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Phenomenology, Simulation and Parameterization of Atmospheric Convection Pier Siebesma Yesterday: “Dry” Atmospheric Convection Today: “Moist” Convection and (shallow cumulus) clouds Dry Convection 1

1.

Motivation 2. Equations 3. Moist Thermodynamics Concepts 4. LES of shallow cumulus convection 5. Parameterization of cumulus convection 6. Geometry of Cumulus Clouds 7. (PDF cloud schemes) Dry Convection 2

Tropopause 10km Subsidence ~0.5 cm /s 10 m/s Cloud base ~500m Equator 0 o

•Deep Convective Clouds •Precipitation •Vertical turbulent transport • Net latent heat production •Engine Hadley Circulation

inversion E v Trade wind region E v

•Shallow Convective Clouds •Little precipitation •Vertical turbulent transport •No net latent heat production •Fuel Supply Hadley Circulation

North 30 o N

•Stratocumulus •Interaction with radiation

EUROCS intercomparison project on cloud representation in GCM’s in the Eastern Pacific Large Scale Models tend to overestimate Tradewind cumulus cloudiness and underestimate Stratocumulus

Deep cu Shallow cu scu

Siebesma et al. (2005, QJRMS)

1. Motivation 2. Equations 3. Moist Thermodynamics Concepts 4. LES of shallow cumulus convection 5. Parameterization of cumulus convection 6. Geometry of Clouds 7. (PDF cloud schemes) Dry Convection 5

Grid Averaged Equations of thermodynamic variables

  

t

 

q v

t

q l

t

  

v

   

v

 

q v

v

 

q l

  

w

  

z w

q v

z w

q l

z

    

x i u i

     

x i

x i u i

q v

u i

q l

  

L

c p

c

e

 

c

e

  

c

e

  

Q rad P r

Large scale advection Large scale subsidence turbulent transport Net Condensation Rate

Introduce moist conserved variables!

l

  

L c p

q l q t

q v

q l

Liquid water potential Temperature

Total water specific humidity

  

t l

q t

t

  

v

  

l

v

 

q t

 

w w

  

z l

q t

z

    

z

z w

 

w

q t

l

  

Q rad P r

What happened with the clouds?

Buoyancy is the primary source for the vertical velocity

w

t

  

g

0  

v

With:

v

  ( 1  0 .

61

q v

q l

)  

v

    1 .

61  

q v

  

q l

Typical numbers:



= 0.5K

q v = 1~5 g/kg

q l = 0~3 g/kg

 0 .

5

K

 0 ~ 3

K

 0 ~ 1

K

So we need to go back to “down to earth” variables:

{

q l a c

 0 ,  0 ,

Cloud Scheme in LES: All or Nothing

if q t

q sl

 0 {

q l a c

 1 ,   (

q t

q sl

),

if q t

q sl

 0 In Climate models we have partial cloud cover so we need a parameterization.

1. Motivation 2. Equations 3.

Moist Thermodynamics Concepts 4. LES of shallow cumulus convection 5. Parameterization of cumulus convection 6. Geometry of Clouds 7. (PDF cloud schemes) Dry Convection 10

Conditional Instability

Lift a (un)saturated parcel from a sounding at z0 by dz

Check on buoyancy with respect to the sounding:

B

g

 0  

v

,

p

 

v

profile

d

z unstable

v

m

5.4K/km

stable Stable for unsaturated parcels Unstable for saturated parcels Conditionally Unstable!!!

d

   

z v

 

m

CAPE CIN

Introductory Concepts 1:

CAPE

CAPE = Convective Available Potential Energy.

CIN = Convection Inhibition •

CAPE and CIN unique properties of moist convection

Primary Reason why moist convection is so intermittant

Free Energy CAPE and CIN: An Analogue with Chemistry Surf Flux Mixed Layer Activation (triggering) CIN CAPE LFC Parcel Height LS-forcing RAD LS-forcing LNB 1) Large Scale Forcing :

Horizontal Advection

Vertical Advection (subs)

Radiation 2) Large Scale Forcing: slowly builds up CAPE 3) CAPE

Consumed by moist convection

Transformed in Kinetic Energy

Heating due to latent heat release (as measured by the precipitation)

Fast Process!!

Free after Brian Mapes

Introductory Concepts 3:

Quasi-Equilibrium

(Arakawa and Schubert JAS 1974)

dCAPE

dt JM b

F LS

 0

LS-Forcing that slowly builds up slowly The convective process that stabilizes environment Quasi-equilibrium: near-balance is maintained even when F is varying with time, i.e. cloud ensemble follows the Forcing.

Forfilled if :

t

adj <<

t

F w u a u Used convection closure (explicit or implicit) JM b

t

adj ~ CAPE/

t

adj : hours to a day.

M b =a u w u

r :

Amount of convective vertical motion at cloud base (in an ensemble sense)

Introductory Concepts 4:

Earthly Analogue

Free after Dave Randall:

Think of CAPE as the length of the grass

Forcing as an irrigation system

Convective clouds as sheep

Quasi-equilibrium: Sheep eat grass and no matter how quickly it grows, the grass is allways short.

Precipitation………..

1. Motivation 2. Equations 3. Moist Thermodynamics Concepts 4.

LES of shallow cumulus convection 5. Parameterization of cumulus convection 6. Geometry of Clouds 7. (PDF cloud schemes) Dry Convection 16

History of LES of cumulus topped PBL

1.

2.

3.

4.

5.

6.

7.

Sommeria, G. (1976) J. Atm Sci. 33, 216-241 Sommeria, G and Lemone, M.A (1978) J. Atm Sci. 35, 25-39 Beniston, M.G. and Sommeria G (1981) J. Atm Sci. 38, 780-797 Bougeault, Ph (1981) J. Atm Sci. 38, 2414-1438 Nicholls, L, Lemone, M.A. and Sommeria, G. (1982) QJRMS 108, 167-190 Cuijpers J,W,M and Duynkerke, P.G, (1993) J. Atm Sci. 50, 2894-3908 Siebesma and Cuijpers J,W,M (1995) J. Atm Sci. 52, 650-666 GCSS; LES intercomparison studies of shallow cumulus:

Experiment BOMEX Case Steady state Trade wind cu year 1997

Siebesma et al. JAS 2003

ATEX Trade wind cu topped with Scu 1998

Stevens et al. JAS 2001

ARM RICO Diurnal Cycle Cumulus Precipitating trade wind cu 2000 2006

Brown et al. QJRMS 2002 Van Zanten et al. in preperation

No observations of turbulent fluxes.

Use Large Eddy Simulation (LES) based on observations BOMEX ship array (1969)

  

t

      

t

   large scale       

t

   LES  0

observed observed To be modeled by LES Nitta and Esbensen 1974 JAS

11 different LES models

Initial profiles

Large scale forcings prescribed

6 hours of simulation Is LES capable of reproducing the steady state?

Large Scale Forcings

Mean profiles after 6 hours

Use the last 4 simulation hours for analysis of …….

Turbulent Fluxes of the conserved variables qt and

l

w

 

l

 

w

   

L c p w

q l

w

q t

 

w

q v

Cloud layer looks like a enormous entrainment layer!!

w

q l

LES: “clouds in silico” Convective Mass flux decreasing with height

mass flux = cloud core fraction * core velocity

Siebesma et al JAS 2003

x x =

Recently validated for “Clouds in vivo” (Zhang, Klein and Kollias 2009) clouds “in vivo”

ARM mm-cloud radar Updraft mass flux = updraft fraction * updraft velocity

Conditional Sampling of:

Total water qt

Liquid water potential temperature

l

Lateral Mixing between clouds and environment

1. Motivation 2. Equations 3. Moist Thermodynamics Concepts 4. LES of shallow cumulus convection 5.

Parameterization of cumulus convection 6. Geometry of Clouds 7. (PDF cloud schemes) Dry Convection 26

Mass Flux decomposition

a 

u

 

u

  

u u

e

 

e

  

e e

 

a

u u

 ( 1 

a

) 

e e

Courtesy : Martin Kohler (ECMWF)

M

w

   

a w

  

u u

 ( 1 

a

)

w

  

e e

a w u

( 

u

  ) sub-core flux env. flux Siebesma and Cuijpers JAS (1995) M-flux

In general: bulk approach:

Cloud ensemble:

approximated by

1 effective cloud:

How to estimate updraft fields and mass flux?

The old working horse: Entraining plume model:

1

M

1 2   

z c

M

z

w c

2 

z

   ( 

c

     

b

   ) for     l ,

q t

w c

2 

aB

,

B

g

 0  

v

 

v

Betts Arakawa&Schubert Tiedtke Gregory & Rowntree Kain & Fritsch And many more……..

1974 JAS 1974 JAS 1988 MWR 1990 MWR 1990 JAS

M

Plus boundary conditions at cloud base.

Different tendency to form cumulus anvils is caused by differences in the vertical structure of model mass flux: 

,

values fixed Mixing; Flexible structure M

Tiedtke (1989) in IFS EDMF-DualM

M Siebesma et al 2007 (JAS) Neggers et al 2009 (JAS)

Standard (schizophrenic) parameterization approach:

w

    

K

  

z w

   

M

( 

u

  )   

t

   

z

S

This unwanted situation has led to:

Double counting of processes

Problems with transitions between different regimes: dry pbl

shallow cu scu

shallow cu shallow cu

deep cu

Deterministic versus Stochastic Convection (1) •

Traditionally convection parameterizations are deterministic:

Instantaneous large scale Forcing and mean state is taken as input and convective response is deterministic

One to one correspondency between sub-grid state and resolved state assumed.

Conceptually assumes that spatial average is a good proxy for the ensemble mean.

~500 km

Deterministic versus Stochastic Convection (2) •

However: Cloud Resolving Models (CRM’s) indicate that operational resolutions show considerable fluctuations of convective response around the ensemble mean.

This suggests that a deterministic (micro-canonical) approach might be too restricitive for most operational resolutions.

pdf Mass Flux

Plant and Craig 2006 JAS

More Sophisticated Parameterization (2) (Plant and Craig 2007)

Parameterization:

Select N cloud updrafts stochastically according to the pdf

Calculate impact for each updraft by using a cloud updraft model

Note : N is a function of the resolution

Only tested in 1D setting

1. Motivation 2. Equations 3. Moist Thermodynamics Concepts 4. LES of shallow cumulus convection 5. Parameterization of cumulus convection 6.

Geometry of Clouds 7. (PDF cloud schemes) Dry Convection 35

Is this a Cloud??

….and, how to answer this question?

Fractal Geometry

 “Shapes, which are not fractal, are the exception. I love Euclidean geometry, but it is quite clear that it does not give a reasonable presentation of the world. Mountains are not cones, Euclidean”. clouds are not spheres , trees are not cylinders, neither does lightning travel in a straight line. Almost everything around us is non Benoit Mandelbrot

Instead of

Area-Perimeter analyses of cloud patterns (1) Procedure:

•Measure the projected cloud area A p and the perimeter L p of each cloud •Define a linear size through

l

A p

• Perimeter dimension define through:

L p

l D p

For “ordinary” Euclidean objects:

log

L p

Slope: D p = 1 log

l

Area-Perimeter analyses of cloud patterns (2)

Pioneered by Lovejoy (Science 1982)

Area-perimeter analyses of projected cloud patterns using satellite and radar data

Suggest a perimeter dimension Dp=4/3 of projected clouds!!!!!

Confirmed in many other studies since then… Instead of Consequences:

Cloud perimeter is fractal and hence self-similar in a non-trivial way.

Makes it possible to ascribe a (quantitative) number that characterizes the structure

Provides a critical test for the realism of the geometrical shape of the LES simulated clouds!!!!

Slope 4/3

Similar analysis with LES clouds

• •

l

V

1

/

3 •

Plot in a log-log plot

S

(

l

) 

l D s

Assuming isotropy, observations would suggest Ds=Dp+1=7/3

Siebesma and Jonker Phys. Rev Letters (2000)

Result of one cloud field

Repeat over 6000 clouds

Some Direct Consequences Surface area can be written as a function of resolution (measuring stick)

l :

S

(

l

) 

S L l L

2 

D s

,  

l

L D s

 7 / 3

S L

L

measured with L.

Euclidian area SL underestimates true cloud surface area S(l=

) by a factor

 

L

 2 

D s

 100 •

LES model resolution of l=50m underestimates cloud surface area still by a factor 5!!!

Does this have consequences for the mixing between clouds and the environment???

l

0

T

(

l

0

) Transport = Contact area x Flux

S

(

l

0

)

F

(

l

0

)

 

S

(

l

0

)

K

(

l

0

)

c

x

turbulence diffusive flux

resolved advection

S

(

l

0

)

Subgrid diffusion

K

(

l

0

)

c

x

Consequences for transport over cloud boundary (2)

T

(

l

0

)

S

(

l

0

)

F

(

l

0

)

 

S

(

l

0

)

K

(

l

0

)

c l

0

S

(

l

0

)

S L l

0

L

2 

D s K

(

l

0

)

l

0 

u

(

l

0

)

l

0 

u

(

L

)

l

0

L

(Richardson Law) 1

/

3

T

(

l

0

)

 

c

u

(

L

)

S

(

L

)

 

l

0

L

  7

/

3 

D s !

!

!

!

!

No resolution dependancy for Ds=7/3!!

Is this shear luck ????

Not really: Repeat the previous arguments for

l

0  

T

(  )  

c

u

(

L

)

S

(

L

 )  

L

7

/

3 

D s

 Re 3/4  7/3 D s 

Boundary flux T only Reynolds independent if

D s

 7 / 3

which completes a heuristic “proof” why clouds are fractal with a surface dimension of 7/3.

Gradient Percolation Dp=4/3 A stronger underlying mechanism ? (Peters et al JAS 2009) Dry Convection 47

high

Conceptual models Statistical Mechanics Self-Organised Criticality

Level of “understanding ” or conceptualisation low

Direct Interface & microphysical models Numerical Simulati on Large Eddy Simulations Mixed layer models Models/Parameterizations Global Climate Simulations Simulations Laboratory experiments

High

Atmospheric Profiling stations Field campaigns resolution Scale Hierarchy Satellite data Observations

Low