© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 1 Met Office Unified Model Terry Davies Dynamics Research
Jan 14, 2016
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 1
Met Office Unified Model
Terry Davies
Dynamics Research
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 2
UM Dynamical Core
Non-hydrostatic formulation Hybrid-height co-ordinate Semi-Lagrangian advectionSemi-implicit predictor-corrector integrationC grid horizontal staggeringCharney- Phillips vertical staggering
Davies, Cullen, Malcolm, Mawson, Staniforth
White, Wood 2005 Quart. Journal Roy. Met. Soc
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 3
Vertical and Horizontal Grid Staggering
Horizontal staggering - Awakawa c-grid
No grid decoupling
Better geostrophic adjustment for wavelengths of grid size less than Rossby radius of deformation
Vertical staggering - Charney-Phillips
No computational modes
More consistent with thermal wind balance
Can have complications in coupling with boundary layer parametrization
W,
U,ρ
W,
Ui- 2
1 ,j
2
1Vi,j+
2
1Vi,j-
Ui+
2
1 ,ji,j
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 5
Physical Parametrizations
Edwards-Slingo Radiation (Edwards & Slingo 1996)
Mixed phase precipitation (Wilson & Ballard 1999)
New Boundary Layer + 38L (Lock et al 2000)
New GWD scheme + GLOBE orography
smoothed (Raymond filter)
Modern spectral database for gaseous absorption in the atmosphere + new H2O continuum -
flexible configuration Multiple scattering included Better optical properties for
clouds inc. non-spherical ice parametrisation
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 6
Physical Parametrizations
Edwards-Slingo Radiation (Edwards & Slingo 1996)
Mixed phase precipitation (Wilson & Ballard 1999)
New Boundary Layer + 38L (Lock et al 2000)
New GWD scheme + GLOBE orography
smoothed (Raymond filter)
Physically based transitions between vapour, liquid, ice and rain
Ice content now a prognostic variable rather than diagnosed from cloud scheme
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 7
Physical Parametrizations
Edwards-Slingo Radiation (Edwards & Slingo 1996)
Mixed phase precipitation (Wilson & Ballard 1999)
New Boundary Layer + 38L (Lock et al 2000)
New GWD scheme + GLOBE orography
smoothed (Raymond filter)
Allows for non-local mixing in unstable regimes
Scheme diagnoses 6 different mixing regimes in order to represent stable, well mixed and cumulus processes
Scheme includes boundary layer top entrainment parametrisation
Improved interaction with the convection scheme
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 8
Physical Parametrizations
Edwards-Slingo Radiation (Edwards & Slingo 1996)
Mixed phase precipitation (Wilson & Ballard 1999)
New Boundary Layer + 38L (Lock et al 2000)
New GWD scheme + GLOBE orography
smoothed (Raymond filter)
Simplified scheme Expression for linear 2D flow
used to calculate total surface pressure drag
Gravity wave amplitudes proportional to depth of sub-grid mountains above blocked layer
Remainder of drag is attributed to flow blocking
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 9
Future Developments
Dynamical core improvements
More consistent treatment of moisture
Conserving semi-Lagrangian advection scheme
Variable resolution grid
Resolution increases - (70 levels, 40km)
New physical Parametrisations
New prognostic cloud scheme
New convection scheme
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 10
UM Operational Configurations
Global 40 kmN320L50640x481x50 63 km top150 million numbers
North Atlantic & European 12 km720x432x38 38 km top120 million numbers
Old UK 12 kmRetiring eventually
New UK 4 km288x320x38 38 km top35 million numbers
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 11
MOGREPSMet Office Global and Regional Ensemble
Prediction System
Ken Mylne
Ensemble Forecasting Manager
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 12
ECMWF Ensemble (EPS)
51 members Control (unperturbed) + 25 pairs formed by adding
and subtracting a perturbation TL255 Resolution (approx 80km) Designed for use beyond 48h Perturbations are linear combinations of
Forward and Evolved Singular Vectors Includes Stochastic Perturbations to model
physics
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 13
MOGREPS – The Met Office short-range ensemble
NAE
MOGREPS is on Operational Trial for 1 year from September 2005
Ensemble designed for short-range forecastingGlobal ensemble (~90km resolution, 38 levels)ETKF used within global ensemble to determine initial condition pertsRegional ensemble over N. Atlantic and Europe (NAE) at 24km resolution, 38 levels. Nested within global ensemble for initial and lateral boundary conditionsStochastic physicsT+72 global, T+36 regionalGlobal run at 0Z and 12Z. Regional run at 6Z & 18Z
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 14
Ensemble Creation – Analysis Perturbations
To achieve these desirable properties: Not sufficient to sample randomly
models have ~107 degrees of freedom - too many slow-growing directions!
Look for rapidly growing perturbations Singular vectors (ECMWF)
Error breeding (NCEP) New! Ensemble Transform Kalman Filter (Met
Office) Thanks to Craig Bishop and colleagues.
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 15
Singular Vectors (SVs)
SVs use linear adjoint of ECMWF model to identify fastest-growing directions in phase-space over the next 48 hours. SV perturbations scaled by forecast error statistics
at 48h - fast-growing so very small at initial time Perturbations also include Evolved SVs from
48h previously identify areas of greatest analysis uncertainty
(where model background is likely to be in error)
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 16
SV Perturbations
Each perturbation is a linear combination of: 25 NHem SVs 25 SHem SVs 25 Tropical
moist SVs targetted on Caribbean TCs
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 17
Error Breeding
Start with random perturbation - allow to grow in forecast Rescale bred mode to analysis errors (fixed climatological rescaling factor)
Use for perturbation in next cycle
Cycle “breeds” the rapidly growing modes in the analysis cycle
Toth and Kalnay (1997), MWR 125, 3297-3319
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 19
Ensemble Transform Kalman Filter (ETKF)
T+12 perturbed forecast
T+12 ensemble mean forecast
( - ) + =
( - ) + =
( - ) + =
( - ) + =
( - ) + =Transform matrix
Control analysis
Perturbed analysis
0.9 Pert 1-0.1 Pert 2-0.1 Pert 3-0.1 Pert 4-0.1 Pert 5
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 20
Perturbation Structures – Mean and spread PMSL
Spread tends to be concentrated around fronts and sharp gradients
Perturbation is non-zero everywhere (in contrast to SVs)
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 21
Stochastic physics
…. the quest to increase spread!
Buizza et al., MWR, 2004
All three systems are
under-dispersive!!
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 22
MOGREPS employs three schemes to address different sources of model error: Random Parameters (RP)
Error due to approximations in parameterisation
Stochastic Convective Vorticity (SCV) Unresolved impact of organised convection (MCSs)
Stochastic Kinetic Energy Backscatter (SKEB) Excess dissipation of energy at small scales
Impact is propagated to next cycle through the ETKF
Stochastic physics in MOGREPS
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 23
Parameter Scheme min/std/MaxEntraiment rate CONVECTION 2 / 3 / 5
Cape timescale CONVECTION 30 / 30 / 120
Rhcrit LRG. S. CLOUD 0.6 / 0.8 / 0.9
Cloud to rain (land) LRG. S. CLOUD 1E-4/8E-4/1E-3
Cloud to rain (sea) LRG. S. CLOUD 5E-5/2E-4/5E-4
Ice fall LRG. S. CLOUD 17 / 25.2 / 33
Flux profile param. BOUNDARY L. 5 / 10 / 20
Neutral mixing length
BOUNDARY L. 0.05 / 0.15 / 0.5
Gravity wave const. GRAVITY W.D. 1E-4/7E-4/7.5E-4
Froude number GRAVITY W.D. 2 / 2 / 4
The Random Parameters
Stochastic scheme for the UM
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 24
RP+SCV in MOGREPS
Page 25
SKEB
Stochastic Kinetic Energy Backscatter (SKEB) Based on original idea and previous work by Shutts (2004) Related to new scheme for ECMWF EPS
Aim: To backscatter (stochastically) into the forecast model some of the energy excessively dissipated by it at scales near the truncation limit
In the case of the UM, a total dissipation of 0.75 Wm-2 has been estimated from the Semi-lagrangian and Horizontal diffusion schemes. (Dissipation from Physics to be added later on)
Each member of the ensemble is perturbed by a different realization of this backscatter forcing
Page 26
SKEB
Streamfunction forcing:1
( , )2
DF K R
K.- Kinetic En.; R.- Random field;
D.- Dissipated en. in a time-step
R is designed to reproduce some statistical properties found with CRMs
Largest at the jets/storm track
Example: u increments at H500
Page 27
SKEB
Preliminary results: Positive increase in spread (comparable to that seen at ECMWF)
SKEB
RP+SCV
Increase in spread respect to an IC-only ensemble
500 hPa geopotential height
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 28
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 29
Products for the Risk Manager
Plot of ensemble spread Range of uncertainty
0%
100%
Prob
Probability graph for multiple severity thresholds
Example of use for risk management in offshore oil industry
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 30
2006-2009 plans
Forecast uncertainty information derived from EPS (July 2007)
Report on public understanding of probabilistic forecast information based on experiments at Exeter University (July 2007)
Ensemble surge prediction system trials (October 2007)
Report on predicting extreme deviations from ensemble mean using singular vector perturbations (March 2008)
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 31
2006-2009 plans
Probabilistic short-range first-guess warning system for severe weather (March 2008)
Verification report on first-guess warnings (March 2009)
50 km global ensemble, 12km regional ensemble (November 2009)
Verification report on the enhanced resolution ensembles (March 2010)
Report on potential benefit of a convection-resolving EPS (March 2010)
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 32
HIGH RESOLUTION DATA ASSIMILATION
Sue Ballard
Z. Li, M. Dixon, S.Swarbrick, O.Stiller and H. Lean
Met Office, JCMM, Reading University
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 33
Contents
Aim of high resolution convective scale system Prediction of flood risk, replace nowcasting system Detailed local weather 4km UK 2005, 1.5km ~ 2008-2010
Trial system – small domains
Data assimilation options
Assimilation issues Impact of data assimilation Impact of relative humidity and latent heat nudging 4DVar of cloud and precipitation Assimilation of radar doppler radial winds
Conclusions
Exploitation of high resolution observations
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 34
High Resolution Trial Model
1 km76 levelsResolved convection
4 km38 levelsMass-limited convection
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 35
Original HRTM Assimilation Options
12 km 3D-Var Data Assimilation With or without moisture and Latent Heat Nudging (LHN)
using AC scheme (referred to as MOPS data – moisture observation processing system)
i.e. spin up 4km, 1km from 12km T+1 each cycle.
4km 3D-VAR with continuous cycles with or without MOPS 1km with nudged reconfigured 4km increments using IAUWith or without LHN and moisture nudging using AC scheme
IAU – increments output from 3D-Var and fixed over time window
AC scheme – increments depend on latest model fields so vary with timestep through weighting factor and model evolution/impact of data
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 36
Plans - ongoing
4km MOPS - Hourly cloud, 15min precipitation, filtering, weights Background errors – lagged/unlagged, lengthscales Operational doppler radar winds – superobbing, errors, monitoring
Salford Univ and COST 731
Observations – Satellite Applications + Radar Group + Obs Radar reflectivity – observation operators, compare model and obs
Reading Univ Geostationary imagery – low level moisture, cloud top Radar refractivity – low level moisture (Reading Univ) Wind profiler humidity, ground based radiometer, cloud radar
Development of 3D-Var and 4D-Var for direct assimilation of cloud and precipitation
3D-Var MOPS cloud cover, precipitation rate – currently not resourced Cloudy radiance, PF physics, infrastructure
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 37
Moisture Observation Preprocessing
Resolution: 15km, 3 hours
(Testing 1 hour)
Surface reports
Satellite data Radar data
3D Cloud fraction
3D Relative humidity
Nudge model state
Precipitation5km smoothed to 15km HourlyTesting 15min
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 38
T-3 T-1 T+0 T+1 T+3
AC scheme/UM3D cloud fractionSurface rainrate
IAU3 hour f/c: background Hourly ModelOb
Next analysisPrevious analysisNudging RH & Latent heat
T+2T-2
Conventionalobservations
3D-Var (FGAT)
Obs window
3D-Var system including MOPS RH and LH nudging via AC scheme
6hr accumulations from13Z to 19Z 16/8/04 from 12UTC analysis
Rain rates at 14.30 UTC from 12UTC analysis
With 4km 3D-Var +MOPS radarSpun-up from 12km T+1
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 40
Impact of cloud and precipitation data
Radar1 hour accumulation
T+2 forecast 15min precip and hrly cloud
T+2 forecast No MOPS data
14UTC 25 August 2005 – CSIP IOP 18
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 41
Development of 4D-Var
4D-Var operational in global and 12km NAE models3D-Var operational in 12 and 4km UK models3D-Var being set-up/run for 1.5km model
4D-Var NAE has MOPS RH and latent heat nudging in outer loop
Developing direct assimilation of surface precipitation rates (accumulations?)Cloudy radiancesCloud top pressure
Starting to set up research 4D-Var at 4km resolution
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 42
Trial Results - NAE summer rainfall
t+9 3DVAR
t+9 4DVAR radar
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 43
Exploitation of high resolution data
Radar radial doppler winds
Initial development using Chilbolton research radar – single elevation
Now winds available from 2-4 radars in operational network – multiple elevations
Need to modify background errors to exploit high resolution information
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 44
Impact of S-band radial radar wind data- radial wind on 1deg scan elevation
12km Back-ground
Super-obbedRadarDopplerwind
½ Length scaleAnalysis
Reduced background wt
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 45
Impact of S-band radial radar wind data- radial wind on scan elevation
4km Back-ground
Super-obbedRadarDopplerwind
½ Length scaleAnalysis
Reduced background wt
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 46
Need to combine synoptic scale and high resolution analysis
3D-Var analysis in small area cannot capture synoptic scales
Need to somehow get synoptic scale information from larger area coarser resolution analysis
Can analyse different scales in different areasHowever won’t always have an up-to-date coarser resolution analysis eg 6 hourly with high resolution hourly
Needs further research
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 47
theta inc
12km analysis
“new” 4km analysis
/12km back
“new” 4km analysis
/4km back & half length
standard 4km analysis doesn’t see obs outside domain
Zero at boundary
4km short wave analysis 12km long waves
Problem of small domain Scale selective analysis
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 48
Conclusions
Need 1-4km to capture small scale severe events Need DA to overcome spin-up of explicit convection MOPS RH & LHN improves locations
Amounts sensitive to model formulation, weights, frequency of data
Ideally want to use assimilation of cloud and precipitation in 3D-Var and 4D-Var
Need to combine synoptic scale and convective analysis
Need improved background error covariances Need to move towards full analysis for 1km model
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 49
Plans - Future
Aim: 1hrly forecasts 0-6hours 1-1.5km NOWCASTS also 36 hour UK forecasts ?
Need to move towards full analysis for 1km model Ideally want 4D-Var and Ensembles - Start with 3D-Var +MOPS
need to build on experience with 4km and NAE Use reduced vertical resolution (and horizontal?) for
analysis? High resolution data Balance and background errors Variable resolution model Surface analysis – SST and soil mositure
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 50
Other Collaborations
DARC (Reading University) PhD – combining small scale and large scale in LAM
analysis Post-doc/lecturer – surface friction in control variable Post-doc/lecturer – non-linear evolution of Gaussian pdfs Post-doc – balance at convective scale Post-doc – wavelet transforms Post-doc and PhD – Ensemble Kalman Filter
EPSRC project – Peter Clark, Surrey, Aston FREE (Flood Risk from Extreme Events) – Reading
University, Met Office and CEH, Wallingford – assimilation of clear air doppler winds and humidity from refractivity
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 51
Current/planned data sources include:
Surface observations : now SYNOPs hourly, 69 stations every 10mins, full network every 10 mins by 2006-2009
AMDAR : now every 3 hours take off and landing can request hourly at extra cost
Geostationary imagery: every 15mins
Radar VAD profile: every hour user requirement, every 15mins potentially Radar radial doppler winds: every 15mins, 5 elevations range 125km now 2 radars
Rainfall rate analysis : now every 15minutes 12 radars potentially every 5 mins
Radar reflectivity : 12 radars every 5 mins , 5 elevations range 255km
Cloud cover analysis: every hour (potentially every 15mins)
Wind profiler: 5 sites every 30mins (poss 15mins)
GPS: every 15mins 70-150 sites in GB end 2006
Integrated system – wind profiler, microwave radiometer (1+2), cloud radar, ceilometer, GPS
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 52
Radar Network Coverage – 2006
1km resolution
2km
5km
© Crown copyright 2006 COSMO, 18-21 September 2006, Bucharest Page 53
2006-2009 plans
Deliver capability to assimilate operational Doppler radar winds (March 2006)
Higher frequency cycles at 1km resolution (March 2007)
Initialise high resolution model using high resolution observations but remaining consistent with large-scale model at synoptic scales (December 2007)
Enhancements to convective scale data assimilation (December 2008)