Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

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What’s quasi-equilibrium What’s quasi-equilibrium all about? all about? Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Transcript of Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Page 1: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

What’s quasi-equilibrium all What’s quasi-equilibrium all about?about?

What’s quasi-equilibrium all What’s quasi-equilibrium all about?about?

Laura Davies, University of Reading, UK.

Supervisors:Bob Plant, Steve Derbyshire (Met Office)

Page 2: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Why is convection important?

Major transport of heat, moisture and momentum.

Focus on deep convection

Fair weather cumulus

Cumulonimbus

Focus on this!

Page 3: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Develop on organised, long-lived systems such as squall lines and MCSs.

What is deep convection?

Page 4: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Provide energy to large-scale circulations eg Hadley cell.

Convection interacts and modulates MJO.

What is deep convection?

Page 5: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

E

ffect

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What is deep convection?

Page 6: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Convection meets NWP Convective systems are a major contributor to global

circulations of heat, mass and momentum Representation depends on scale of model

High resolution models explicitly resolve clouds

Large scale models require parameterisation Parameterisations represent the mean effect of the

sub-grid scale cloud process on the large scale flow

For validity this requires assumptions to be made about the mean convection

Page 7: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Parameterisation basicsArakawa and Schubert (1974)

adj ls Key assumption

Page 8: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Scale separation in time and space between cloud processes and large scale flow

Convection acts on smaller and faster scales than the large scale flow

AV

HR

R v

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Convective ensemble

Analogous to the equation of state

p=ρRT

The assumptions

Page 9: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

MotivationModel compared to observations (Yang & Slingo 2001)

Longer systematic life cycle…memory?

Page 10: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

LEM run as a CRM explicitly resolves cloud-scale dynamics but parameterises sub-grid processes

Largest eddies are responsible for majority of transport so are explicitly resolved

Large eddy models setup

Vary the lengthof the cycle

Initialised with profiles of θ and qv

Non-rotating, no wind shear 1 km resolution Balanced in terms of

moist static energy

Page 11: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Control run

Time-varying portion of run

Initial convective response is strongly influenced by the control run. It was found a portion of ~ 6hrs need to be removed. This suggests ‘memory’ within the system.

Control run:Applying constant surface fluxes until equilibrium achieved

A long time Repeating 3hr cycles

Page 12: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Equilibrium response

Decay consistent with forcing

Fluctuations around an equilibrium mass flux

Rapid triggering but variable magnitude and timing

Long timescale - 36 hrs

Page 13: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Non-equilibrium responseShort timescale - 3 hr

All times show convective activity

Gradual triggering

Peak response highly variable cycle-to-cycle

Page 14: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Increased variability in mass flux response

Effect of forcing timescale

Similar response for precipitation.Increased variability in mean totalprecipitation per cycle.

Page 15: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Control run

Page 16: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Diurnal cycle depends on… Localised solar heating due to surface Sea-breezes Cold pools and gust fronts Dry lines Horizontal convective rolls

Khairoutdinov and Randell (2006)

Earlier rain events Land use Soil moisture Cold pools in boundary layer Humidity of free troposphere

Stirling and Petch(2004)

Page 17: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Perturb key thermodynamic variables by damping them back to the horizontal mean

Damp on the convective timescale ~ 15 mins Investigate effect on variability in 3 hr run

Experimental set up

Horizontal winds, u, v Vertical wind, w

Variables to damp

Moisture, qv

Temperature, θ

Page 18: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Damping u, v

Reduced precipitation Increased precipitation

Damping u, v reduces the variability in the precipitation where the variability was stronger.

It increases the variability where it was weaker.

Page 19: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Vertical profile of horizontal wind speed

X-section of horizontalwind speed (m/s)

At surface At top of boundary layer(925 m)

Dam

ped

u, v

Non

-dam

ped

At time of maximumforcing

Page 20: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Damping θ

Includes 1st 12 cycles

Page 21: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Damped θ Non-dampedN

ear

star

t of

dam

ping

Tow

ards

end

of

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ion

X-section θ’2 (K2) at 3 km At time of maximum forcing

Page 22: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Cloud distribution

Increasing height

Increasing height

Clouds defined as buoyant, moist and upward moving

Mean number of clouds

Damped θNon-damped

2.4 km

12.4 km

Page 23: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Conclusions Including convective parameterisations in numerical

models is essential. However results suggest that making an equilibrium

assumption might not always be valid. At short forcing timescales the convection is not a

direct function of the forcing. The time-history of the system affects the current

amount of convection. The system has an element of memory.

Experiments are starting to consider what variables may cause this memory.

u, v and θ are initial suggestions but experiments need to be carefully constructed.

Page 24: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)

Discussion points How do we make a parameterisation that works for all

forcing timescales eg. What key variables provide the memory in the

convective system? At what height do they have greatest effect? Is their spatial variability also a key factor?

adj ls

Page 25: Laura Davies, University of Reading, UK. Supervisors: Bob Plant, Steve Derbyshire (Met Office)