Vertical velocity
RUC13 update (The RUC vertical motion is
at a given time step and is not time-averaged.)
The RUC vertical velocity (omega = dp/dt) is
diagnosed in the RUC model and is not a part of the RUC pronostic
equation set. It is calculated from 3 terms: 1) vertical motion
through coordinate surfaces, 2) vertical motion of the
coordinate surfaces, and 3) vertical motion along the
coordinate surfaces. See
Benjamin et al. (2004 - MWR - RUC model)
- see p.15
for more information and the omega equation used
in section 4.c. Note -- since omega (dp/dt) is relative to
pressure, a positive value (increasing pressure) means decreasing
height and a negative valud (decreasing pressure) means upward
vertical motion with respect to height.
RUC13 fix - The effects of diabatic heating in term 1 above
were exaggerated in previous versions before the RUC13.
This is now corrected.
[Following is a write-up from 1998
on RUC vertical motion, but
first read information above and Benjamin et al. 2004-MWR paper.]
The vertical motion, -omega, positive upward,
in the hybrid-coordinate RUC model
is diagnosed , using the formula
-omega = -Dp/Dt = -[(partial p/partial t)_s +
(vector V_H dot del_s) p + sdot*(partial p / partial s)],
where p is pressure, V_H is the horizontal velocity vector, del_s is the
gradient operator on a hybrid coordinate surface sdot is,s the rate at
which air parcels are moving vertically with respect to the hybrid coordinate, s,
which increases vertically, and (partial p / partial s) expresses the decrease
in pressure with increasing s.
Omega is not actually needed to solve the
RUC's model governing equations. It is, instead, a diagnosed quantity that
is provided to see the effective vertical motion in the RUC model.
The three terms of the omega equation correspond to:
- Motion through coordinate surfaces. This term is quite large
on sigma levels, but zero on isentropic levels except in the event
of diabatic processes (e.g., latent heat release, evaporation, radiational
heating/cooling).
- Local movement of the surfaces. For isentropic surfaces, this can be
considerable and corresponds roughly to the phase speed of the entire weather
system. For sigma levels, it is negligible.
- Upslope/downslope motion of the horizontal wind on the coordinate
surfaces.
This is the classical upglide/downglide term that makes it easy to see
vertical motion on isentropic coordinates. In sigma coordintes, it corresponds
primarily to terrain-forced motion.
The first two terms on the right-hand side of this equation
describe mathematically the change of pressure
a hypothetical air parcel would experience if it traveled along a coordinate
surface with the horizontal wind velocity on that surface. The last term
describes the change in pressure that results from air parcels moving
through coordinate surfaces. This last term will tend to be large only
in regions of strong latent heating particularly in the isentropic portion of
the model domain. The first two terms, however, can
be large in regions where winds are strong and where the coordinate
surfaces are sloped, as just above mountain ranges in the sigma
part of the vertical domain, or where isentropic "upglide" or descent is
occurring.
In mountain wave situations, isentropes themselves tend to follow the
terrain, espcially close to the surface. Higher up, they can be very
steeply sloped, even more so than the (smoothed) terrain.
An important factor to bear in mind when considering model-produced vertical
motion concerns a fundamental aspect of flow
patterns in the middle latitudes. That is, above the planetary
boundary layer,
the Coriolis force and the
horizontal component of the pressure-gradient force tend to be in balance
in synoptic-scale weather systems. This means that the horizontal winds
tend to be approximately geostrophic and that the typical relative vorticity
of these winds is typically much larger in magnitude
than their horizontal divergence.
As a result, vertical motions in synoptic-scale systems are usually small,
particularly outside areas of heavy precipitation.
However, for smaller, more rapidly changing mesoscale motion fields, this
constraint toward geostrophic balance imposed by the earth's rotation is
less strong, and divergence and vorticity will often have about the same
magnitude. With stronger divergence, vertical motions are typically also
stronger for mesoscale motions.
PBL depth
- Using vertical profile of virtual potential temperature from RUC
native levels, find height above surface at which
theta-v (virtual potential temperature) again exceeds theta-v at
surface (lowest native
level - 5 m above surface). Distance above surface.
gust wind speed
- Within PBL depth, calculate excess of
wind speed
over surface speed at each level. Multiply this excess by a
coefficient (f(z)) that decreases with height from 1.0 to 0.5 at 1 km height,
and is 0.5 for any height > 1 km. Add the maximum weighted wind excess
back to the surface wind. [gust = vsfc + max (f(z)*(v(k)-vsfc) ]
cloud base height
- Lowest level at which combined cloud and ice mixing
ratio exceeds 10**-6 g/g. Units - meters above sea level.
Horizontal grid points without any cloud layer are
indicated with -99999.
cloud top height
- Top level at which combined cloud and ice mixing
ratio exceeds 10**-6 g/g. Units - meters above sea level.
Horizontal grid points without any cloud layer are
indicated with -99999.
cloud fraction
- (available in BUFR only)
In the RUC, this is either 0 or 100% since non-zero cloud
hydrometeor mixing ratios can only occur if the grid volume
is saturated.
(This characteristic is also found with
MM5 and some physics packages with WRF.
The RUC the NCAR/Thompson mixed-phase cloud microphysics.)
In the RUC,
if there are any levels from the native grids with
cloud water or ice mixing ratio > 10**-6 g/g, then the cloud
fraction is set as 100% and 0% otherwise.
This approach is different from the Eta model, where
saturation exists at < 100% RH and the cloud fraction
varies continuously from 0 to 100% based on a function
of RH.
Cloud layers in the RUC are defined as follows:
- low - lowest 10 native levels (approximately lowest
50-75 hPa)
- middle - above lowest 10 native levels and below
400 hPa level
- high - above 400 hPa level