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GUIDE WAVE ANALYSIS AND FORECASTING - WMO

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30<br />

a general sense, and can be applied to the atmosphere.<br />

These concepts have been developed to formulate diagnostic<br />

models that allow us to deduce surface turbulent<br />

flow fields from the free atmospheric flow.<br />

The marine boundary layer itself can be separated<br />

into two regimes: the constant flux (or constant stress)<br />

layer (from the surface to about 50 m) and the Ekman<br />

layer (from about 50 m up to the free atmosphere<br />

≈ 1 km). In the surface layer it can be assumed that the<br />

frictional forces contributing to turbulence are constant<br />

with height, and the effects of the Coriolis and pressure<br />

gradient forces, as well as the horizontal gradient of<br />

turbulent fluxes, are negligible. The wind direction is<br />

consequently constant with height. Using the mixing<br />

length theory developed by Prandtl, it can be shown<br />

that the flow in the constant flux layer (or Prandtl layer)<br />

depends only on the surface roughness length.<br />

2.4.1 Constant flux layer<br />

Under neutral conditions, Prandtl’s solution shows that<br />

the horizontal flow over the ocean surface follows the<br />

well known “log” (logarithmic) profile in the vertical<br />

direction,<br />

u = u *<br />

κ ln<br />

(2.8)<br />

where κ is the von Kármán constant, z 0 is the constant of<br />

integration, known as the roughness length, and u * is the<br />

friction velocity, which has magnitude:<br />

u * =<br />

⎛ z ⎞<br />

⎜ ⎟<br />

⎝ ⎠<br />

,<br />

(2.9)<br />

τ is the magnitude of the surface stress, and ρa the<br />

density of air. u * can be thought of as a proxy for the<br />

surface stress.<br />

It is common also to express stress (τ) through the<br />

bulk transfer relation:<br />

τ = ρa Cd u2 , (2.10)<br />

where Cd is the drag coefficient. In general, Cd and u are<br />

both functions of height. Determining Cd has been the<br />

objective of many field research programmes over the<br />

years.<br />

One of the problems of specifying the wind in the<br />

turbulent layer near the ocean is the formulation of z0 and its relationship to u *. Using dimensional argument,<br />

Charnock (1955) related the roughness length of the sea<br />

surface to the friction velocity of the wind as follows:<br />

z0 = (2.11)<br />

where α is the Charnock constant, with a value as determined<br />

by Wu (1980) of 0.0185 , and g is the acceleration<br />

by gravity.<br />

If the boundary layer is in a state of neutral stratification,<br />

the drag coefficient, which is a function of<br />

height, can be expressed as:<br />

αu * 2<br />

,<br />

g<br />

τ<br />

ρ a<br />

z 0<br />

,<br />

<strong>GUIDE</strong> TO <strong>WAVE</strong> <strong>ANALYSIS</strong> <strong>AND</strong> <strong>FORECASTING</strong><br />

or<br />

C z<br />

d( )=<br />

κ 2<br />

Cd ( z)<br />

=<br />

⎛ ⎡ z ⎤⎞<br />

/ ⎜ln<br />

⎢ ⎥<br />

⎝ ⎣ z<br />

⎟ ,<br />

0 ⎦⎠<br />

⎛ u * ⎞<br />

⎜ ⎟<br />

⎝ uz⎠<br />

( )<br />

(2.12)<br />

(2.13)<br />

However, the boundary layer over the ocean is not<br />

necessarily neutral. A stability dependence was originally<br />

derived by Monin-Obukhov (1954) from profile<br />

similarity theory. This is used to modify the simple log<br />

relation provided above:<br />

u = (2.14)<br />

u *<br />

κ ln<br />

⎡ ⎛ z ⎞<br />

⎜ ⎟ – ψ<br />

⎛ z ⎞ ⎤<br />

⎢<br />

⎝ z0 ⎠ ⎝ L ⎠<br />

⎥<br />

⎣⎢<br />

⎦⎥<br />

⎛ ⎡ ⎛ z ⎞<br />

C z<br />

⎛ z ⎞⎤⎞<br />

d( )= ⎜κ<br />

/ ⎢ln<br />

⎜ ⎟ – ψ<br />

(2.15)<br />

⎝ z ⎠ ⎝ L⎠<br />

⎥⎟<br />

.<br />

⎝ ⎣⎢<br />

0 ⎦⎥<br />

⎠<br />

The function ψ has been derived for both stable and<br />

unstable conditions. L is the Monin-Obukhov mixing<br />

length. For neutral conditions ψ (z/L) = 0. Businger et al.<br />

(1971) proposed functional relationships between the<br />

non-dimensional wind shear and z/L which can be used<br />

to determine the stability function ψ (z/L) in Equation<br />

2.14.<br />

2.4.2 The use of the drag coefficient<br />

In the above discussion, we developed the concept of the<br />

drag coefficient, as defined in Equation 2.10. There have<br />

been many studies to determine Cd under varying wind<br />

speeds and stabilities and a summary can be found in<br />

Roll (1965). More recently, Wu (1980, 1982) has shown<br />

through empirical studies that the drag coefficient at a<br />

given height depends linearly on the wind speed, and<br />

that the following formulation holds for a wide range of<br />

winds under near neutrally stable conditions:<br />

103 C10 = (0.8 + 0.65 U10) (2.16)<br />

where: C10 = Drag coefficient at the 10 m level; and<br />

U10 = Wind speed (m/s) at the 10 m level.<br />

This simple linear empirical relationship, however,<br />

needs to be modified when temperature stratification is<br />

present. Stratification affects turbulent momentum transport,<br />

thereby causing the wind profile to deviate from the<br />

logarithmic form.<br />

Schwab (1978) determined Cd over water for a<br />

wide range of wind speeds and atmospheric stabilities.<br />

Figure 2.9 shows the results of his calculation. A crucial<br />

issue to be addressed at this juncture concerns the effect<br />

of changing stability and wind stress on the prediction<br />

of wave growth. It can be inferred from Figure 2.9 that,<br />

for a given 10 m level wind speed, unstable conditions<br />

result in higher drag coefficients (or surface stress) and<br />

hence larger wave growth than stable conditions. Liu et<br />

al. (1979) have developed a set of equations which<br />

compute the surface variables u * , z0 and the boundarylayer<br />

stability length (L), so that the wind profile of<br />

2<br />

.<br />

2<br />

2

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