />

The wavenumber k = 2π/λ at depth h can be<br />

approximated as follows:<br />

k = k 0 (tanh kh) –1 ,<br />

k = k 0 [tanh (k 0 h tanh kh) –1 ] –1 ≈ k 0 (tanh k 0 h) –1 . (4.12)<br />

Figure 4.7(a) shows various curves involved in the<br />

transformation of properties of a wave propagating from<br />

deep to shallow water. The shoaling factor, K s, is also<br />

shown in this figure. But for the convenience of the<br />

user interested in obtaining only the shoaling factor K s<br />

associated with a deep water wave of a given wavenumber<br />

k 0 (= 2π/λ 0), the curve of K s vs h/λ 0 is presented<br />

in Figure 4.7(b) in an expanded scale.<br />

0.0001 0.001 0.01 0.1 1<br />

h/λ0<br />

Figure 4.7(a) — Illustration of various functions of h/λ 0 (derived from CERC, 1984)<br />

K s<br />

cg/c0<br />

h/λ<br />

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!