HIRLAM towards mesoscale and physics towards AROME - PowerPoint PPT Presentation

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HIRLAM towards mesoscale and physics towards AROME

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6.2.4 29 March. Radiation changes. Increased mixing in stable ... 6.3.4 21 Sep many physics corr cleanup FAK. Mod (reduced) z0 and drag and smoother mixing ... – PowerPoint PPT presentation

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Title: HIRLAM towards mesoscale and physics towards AROME


1
HIRLAM towards meso-scale and physics towards
AROME
  • Per Undén
  • HIRLAM-6

2
HIRLAM Vision for 2010
  • (I) Best available 2.5 km meso-scale modelling
    system operational in most of the HIRLAM
    countries for parts or all of the territory
    and applicable for 1 km
  • Non-hydrostatic (non approximated equations)
  • Efficient dynamics (long time steps possible)
  • Advanced physics for clouds and precipitation
    species and turbulence (convection mainly
    resolved)
  • Advanced data assimilation that initialises
    particularly the moist processes (rain and
    clouds)
  • Integrated system for estimating the
    probabilities
  • Transparent boundary treatment

3
  • (II) Synoptic scale 10 km model for coupling from
    ECMWF and for regional forecasting
  • Of equal quality to global model and tightly
    coupled to ECMWF
  • Consistent physics with meso-scale model
  • To provide best forecasts of synoptic
    disturbances with short data cut off
  • To provide coupling to meso-scale and other
    models and many applications

4
Why meso-scale model?
  • Is stated in HAC strategy 2002 and in HIRLAM-6
    MoU and Management Group needed to take
    intitiative
  • Is absolutely needed in mountainous countries
  • Is needed for severe precipitation weather not
    resolved otherwise
  • Needed for applications (wind energy, radar usage
    , environmental dispersion, aviation
  • Because everybody else does it

5
How?
  • Develop own meso-scale model? No
  • Tartu NH outside Project work and not full Euler
    equations and not really used in member
    institutes
  • Not enough dynamics staff
  • Large effort years of development
  • Duplication of work in Europe
  • New developments in assimilation and physics also
  • Still resources needed for synoptic model as well
  • Collaborate - Yes
  • Quickly re-gain lost time of development
  • Sharing research resources with partner(s)
  • Actively contributing in many key areas
  • Relying on partner(s) for other things
  • Enough critical mass in all areas

6
Why ALADIN?
  • HIRLAM and ALADIN are closely related
    scientifically
  • Spectral LAM and analysis with extension zones
  • Both born out of ECMWF and ECMWF similarities
  • ECMWF code commonality in ALADIN
  • ALADIN non-hydrostatic model breakthrough
  • Advanced meso-scale physics through Meso-NH -gt
    AROME
  • Advance Data Assimilation developing
  • Meteo-France participates in HIRLAM since 1992
  • Good experience of MF collaboration in HIRLAM
  • Informal offers in 2003 to use ALADIN NH dynamics
  • Likely to be a true collaboration from both sides
  • Many partners of different size
  • Organisation more dispersed than HIRLAM

7
Choices made (MG Sept 2003, HAC Jan 2004, Council
June 2004, Dec 2004)
  • Collaborate with MF/ALADIN at code collaboration
    level on meso-scale modelling gt
  • Achieves all the advantages of ALADIN and AROME
    dynamics, physics and Data Assimilation
    developments AND ECMWF IFS System and Code
    standards
  • Commitments to synchronise the code at regular
    intervals
  • Coordination of research in the agreed Area and
    sharing of the work

8
Further necessary steps
  • Agreement on collaboration in meso-scale
    modelling and associated areas
  • Definition of cross steering mechanisms
  • Formulation of rights and obligations and MoUs
    2006-
  • Coordination of common research areas for 2006 -

9
Choices not made (yet?)
  • Code collaboration in the rest (synoptic scale
    model)
  • Or HIRLAM may continue with own separate code for
    synoptic scale
  • Scientific and technical extra work to maintain
    and develop two code systems (the synoptic and
    meso-scale model share large parts of the codes
    and scripts)
  • Allows for clear HIRLAM brand for synoptic
    scale model (10 km)
  • Some inconsistencies in coupling of boundaries to
    meso-scale model (physics and also grid)
  • HIRLAM physics in ALADIN synoptic model
  • HIRLAM brand can still be maintained

10
HIRLAM status
  • Hydrostatic 2 TL SL-SI LAM
  • Non-hydrostatic p-anelastic kernel (Tartu)
  • Reference at 22 km 40 levels
  • 50 km 30 22 17 11 5 km (2.5)(1.4)
  • Comprehensive physics for synoptic scales
  • (meso-b 40-10 km)
  • SW/LW simple radiation
  • CBR TKE 1D turbulence advected TKE
  • ISBA surface tiled scheme with assimilation/snow/s
    oil
  • STRACO conv/cond (Kuo-Sundqvist type)
  • Kain-Fritsch/Rash-Kristjansson alternative
  • Meso-scale orography/Sub grid scale implementing

11
Model Physics in High Resolution NWP
Physics No Mans Land
Klemp (2002) Dublin WS
12
6 h WRF Forecast Reflectivity at 6/15/02 18z
4 km Lin
10 km Lin, KF
Radar Composite
10 km Lin
(Weisman, Wang, Klemp)
(dBZ)
13
HIRLAM components for Meso-scale
  • Surface scheme ISBA, snow, soil models
  • Still mainly horizontally uncoupled upper air
    flow couples but flux aggregation ?
  • Tiled or untiled ? tiles still exist below 1 km
  • Turbulence scheme CBR TKE - moist
  • 1D or 3D ? 1D at 3 km and 3D at 1 km?
  • Interactions with cloud scheme and convection
  • Shallow convection ?
  • Radiation scheme slopes considered
  • 3D ? - More advanced more species
  • Cloud scheme more advanced and more species
  • MSO/SSO
  • MSO relaxed but SSO needed at 1 km

14
AROME and ALADIN components
  • Turbulence CBR HIRLAM 1d
  • Externalised ISBA HIRLAM tiled
  • (Kain-Fritsch synoptic scale - HIRLAM)
  • Town model
  • Advanced cloud physics
  • Radiation scheme (Morcrette, ECMWF)
  • Chemical modelling

15
HIRLAM strategy and plans
  • Maintain and improve HIRLAM physics for synoptic
    scales
  • Interface HIRLAM physics in ALADIN and compare in
    meso-scale and with AROME
  • Integrate some as AROME option or mainly AROME in
    meso-scale
  • Compare synoptic ALADIN with HIRLAM physics with
    HIRLAM
  • Plan for transfer to ALADIN with HIRLAM switches

16
HIRLAM work with ALADIN in 2005
  • Make experiments at 11 and 2.5 km
  • Interface HI -ALADIN coupling-boundaries
  • Interface some HI physics
  • Implement climate generation software
  • Introduce AROME system
  • Experience from AROME from events -evaluate some
    HI physics
  • Develop meso-scale diagnostics

17
Synoptic HIRLAM work 2005
  • 3D-VAR improvements
  • 4D-VAR to be made operational (almost)
  • More satellite use
  • Surface analysis SST , ice, SAF products
  • Turbulence and moist version
  • Surface scheme, fluxes, snow
  • Meso-scale / sub-grid scale orography
  • KF convection, statistical cloud scheme
  • SL dynamics
  • Transparent boundary conditions
  • Verification and diagnostics
  • CVS code maintenance and unification -HIRLAM

18
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20
6.3.5 test
21
Challenges for meso-scale forecasting
  • Meso-scale data and assimilation
  • Modelling and predictability
  • Probability / ensemble forecasting
  • Presentation to users
  • Verification at high resolution and of extreme
    events
  • Computational resources

22
Summary
  • Synoptic system state of the art
  • Synoptic system needs to be maintained
  • Meso-scale modelling through collaboration
  • Synoptic scale should be collaborated on
  • A number of HIRLAM physics modules valid in
    meso-scale or combine the best
  • Many challenges in meso-scale not all in
    physics

23
Physics interfaces and options
  • All building blocks of physics routines should be
    available without restrictions
  • ARPEGE/ALADIN
  • Meso-NH
  • HIRLAM
  • ALARO
  • Start with low-level routines to adapt for
    interface and high level changes to use them
  • Iterate and work and clarify the design

24
Reference system
  • 6.2.2 Feb 2004 -gt Reference 6.3 RCR
  • Climate files and corrections
  • 6.2.3 22 Mar climate corrections
  • 6.2.4 29 March
  • Radiation changes
  • Increased mixing in stable conditions
  • Much increased roughness length
  • parallelisation much improved
  • 6.2.5, 6.3.2 minor corrections HIRVDA
  • 6.3.3 28 June water vapour saturation mod
  • 6.3.4 21 Sep many physics corr cleanup FAK
  • Mod (reduced) z0 and drag and smoother mixing
  • Ritchie-Tanguay T eq. SL extrap. techn.
    Changes, job subm.
  • 6.3.5 Nov
  • Rotated surface stress and reduced stable mixing
  • Phys-Dyn coupling
  • Melting of soil ice faster many technical
    climate files

25
Envisaged HIRLAM configurations
26
  • High performance computer resources
  • 4 x higher resolution gt 4x4x4, but..
  • Smaller area(s) ,
  • More efficient dynamics
  • - more expensive physics
  • Linux clusters very promising to reduce costs
  • Moores law 2x / 1.5 years wait .
  • But EPS .. More forecasts- lagged average?

27
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