Transcript clws2 9127

Representing Diverse Scales in OLAM
Advantages and Challenges of Locally-Refined Unstructured Grids
Robert L. Walko
Rosenstiel School of Meteorology and Physical Oceanography
University of Miami, Miami, FL
Presented at IPAM, UCLA, April 16, 2010
Acknowledgments:
1) Roni Avissar – Dean of Rosenstiel School
2) Pratt School of Engineering, Duke University
3) NSF, NASA, DOE
4) William R. Cotton, Roger A. Pielke, Sr.
Outline:
1. Background and motivation for OLAM (the Ocean-Land-Atmosphere
Model)
2. Summary of OLAM dynamic core – local mesh refinement – some physics
3. Numerical experiments to examine how convection responds to variable
resolution
4. What the experiments tell us – some suggestions for future research
5. Summary
OLAM background

OLAM is based partly on RAMS, a limited area model specializing in
mesoscale and cloud scale simulations.

The original motivation for OLAM was to provide a unified global-regional
modeling framework in order to avoid the disadvantages of limited area
models.
External GCM domain
Traditional RCM
domain
Numerical noise at
lateral boundary
Information
flow
OLAM global lower resolution domain
OLAM local high
resolution region
Information
flow
Well behaved transition region

OLAM went through several versions, including overlapping polarstereographic projections, but eventually we settled on the geodesic mesh
because of its facility in local mesh refinement.

OLAM works with either triangles or hexagons as the primary mesh. With
hexagons, a few pentagons and heptagons are required for local mesh
refinement.

Physical parameterizations were adapted from RAMS, with others added
later.

OLAM’s dynamic core was a new formulation, not from RAMS.
Mass & Momentum conserving FV dynamic core

 

 

Vi
   viV  p  i  2    v i   g i  Fi
t
Momentum conservation
(component i)


   V  M
t
Total mass conservation

 (  )
   V  H
t

 
p   d Rd   v Rv  
CP
CV
 1 
 
 p0 
conservation
Rd
CV
Equation of State

(  s)
   s V  Q
t
Scalar conservation
(e.g. sv   v /  )
  d  v  c
Total density


V v
Momentum definition
 


qlat
   1 

C
max(
T
,
253
)


p
 = potential temperature
 = ice-liquid potential temperature
Integrate over finite volumes and
apply Gauss Divergence Theorem:






d




d






d

Discretized equations:
 

 



p
Vi d    viV  d  
d   2    v

t
xi



 d    V  d   Fm d

t
 





d




V

d

  F d


t
 




s
d



s
V

d

  Fs d


t

i
d    g i d   Fi d
Terrain-following coordinates
OLAM uses cut (“shaved”) grid cells
Anomalous vertical dispersion
Wind
Terrain-following coordinate levels
Terrain
Numerical experiments
Investigate behavior of parameterized and/or resolved
convection across grid scales.
We look only at accumulated surface precipitation at end of 6
hours.
Choose very simple horizontally-homogeneous forcing of
environment (no topography, no land/water, no large-scale flow
or disturbances).
Begin with horizontally-homogeneous, conditionally unstable
atmosphere at rest.
Impose constant surface sensible heat flux (~300 W m-2).
Grid number
1
2
3
4
5
6
7
Grid cell size
200 km
100
50
25
12
6
3
Cumulus parameterization only – no microphysics
Average parameterized convective precipitation over each refinement zone
We find that area-averaged parameterized precipitation is
insensitive to grid spacing for cells larger than about 30 km,
but increases (by about 50%) as cells reduce to 3 km.
We need to ask ourselves:
Do we want convective parameterization to give uniform
precipitation at all scales where it is applied?
Or not?
Is convective parameterization performing as intended, i.e.,
according to its design? In particular, is it responding correctly to
the host model’s ability (and tendency) to generate stronger W
on finer grids?
If we choose to take the “route 1” approach described by A.
Arakawa, can we adjust the fractional updraft area  in a way to
achieve the desired result?
Microphysics only – no cumulus parameterization
Average resolved convective precipitation over each refinement zone
Should the model even be allowed to produce convective-type vertical
motion on 6 km, 12 km, or larger cells? Such convection is unrealistically
wide, and is not well represented on the grid.
Perhaps a convective parameterization should be retained at these
resolutions to remove convective instability (the “route 1” approach)
Cumulus parameterization and microphysics together
Horizontally averaged combined precipitation
Horizontally-averaged parameterized convective precipitation
Obviously, in locations where convection is resolvable, we want resolved
convection to prevail and parameterized convection to become inactive.
This will not not happen unless parameterized convection is switched off
or is somehow supressed.
Can this transition be made smoothly?
Many more complicating factors need to be considered:
Ambient wind
Large-scale disturbances
Orographic lifting
High-CAPE convection (not generally permitted by
parameterized convection)
Can blending methods be made to work well for all situations?
Possible configuration for embedded “superparameterization” grid:
Inner cells fine enough to resolve primary updraft and rain-cooled downdraft
Overall cluster of cells wide enough to encompass mesoscale subsidence
Achieves both goals with fewer cells than uniform embedded grid
Motion of convection grid
Summary:
Local mesh refinement within a single model framework enables
numerical experiments that examine how a model represents
parameterized and resolved convection:
1) at different scales
2) where grid scale changes
OLAM has the appropriate tools for this investigation, including extensions
for topographic, land/sea, and realistic large-scale forcing
Both “route 1” and “route 2” approaches are being investigated.