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Recent extensions of the COSMO TKE scheme related to the interaction with non turbulent scales. Separation between turbulence and non turbulent sub grid scale circulations. Additional scale interaction terms in the separated TKE budget. - PowerPoint PPT Presentation
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Matthias Raschendorfer
DWD
Recent extensions of the COSMO TKE scheme related to the interaction with non turbulent scales
COSMO Offenbach 2009Matthias Raschendorfer
Separation between turbulence and non turbulent sub grid scale circulations
Additional scale interaction terms in the separated TKE budget
Parameterization and effect of 3 important scale interaction terms with separated:- Horizontal shear modes (e.g. at frontal regions)- Wake modes from SSO blocking (over mountains)- Buoyancy forced thermal circulations (e.g. due to shallow convection or
sub grid scale katabatic flows) Considering of non turbulent sub grid scale circulations in the statistical
condensation scheme (including non Gaussian effects)
Turbulence closure is only valid for scales not larger than
- the smallest peak wave length Lp of inertial sub range spectra from samples in any direction, where - the largest (horizontal) dimension Dg of the control volume
Spectral separation by
- averaging these budgets along the whole control volume (double averaging)
Partial solution for turbulence by spectral separation:
Turbulence is that class of sub grid scale structures being in agreement with turbulence closure assumptions!
- considering budgets with respect to the separation scale
gp DLL ,min
generalized turbulent budgets including additional scale interaction terms
pp LL
COSMO Offenbach 2009Matthias Raschendorfer
LLLLLtD ˆˆ vv
LLL ˆˆ vv
average of the non linear turbulent shear terms
circulation shear term
Additional circulation terms in the turbulent 2-nd order budgets:
turbulent shear term
CS
ˆˆLLL vv
turbulent shear term
COSMO Offenbach 2009Matthias Raschendorfer
Physical meaning of the circulation term:
Budgets for the circulation structures:
LLLLLtD ˆ~ˆ~ vv
CS
Circulation term is the scale interaction term shifting Co-Variance (e.g. SKE) form the circulation part of the spectrum (CKE) to the turbulent part (TKE) by virtue of shear generated by the circulation flow patterns.
CKE TKE
production terms dependent on:
specific length scales and specific velocity scales (= )
production terms depend on:
the turbulent length scale and the turbulent velocity scale (= )CKE TKE
21
CL
CL
21
pL
pL
circulation-scale turbulence-scalestatistical moments
vvCS
COSMO Offenbach 2009Matthias Raschendorfer
and other and other
We need to consider additional length scales besides the turbulent length scale!
Separated semi parameterized TKE equation (neglecting molecular transport):
buoyancy production
eddy-dissipationrate (EDR)
0labil:neutral:stabil: 0
00
time tendency of TKE
transport of TKE
shear production by sub grid scale circulations
0
2
Lt q21
v2
Lq21
3
1iiLi vv ˆvLv
v
wg ̂
3
1iLiLi vv ˆv
MM
3
Lq
expressed by turbulent flux gradient solution
to be parameterized by a non turbulent approach
v
COSMO Offenbach 2009Matthias Raschendorfer
shear production by the mean flow
0
v
222
211
21221gHHSHSC vv2vvDqS :_
vv
Separated horizontal shear production term:
effective mixing length of diffusion by horizontal shear eddies
velocity scale of the separated horizontal shear mode
1H scaling parameter
Equilibrium of production and scale transfer towards turbulence:
gH
3HM
HgHH Dq
FDq
MHF:
1H scaling parameter
23
MH
2g
23
H21
HMHgHHSHSC FDFDqS vv
_2S:
horizontal shear eddyisotropic turbulence
z
x
y zvh
xvh
xvh
horizontal grid plane
TKE-production by separated horizontal shear modes:
zvh
grid scale
21
pL
gD
……….effective scaling parameter
separated horizontal shear
additional TKE source term
COSMO Offenbach 2009Matthias Raschendorfer
out_usa_shs_rlme_a_shsr_0.2
20
40
60
Pot. Temperature [K]
S N
06.02.2008 00UTC + 06h -92 E
out_usa_shs_rlme_a_shsr_1.0
COSMO Offenbach 2009Matthias Raschendorfer
= (dissipation)1/3
frontal zone
B
2iiiiiit sdnp
G1
pgvvvvvs
sv ˆˆˆˆ
SSO-term in filtered momentum budget:
Q
n
ivSSOQblocking term
SSO-term in SKE-equation:
2
1i
vSSOi
B
2h
hhhSSOC
iQvsdnpG
pS ˆˆ_
s
vv svv
hv
21x ,
3x
TKE-production by separated wake modes due to SSO:
Bseparated sub grid orography
currently Lott und Miller (1997)
COSMO Offenbach 2009Matthias Raschendorfer
moderate light
S N
06.02.2008 00UTC + 06h -77 E
mountain ridge
SSO-effect in TKE budget
out_usa_rlme_tkessoout_usa_rlme_sso
out_usa_rlme_tkesso – out_usa_rlme_ssoMIN = 0.00104324 MAX = 10.3641 AVE = 0.126079 SIG = 0.604423 MIN = 0. 00109619 MAX = 10.3689 AVE = 0.127089 SIG = 0.804444
MIN = -0.10315 MAX = 0.391851 AVE = 0.00100152 SIG = 0.00946089
COSMO Offenbach 2009Matthias Raschendorfer
= (dissipation)1/3
0FLwg
wg
S 23
H3patzvvC
vV
vSTHC
2
V LLLLL
ˆˆˆ
ˆˆ
_vv
virtual temperat. of ascending air
circulation scale temperature variance ~ circulation scale buoyant heat flux circulation term
A first parameterization of the thermal circulations term:
Circulation scale 2-nd order budgets with proper approximations valid for thermals:
pattern length scale
square for Brunt-Väisälä-frequency
separated thermals
Simplified max flux approach for the circulations:
virtual temperat. of descending air
COSMO Offenbach 2009Matthias Raschendorfer
bC
b2
1
Cv
vvCC H
Hgw expˆ
v
vv
vv
vvC q
gLw
ˆˆˆˆ
scaling factor circulation height: e.g. BL-height
bottom level
turbulent velocity scale
horizontal updraft scale
ahorizontal updraft fraction ww ˆ
TKE2q
vertical velocity scale of circulation
current formulation using an additional assumption about the gradient
v̂
Cvvvv H0 ˆ,ˆˆ,ˆ
Effect of the thermal circulation term for stabile stratification:
v̂
x
wv
0
x
ˆzturbv Kw
circv w
wg
uwuTKED vv
zt ˆ
0
• Even for vanishing mean wind and negative turbulent buoyancy there remains a positive definite source term
TKE will not vanish Solution even for strong stabilityCOSMO Offenbach 2009Matthias Raschendorfer
CH a a1
0
0
.const
CH
v
v
horizontal scale of a grid box
simulated midnight profile of potential temperature
measured midnight profile of potential temperature
COSMO Offenbach 2009Matthias Raschendorfer
x
vsqfrom normal distribution of turbulence
Convective modulation of turbulence in a statistical condensation scheme:
0
from bimodal distribution of convective circulation
cloud
turbulent Gaussian saturation adjustment using average oversaturation of upward flow
vsuq
turbulent Gaussian saturation adjustment using average oversaturation of downward flow
vsdq
vsuq
vsdq
a a1
vsgq
grid scale oversaturation vs
gq
vsd
vsu
vsg qa1qaq
,a ,vsuqto be estimated form
relevant 2nd order scheme describing convective circulations
total oversaturation
vsdq
COSMO Offenbach 2009Matthias Raschendorfer
2vsd
vsu
vsC qqa1aqVar
a1a
a21qSkew vsC
horizontal direction
derivable directly from proper mass flux scheme describing convective circulations
• 3D-shear terms have got a significant effect only, when formulated as a scale interaction term producing TKE by shear of a separated horizontal shear mode with its own length scale.
• Wake production of TKE by blocking can be formulated as a scale interaction term as well and can be described by scalar multiplication of the horizontal wind vector with its SS0-tendencies yielding some effect above mountainous terrain.
Conclusions:
Prospect:• We intent to implement the revised formulation of the circulation term together with the
“convective modulation” of the statistical cloud scheme and to derive a similar scale interaction term from the current convection scheme as well.
COSMO user seminar Offenbach: 09-11.03.2009Matthias Raschendorfer
• Non turbulent sub grid scale modes interact with turbulence through additional shear production in the TKE equation.
• Buoyancy forced (convective) circulations can be described either by a mass flux approach or 2-nd order closure. The according TKE production term is related to the circulation buoyancy heat flux.Interaction of those circulations with the statistical saturation adjustment (cloud scheme) can be formulated by “convective modulation”.
• Further we plan to consider the circulation scale fluxes in the 1-st order budgets leading to additional non local mixing tendencies of the prognostic variables.
Thank You for attention!
COSMO Offenbach 2009Matthias Raschendorfer
Matthias Raschendorfer
DWD
About the results of UTCS Tasks (ii)a,c and (iii)a
As far as attended by
COSMO Offenbach 2009Matthias Raschendorfer
3D-run
mesdat only with model variables
Forced correction run with SC version
outdat with correction integrals
Identical except horizontla operations and w-equation
mesdat containing geo.-wind, vert.-wind undtendencies for horizontal advektion
Realistic 3D-run (analysis)
Forced test run with SC version
outdat with similar results compared to compared test run using the 3D-model
Basic scheme of advanced SC-diagnostics:
COSMO Offenbach 2009Matthias Raschendorfer
or
Component testing:
outdat or mesdat may contain 3D-corrections and arbitrary measurements (like surface temperature or surface heat fluxes) the model can be forced by.
COSMO Offenbach 2009Matthias Raschendorfer
interpolated measurements
free model run starting wit 3D analysis
free model run starting with measurementsforced with prognostic variables from 3D-run
forced with 3D corrections
forced with 3D corrections and measured surface temperature
forced with 3D corrections and measured surface heat fluxes
Stable stratification over snow at Lindenberg
Potential temperature profile
atmosphere
soil
Potential temperature profile
atmosphere
soil
too much turbulent mixing
Turbulent fluxes of the non conservative model variables:
vcw
ccp
ww
2
1
qqq
qrTthermodynamic
non conservative model variables
mznmnmH
nzH
n cKKwf n ~~:
flux-gradient form explicit flux correction
cTcpTc
cTcpTc
cccTcTc
nm
rrrrrrr1rr1rrr
r1rrr1r1c
dp
d
cR
3phPa10
pTr
dp
cT
cL1
1r
:
vsTq :
dpp
cc cr
L :
cr cloud fraction
steepness of saturation humidity
Exner factor
Conversion matrix:
ˆzKww
c
v
3
2
1
thermodynamic conservative model variables
fg
cvz
vvz
czcz
z
qqqq
q
,ˆ,ˆ,ˆˆ
:~
Explicit moisture correction:
COSMO Offenbach 2009Matthias Raschendorfer
should vanish due to grid scale saturation adjustment!
COSMO Offenbach 2009Matthias Raschendorfer
But there are differences … … due do numerical effects with the Exner-factor treatment of the T-equation
Time series of model domain averages
less low level clouds
explicit TKE-diffusion with restriction proper for 50 layer configuration
SC simulations with 80 layers and “implicit TKE diffusion”:
numerically unstable!
COSMO Offenbach 2009Matthias Raschendorfer
Dew point profiles 50 layers
considerable difference
Dew point profiles 80 layers
implicit TKE-diffusion being unconditional stable
almost no difference