ICON Stock-Taking Report - COSMO model · 2016-12-20 · Slow-physics processes (convection, cloud...
Transcript of ICON Stock-Taking Report - COSMO model · 2016-12-20 · Slow-physics processes (convection, cloud...
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ICON Stock-Taking Report
Florian Prill, Gunther Zangl, and the ICON Team
COSMO GM 2013September 2–5, 2013
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Outline
Introduction: Main goals of the ICON project
Important features of ICON
Technical model characteristics
Selected results and ongoing work
Schedule towards operational application
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Introduction
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ICON = ICOsahedral Nonhydrostatic Model
Joint development project of DWD andMax-Planck-Institute for Meteorology for thenext-generation global NWP and climatemodelling system
Nonhydrostatic dynamical core on an icosahedral-triangularC-grid; coupled with full set of physics parameterizationsTwo-way nesting with capability for multiple non-overlapping nestsper nesting level; vertical nesting, one-way nesting mode andlimited-area mode are also available
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Primary Development Goals
Applicability on a wide range of scales in space and time down to meshsizes that require a nonhydrostatic dynamical core
Better conservation properties (air mass, mass of trace gases and moisture,consistent transport of tracers)
Built to run on vector computers as well as x86 based commodity clusters,scales to O
(104+
)cores
Grid nesting in order to replace both GME (global forecast model, mesh size20 km) and COSMO-EU (regional model, mesh size 7 km) in the operationalsuite of DWD
At MPI-M: ocean model based on ICON grid structures and operators;limited-area mode of ICON to replace regional climate model REMO
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Dissemination and Exchange
Models:
COSMOcommon physics packages
ICON-ARTaerosols and reactive trace gases
Projects:
HD(CP)2
very high-resolution simulationto advance the parameterization of clouds and precipitation
ICOMEXICOsahedral-grid Models for EXascale Earth system simulations
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Model Description
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Nonhydrostatic Equation System (Dry Adiabatic)
∂tvn + (ζ+ f ) vt + ∂nK + w ∂zvn = − cpdθv∂nπ
∂tw +vn · ∇w + w ∂zw = − cpdθv∂zπ− g
∂tρ +∇· (vρ) = 0∂t(ρθv)+∇· (vρθv) = 0 (vn, w, ρ, θv: prognostic variables)
vn, w: velocity components
ρ: density
θv: virtual potential temperature
K: horizontal kinetic energy
ζ: vertical vorticity component
π: Exner function
Discretization
Arakawa C-grid with mass-related quantities at cell circumcenters
Lorenz-type vertical staggering
reference atmosphere: only used internally
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The Horizontal Grid
Spherical geodesic grids derived from the icosahedron
R3B01 R3B03 optimized
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Grid Structure with Nested Domains
grid topology stored in NetCDF file format (GRIB format infeasible)
Effective mesh size: ∆x ≈ 5050/( n 2 k ) [km]root divisions bisections
Example:
R2B7 : n = 2, k = 7
20 km global res.≈ 1.3 · 106
sphericaltriangles
× 90 vertical levels(up to 75 km)
global domain
local domain(s)
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Smooth Level Vertical (SLEVE) Coordinate
GMEL60
half levels
z [m]
75 0001
65 5415
56 31810
48 44215
41 54320
35 43625
30 00230
25 15935
20 84540
17 01145
13 62050
10 64055
8 04760
5 82365
3 95470
2 43275
2090
10 20 30 40 50 60 70 80 90
200
400
600
800
1 000
1 200
1 400
1 600
1 800
2 000
2 200
2 400
2 600
2 800
∆z [m]
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Numerical Implementation
Two-time-level predictor-corrector time stepping scheme
Horizontally explicit, vertically implicit on sound waves;larger time step (usually 4x or 5x) for tracer advection/fast physics
Finite-volume tracer advection scheme (Miura) with 2nd-order and 3rd-orderaccuracy for horizontal tracer advection
2nd-order and 3rd-order (PPM) for vertical advection with extension to CFLvalues much larger than 1 (partial-flux method)
Monotonous and positive-definite flux limiters
Mahrer-type pressure discretization (Zangl 2012, MWR)
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Physics ParameterizationsProcess Authors Scheme Origin
RadiationMlawer et al. (1997)Barker et al. (2002)
RRTM (later with McICA McSI) ECHAM6/IFS
Ritter and Geleyn (1992) two-streamδ GME/COSMONon-orographicgravity wave drag
Scinocca (2003)Orr, Bechtold et al. (2010) wave dissipation at critical level IFS
Sub-grid scaleorographic drag Lott and Miller (1997) blocking, GWD IFS
Cloud coverDoms and Schättler (2004) sub-grid diagnostic GME/COSMOKöhler et al. (new development) diagnostic (later prognostic) PDF ICON
MicrophysicsDoms and Schättler (2004)Seifert (2010)
prognostic: water vapor, cloud water,cloud ice, rain and snow GME/COSMO
ConvectionTiedtke (1989)Bechthold et al. (2008)
mass-flux shallow and deep IFS
Turbulent transferRaschendorfer (2001) prognostic TKE COSMOLouis (1979) 1st order closure GMENeggers, Köhler, Beljaars (2010) EDMF-DUALM IFS
LandHeise and Schrodin (2002), Machulskaya, Helmert, Mironov (2008, lake)
tiled TERRA + FLAKE + multi-layer snow GME/COSMO
Raddatz, Knorr JSBACH ECHAM6
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Physics-Dynamics Coupling
Fast-physics processes: incremental update in the sequencesaturation adjustment→ transfer scheme→ surface coupling→ turbulence→ cloud microphysics→ saturation adjustment
Slow-physics processes (convection, cloud cover diagnosis, radiation,orographic blocking, sub-grid-scale gravity waves): tendencies are added tothe right-hand side of the velocity and Exner pressure equation
Diabatic heating rates related to phase changes and radiation areconsistently treated at constant volume
Option for reduced radiation grid
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Technical Model Characteristics
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Growth of Performance and Model Cost at DWD1966
1970
1975
1980
1985
1990
1995
2000
2005
2010
2015
10−1
101
103
105
107
109
1011
Moore’s la
w
MFlops
CDC3800
CDCCyber76
CrayY-MP4/432
CrayT3E
CrayT3E
Ausbau
IBMRS/6000SP
IBMRS/6000Ausbau
IBMp5
575
IBMP5
A
NEC
SX-9
CrayXC30
Phase0
CrayXC30
Phase1
A. Seifert / F. Prill, DWD
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Growth of Performance and Model Cost at DWD1966
1970
1975
1980
1985
1990
1995
2000
2005
2010
2015
10−1
101
103
105
107
109
1011
Moore’s la
w
MFlops
10−1
101
103
105
107
109
1011
relative
model
cost
BKL BKF GM EM DMLM GME60 GME40 GME30 GME20
COSMO DE COSMO EU COSMO DE-EPS ICON global
CDC3800
CDCCyber76
CrayY-MP4/432
CrayT3E
CrayT3E
Ausbau
IBMRS/6000SP
IBMRS/6000Ausbau
IBMp5
575
IBMP5
A
NEC
SX-9
CrayXC30
Phase0
CrayXC30
Phase1
A. Seifert / F. Prill, DWD
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Flat-MPI Performance
200
300
400
500
600
700
800
900
768 1024 1280 1536 1792 2048 3072 4096
MPI tasks
time
(s)
total
netCDF output, sp commw/out output
Test setup: ICON RAPS 2.0, IBM Power720/10/5 km, 8 h forecast, reduced radiation grid
(S. Korner, DWD, 03/2013)
25
50
75
100
150
200
250
300
350
768 1024 1280 1536 1792 2048 3072 4096
MPI taskstim
e (s
)
subtimer
nh_solvenh_solve.exchphysicsexch_data
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Hybrid Performance
Multicore transition:
75% of Top500 HPC systems have ≥ 6 cores per socket.
On-chip clock rates have increased only moderately.
The ICON model supportshybrid parallelization withMPI + OpenMP
Test setup: ICON RAPS 2.0, IBM Power720/10/5 km, 1000 steps 0
25
50
75
100
64x32x1 32x32x2 32x16x4 32x8x8 32x4x16
Procs. and Threads
Tim
e / M
emor
y (%
)
MemoryTime
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ICON’s Domain Decomposition
Geometric decomposition, 20 partitions
Criteria:
1. Static load balancing, e. g.every PE comprises sunlit andshadowed parts of the globe
2. Communication reduction
Explicit array partitioning with
halo regions
lateral boundary regions
interior points
. . . avoids conditionals in iterations.
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I/O: Bottleneck for High-Resolution NWP
Classical root I/O of high-resolution data becomes a critical issue.
The ICON model offloads all computed results to dedicated output nodes.
computation and I/O overlap
fast system layer: Climate Data Interface
WMO GRIB2 standard(ECMWF’s GRIB API)
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Current State of Affairs
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Selected Experiments and Results
(A) Idealized testDetermine ICON’s overall order of convergence
(B) Selected results of NWP test suiteWMO standard verification, comparison to GME
(C) Ongoing work: coupling with data assimilation
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Idealized TestBaldauf, Reinert and Zangl demonstrated that a rigorous assessment of ICON’smodel accuracy is possible (QJRMS, 2013, in rev.).
3D non-hydrostatic Euler equations on the sphere:
∂tv + v · ∇v = −∇p/ρ− g ez − 2Ω× v
∂tρ+ v · ∇ρ = − ρ∇ · v
∂tp + v · ∇p = c2s (∂tρ+ v · ∇ρ) c2
s = R p/ρ
Slight simplifications (extension of DCMIP test case 3):adiabatic
rigid lid BC’s: w∣∣∣surface = w
∣∣∣top = 0
Coriolis term:global f-plane approximation
Test the model response to short time-scale wave motion triggered bytemperature perturbation.
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Convergence Order of the Model
Small earth simulation: rs ← rearth/50
10−1 100
10−5
10−4
10−3
1
0.65
1
0.73
1
0.86
1
1.21
∆φ
Error
L∞-norm: wL2-norm: wL∞-norm: TL2-norm: T
For sufficiently fine resolutions: spatio-temporal convergence rate ≈ 1
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WMO Standard VerificationSelected results of NWP test suite:
Real-case tests with interpolated IFS analysis data7-day forecasts starting at 00 UTC of each day in January and June 2012
Model resolution 40 km and 13 km90 levels up to 75 km (no nesting)
Reference experiment with GME40L60 with interpolated IFS dataWMO standard verification on 1.5 regular grid
BIAS = F−A STDV =[F−A− F−A
]2
ABSE = |F−A| ANOC =
[F−R− F−R
] [A−R−A−R
]√[
F−R− F−R]2 [
A−R−A−R]2
RMSE =
√(F−A)2 SKS1 = 100
∑ |GF −GA|∑max (|GF |, |GA|)
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Verification: Sea-Level Pressure, January 2012
ICONGME40against IFS
ICON 40kmJanuary 2012NH
Verification: G. Zangl, U. Damrath, 08/2013 (DWD)
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Verification: Sea-Level Pressure, January 2012
ICONGME40against IFS
ICON 13kmJanuary 2012NH
Verification: G. Zangl, U. Damrath, 08/2013 (DWD)
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Verification: Geopotential 500hPa, January 2012
ICONGME40against IFS
ICON 40kmJanuary 2012NH
Verification: G. Zangl, U. Damrath, 08/2013 (DWD)
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Verification: Geopotential 500hPa, January 2012
ICONGME40against IFS
ICON 13kmJanuary 2012NH
Verification: G. Zangl, U. Damrath, 08/2013 (DWD)
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Verification: Sea-Level Pressure, June 2012
ICONGME40against IFS
ICON 40kmJune 2012NH
Verification: G. Zangl, U. Damrath, 08/2013 (DWD)
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Verification: Sea-Level Pressure, June 2012
ICONGME40against IFS
ICON 13kmJune 2012NH
Verification: G. Zangl, U. Damrath, 08/2013 (DWD)
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Verification: Geopotential 500hPa, June 2012
ICONGME40against IFS
ICON 40kmJune 2012NH
Verification: G. Zangl, U. Damrath, 08/2013 (DWD)
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Verification: Geopotential 500hPa, June 2012
ICONGME40against IFS
ICON 13kmJune 2012NH
Verification: G. Zangl, U. Damrath, 08/2013 (DWD)
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Integrated System of Data Assimilation and Forecast
Ongoing: Systematic analysis and optimization of forecast quality of ICONusing test series with continuous assimilation cycling
R. Potthast, H. Anlauf (DWD)
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Limited-Area Mode
The HD(CP)2 project will push forwardthe development of the limited-areaversion of ICON
Capability of generating and readingtime-dependent boundary data
Upgrade the non-hydrostaticdynamical core and the physicalparameterizations of ICON to theneeds arising from very small scales
Aim: Length scales down to∆x = 100 m over Germany for LESapplications
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ICON Ensemble
Short range ensemble required for EnKF (J. Ambadan, DWD).
ICON forecast ensemble: First experience within the SFP
”Erschließung und Intensivierung der Nutzung von Fernerkundungsdaten”
Milestones until 2012 – 2014 (M. Denhard, DWD):
implementation of a process chain for a global ensemble forecast
evaluation of statistical properties
optimization for short-range weather forecasts over Europe
Tentative schedule for an operational ICON ensemble:
roll-out plan: ca. 2017
configuration ∼ 20 members, 72 hrs forecast
Also HD(CP)2 S5.WP3: Ensemble simulations and uncertainty (D. Klocke, DWD)
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Final Remarks
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Final Remarks
The global ICON model is entering the home stretch
Verification results are on par / exceeding the GME40L60
optimization of forecast quality still ongoing
Technical parts scale on massively parallel systems
The ICON forecast model has matured over the last 12 months,but . . .
the model is not yet a turnkey application software,still code development needed!
COSMO-CLM December 12, 2013 1:30 – 4:30 pm: DWD, OffenbachInformation event for CLM applications!
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ICON Modelling FrameworkICON RAPS benchmarkfor HPC vendors
Stand-alone grid generatorPublic grid repository on the Web (http://icon-downloads.zmaw.de)
Pre- and post-processing utilitiesI interpolate to/from regular gridsI extract data sets (local regions)I locate cell indices
Yet to come:
Official releases
ICON documentation anddatabase description
Relaunch of public website
User tutorials
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Schedule Towards Operational Application
Q4/2014:first step of operational use:replacement of GME with 13 kmICON without nesting
Q2/2015:replacement of COSMO-EU bynested ICON domain (13–6.5 km)
Q3 – Q4/2013:start of pre-operational testswith data assimilation
Summer 2014:roll-out: source code license and documentation,user seminar (planned)
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Appendix
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Appendix: Performance Test Case
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Appendix: Effect of Reduced Radiation Grid
dycore comm. 2%
dynamical core 14%
hor. diffusion 2%transport 6%
other physics 20%
misc, e.g. I/O andfeedback 2%
radiation 54%
R2B06, without reduced radiation grid
dycore comm. 2%
dynamical core 23%
hor. diffusion 3%transport 9%
other physics 30%
misc, e.g. I/O andfeedback 3%
radiation 30%
with reduced radiation grid
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