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USER MANUAL SWAN Cycle III version 40.72A

USER MANUAL SWAN Cycle III version 40.72A

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90 Appendix A<br />

TM02<br />

Mean absolute wave period (in s) of E(ω,θ), defined as<br />

(∫ ∫ ) ω<br />

T m02 = 2π<br />

2 −1/2 (∫ ∫ )<br />

E(ω,θ)dωdθ<br />

∫ ∫ ω<br />

E(ω,θ)dωdθ<br />

= 2π 2 −1/2<br />

E(σ,θ)dσdθ<br />

∫ ∫ E(σ,θ)dσdθ<br />

DIR<br />

PDIR<br />

TDIR<br />

RTMM10<br />

Mean wave direction (in o , Cartesian or Nautical convention),<br />

as defined by (see Kuik et al. (1988)):<br />

⌊ ∫ ⌋<br />

sin θE(σ,θ)dσdθ<br />

DIR = arctan ∫ cos θE(σ,θ)dσdθ<br />

This direction is the direction normal to the wave crests.<br />

Peak direction of E(θ) = ∫ E(ω,θ)dω = ∫ E(σ,θ)dσ<br />

(in o , Cartesian or Nautical convention).<br />

Direction of energy transport (in o , Cartesian or Nautical convention).<br />

Note that if currents are present, TDIR is different from the mean wave<br />

direction DIR.<br />

Mean relative wave period (in s) of E(σ,θ), defined as<br />

∫ ∫ σ<br />

RT m−10 = 2π<br />

−1 E(σ,θ)dσdθ<br />

∫ ∫ E(σ,θ)dσdθ<br />

RTM01<br />

This is equal to TMM10 in the absence of currents.<br />

Mean relative wave period (in s) of E(σ,θ), defined as<br />

(∫ ∫ ) −1<br />

σE(σ,θ)dσdθ<br />

RT m01 = 2π ∫ ∫ E(σ,θ)dσdθ<br />

RTP<br />

TPS<br />

PER<br />

This is equal to TM01 in the absence of currents.<br />

Relative peak period (in s) of E(σ) (equal to absolute peak period<br />

in the absence of currents).<br />

Note that this peak period is related to the absolute maximum bin of the<br />

discrete wave spectrum and hence, might not be the ’real’ peak period.<br />

Relative peak period (in s) of E(σ).<br />

This value is obtained as the maximum of a parabolic fitting through the<br />

highest bin and two bins on either side the highest one of the discrete<br />

wave spectrum. This ’non-discrete’ or ’smoothed’ value is a better<br />

estimate of the ’real’ peak period compared to the quantity RTP.<br />

Average absolute period (in s) of E(ω,θ), defined as<br />

∫ ∫ ω<br />

T m,p−1,p = 2π<br />

p−1 E(ω,θ)dωdθ<br />

∫ ∫ ω p E(ω,θ)dωdθ<br />

The power p can be chosen by the user by means of the QUANTITY

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