USER MANUAL SWAN Cycle III version 40.72A
USER MANUAL SWAN Cycle III version 40.72A USER MANUAL SWAN Cycle III version 40.72A
88 Chapter 4 ’fname’ name of the file to which the wave field is written. Note: for parallel MPI runs, more than one hotfile will be generated depending on the number of processors (fname-001, fname-002, etc.). STOP This required command marks the end of the commands in the command file. Note that the command STOP may be the last command in the input file; any information in the input file beyond this command is ignored.
Appendix A Definitions of variables In SWAN a number of variables are used in input and output. Most of them are related to waves. The definitions of these variables are mostly conventional. HSIGN Significant wave height, denoted as H s in meters, and defined as H s = 4√ ∫ ∫ E(ω,θ)dωdθ where E(ω,θ) is the variance density spectrum and ω is the absolute radian frequency determined by the Doppler shifted dispersion relation. However, for ease of computation, H s can be determined as follows: H s = 4√ ∫ ∫ E(σ,θ)dσdθ HSWELL Significant wave height associated with the low frequency part of the spectrum, denoted as H s,swell in meters, and defined as H s,swell = 4√ ∫ ωswell 0 ∫ 2π 0 E(ω,θ)dωdθ TMM10 with ω swell = 2πf swell and f swell = 0.1 Hz by default (this can be changed with the command QUANTITY). Mean absolute wave period (in s) of E(ω,θ), defined as ∫ ∫ ∫ ω T m−10 = 2π −1 E(ω,θ)dωdθ ∫ ∫ ω E(ω,θ)dωdθ = 2π∫ −1 E(σ,θ)dσdθ ∫ ∫ E(σ,θ)dσdθ TM01 Mean absolute wave period (in s) of E(ω,θ), defined as (∫ ∫ ) −1 (∫ ∫ ) −1 ωE(ω,θ)dωdθ T m01 = 2π ∫ ∫ ωE(σ,θ)dσdθ E(ω,θ)dωdθ = 2π ∫ ∫ E(σ,θ)dσdθ 89
- Page 45 and 46: Description of commands 37 y ′
- Page 47 and 48: Description of commands 39 [fac]
- Page 49 and 50: Description of commands 41 ’(10X,
- Page 51 and 52: Description of commands 43 | | East
- Page 53 and 54: Description of commands 45 CONSTANT
- Page 55 and 56: Description of commands 47 points o
- Page 57 and 58: Description of commands 49 CRAY WKS
- Page 59 and 60: Description of commands 51 This com
- Page 61 and 62: Description of commands 53 | JANSse
- Page 63 and 64: Description of commands 55 [Csh3] c
- Page 65 and 66: Description of commands 57 [ursell]
- Page 67 and 68: Description of commands 59 [slope]
- Page 69 and 70: Description of commands 61 [cgmod]
- Page 71 and 72: Description of commands 63 < > [lim
- Page 73 and 74: Description of commands 65 SIGIMPL
- Page 75 and 76: Description of commands 67 ’sname
- Page 77 and 78: Description of commands 69 (see bel
- Page 79 and 80: Description of commands 71 [alpn] d
- Page 81 and 82: Description of commands 73 ‘long
- Page 83 and 84: | HSign | | | | HSWEll | | | | DIR
- Page 85 and 86: Description of commands 77 | WLENgt
- Page 87 and 88: Description of commands 79 QP DEPTH
- Page 89 and 90: Description of commands 81 [tbegblk
- Page 91 and 92: Description of commands 83 OUTput [
- Page 93 and 94: Description of commands 85 If SWAN
- Page 95: Description of commands 87 ACCUR MX
- Page 99 and 100: Definitions of variables 91 RPER co
- Page 101 and 102: Definitions of variables 93 WLEN Th
- Page 103 and 104: Appendix B Command syntax B.1 Comma
- Page 105 and 106: Repetitions of keywords and/or othe
- Page 107 and 108: Required data and optional data Com
- Page 109 and 110: Appendix C File swan.edt Below the
- Page 111 and 112: File swan.edt 103 ! | -> DEFault !
- Page 113 and 114: File swan.edt 105 ! FRAME ’sname
- Page 115 and 116: Appendix D Spectrum files, input an
- Page 117 and 118: 0.3892E-03 192.0 15.2 0.8007E-03 24
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Appendix A<br />
Definitions of variables<br />
In <strong>SWAN</strong> a number of variables are used in input and output. Most of them are related<br />
to waves. The definitions of these variables are mostly conventional.<br />
HSIGN<br />
Significant wave height, denoted as H s in meters, and defined as<br />
H s = 4√ ∫ ∫ E(ω,θ)dωdθ<br />
where E(ω,θ) is the variance density spectrum and ω is the absolute<br />
radian frequency determined by the Doppler shifted dispersion relation.<br />
However, for ease of computation, H s can be determined as follows:<br />
H s = 4√ ∫ ∫ E(σ,θ)dσdθ<br />
HSWELL<br />
Significant wave height associated with the low frequency part of<br />
the spectrum, denoted as H s,swell in meters, and defined as<br />
H s,swell = 4√ ∫ ωswell<br />
0<br />
∫ 2π<br />
0 E(ω,θ)dωdθ<br />
TMM10<br />
with ω swell = 2πf swell and f swell = 0.1 Hz by default (this can be changed<br />
with the command QUANTITY).<br />
Mean absolute wave period (in s) of E(ω,θ), defined as<br />
∫ ∫ ∫ ω<br />
T m−10 = 2π<br />
−1 E(ω,θ)dωdθ<br />
∫ ∫ ω<br />
E(ω,θ)dωdθ<br />
= 2π∫ −1 E(σ,θ)dσdθ<br />
∫ ∫ E(σ,θ)dσdθ<br />
TM01<br />
Mean absolute wave period (in s) of E(ω,θ), defined as<br />
(∫ ∫ ) −1 (∫ ∫ ) −1<br />
ωE(ω,θ)dωdθ<br />
T m01 = 2π ∫ ∫ ωE(σ,θ)dσdθ<br />
E(ω,θ)dωdθ<br />
= 2π ∫ ∫ E(σ,θ)dσdθ<br />
89