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%Yannis Cuypers LOCEAN Sorbonne Université 07/2022
computes the vertical oceanic baroclinic modes with background currents U and
startification Nsq (extends dynmodes https://github.com/sea-mat/dynmodes by J. Klinck to the presence of background current). Dynmodes (included in the package is used to get a first guess of the mode phase speed.
Function call:
[Wmod,Pmod,c]=dynmodesShear(Nsq,U,p,nmode)
Nsq (rad/s)^2 and U(m/s) are vectors varying with depth/pressure
(same size as p), p vector of pressure in dbar
nmode= mode number
Wmod,Pmod vertical mode strcture for pressure (Horizontal velocity) and vertical velocity
and phase speed c for the mode nmode
based on Thompson Haskell computation as described in Shi and Fan 2009 DOI: 10.1016/S1001-6058(08)60159-6
Note that there is a typo in Shi and Fan 2009 matrix Eq.16 should be +fp in the exponentials
note that phase speed c is considered positive so that U sign should be
defined with c direction as a reference
Computation will not work for critical or spupercritical condition (U
overocomes c at any depth)
Citar como
Yannis Cuypers (2026). DynmodesShear (https://es.mathworks.com/matlabcentral/fileexchange/115995-dynmodesshear), MATLAB Central File Exchange. Recuperado .
Información general
- Versión 1.0.1 (5,09 KB)
Compatibilidad con la versión de MATLAB
- Compatible con cualquier versión
Compatibilidad con las plataformas
- Windows
- macOS
- Linux
