Difference between revisions of "SoulsbyKH"
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<div class="title">Methods for Calculating ''kh''</div> | <div class="title">Methods for Calculating ''kh''</div> | ||
The dispersion equation for surface gravity waves is <math>\omega^2 = gk~ \text{tanh}(kh)</math>, where <math>\omega</math> is the angular frequency of the wave (<math>2\pi/T</math>) where <math>T</math> is period (s), <math>g</math> is gravitational acceleration (m2 s-1), <math>h</math> is water depth (m), and <math>k</math> is wavenumber (<math>2\pi/\lambda</math>) where <math>\lambda</math> is wavelength (m). <math>k</math> is difficult to calculate because it is implicit.[[Bibliography#WibergP_2008a | Wiberg and Sherwood (2008)]] reported on the speed and accuracy of several explicit and iterative methods for approximating <math>kh</math>. Two good methods are implemented in ROMS/CSTMS. | |||
A fifth-order polynomial approximation attributed to Hunt (1979) by [[Bibliography#DeanR_1991a | Dean and Dalrymple (1991), p72]] is used when SSW_HUNT_KH is defined, and the Newton-Raphson method suggested by [[Bibliography#SoulsbyR_2005a | Soulsby (2005)]] is used when SSW_SOULSBY_KH is defined. | A fifth-order polynomial approximation attributed to Hunt (1979) by [[Bibliography#DeanR_1991a | Dean and Dalrymple (1991), p72]] is used when SSW_HUNT_KH is defined, and the Newton-Raphson method suggested by [[Bibliography#SoulsbyR_2005a | Soulsby (2005)]] is used when SSW_SOULSBY_KH is defined. | ||
{{warning}} '''Note:''' The Soulsby option and these two CPP defs are only implemented in the version of SSW_BBL.h located in [https://www.myroms.org/projects/cstm/browser/branches/crs/cstm_trunk Sherwood's branch]. | {{warning}} '''Note:''' The Soulsby option and these two CPP defs are only implemented in the version of SSW_BBL.h located in [https://www.myroms.org/projects/cstm/browser/branches/crs/cstm_trunk Sherwood's branch]. Define one of these two options: | ||
<div class="box">#define SSW_SOULSBY_KH<br />#undef SSW_HUNT_KH</div | <div class="box">#define SSW_SOULSBY_KH<br />#undef SSW_HUNT_KH</div> | ||
Latest revision as of 11:58, 18 May 2016
The dispersion equation for surface gravity waves is , where is the angular frequency of the wave () where is period (s), is gravitational acceleration (m2 s-1), is water depth (m), and is wavenumber () where is wavelength (m). is difficult to calculate because it is implicit. Wiberg and Sherwood (2008) reported on the speed and accuracy of several explicit and iterative methods for approximating . Two good methods are implemented in ROMS/CSTMS.
A fifth-order polynomial approximation attributed to Hunt (1979) by Dean and Dalrymple (1991), p72 is used when SSW_HUNT_KH is defined, and the Newton-Raphson method suggested by Soulsby (2005) is used when SSW_SOULSBY_KH is defined.
Note: The Soulsby option and these two CPP defs are only implemented in the version of SSW_BBL.h located in Sherwood's branch. Define one of these two options:
#undef SSW_HUNT_KH
