Vertical Terrain-Following Coordinates
From the point of view of the computational model, it is highly
convenient to introduce a stretched vertical coordinate system which
essentially "flattens out" the variable bottom at
.
Such "
" coordinate systems have long been used, with slight
appropriate modification, in both meteorology and oceanography
[e.g., Phillips (1957) and Freeman et al. (1972)].
To proceed, we make the coordinate transformation:





See S-coordinate for the form of
used here.
In the stretched system, the vertical coordinate
spans the
range
; we are therefore left with
level upper (
) and lower (
) bounding
surfaces. The chain rules for this transformation are:



where

As a trade-off for this geometric
simplification, the dynamic equations become somewhat more
complicated. The resulting dynamic equations are, after dropping the
carats:







where


The vertical velocity in
coordinates is
![{\displaystyle \Omega (x,y,s,t)={1 \over H_{z}}\left[w-(1+s){\partial \zeta \over \partial t}-u{\partial z \over \partial x}-v{\partial z \over \partial y}\right]}](https://www.myroms.org/www.myroms.org/v1/media/math/render/svg/351b2674c8914d5ba96e99e20c97cb7e7cb8e861)
and

Vertical Boundary Conditions
In the stretched coordinate system, the vertical boundary conditions
become:
top (
):





and bottom (
):





Note the simplification of the boundary conditions on vertical
velocity that arises from the
coordinate transformation.