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Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

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Page 1: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Introduction to NMMB Dynamics: How it differs from WRF-NMM

Dynamics

Zavisa JanjicNOAA/NWS/NCEP/EMC, College Park, MD

Page 2: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Basic Principles

Forecast accuracyFully compressible equationsDiscretization methods that minimize generation of computational noise and reduce or eliminate need for numerical filtersComputational efficiency, robustness

Janjic, Z., and R.L. Gall, 2012: Scientific documentation of the NCEP nonhydrostatic multiscale model on the B grid (NMMB). Part 1 Dynamics. NCAR Technical Note NCAR/TN-489+STR, DOI: 10.5065/D6WH2MZX.

http://nldr.library.ucar.edu/repository/assets/technotes/TECH-NOTE-000-000-000-857.pdf

Page 3: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Nonhydrostatic Multiscale Modelon the B grid (NMMB)

Wide range of spatial and temporal scales (meso to global, and weather to climate)Built on NWP and regional climate experience by relaxing hydrostatic approximation rather than by extending a cloud model to synoptic scales (Janjic et al., 2001, MWR; Janjic, 2003, MAP)Further evolution of WRF Nonhydrostatic Mesoscale Model (NMM) (Janjic, 2005, EGU; Janjic & Black, 2007, EGU; Janjic & Gall 2012, NCAR)Add-on nonhydrostatic module

Easy comparison of hydrostatic and nonhydrostatic solutionsReduced computational effort at lower resolutions

Pressure based vertical coordinate, nondivergent flow remains on coordinate surfaces

Page 4: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Inviscid Adiabatic Equations

TSfc Difference between hydrostatic pressures at surface and top

Hydrostatic pressureNonhydrostatic pressure

pRT Gas law

Hypsometric (not “hydrostatic”) Eq.

0

ss

ssst ss

v Hydrostatic continuity Eq.

Continued …

Constant depth of hydrostatic pressure layer at the top 1 Zero at top and bottom of model atmosphere

2 Increases from 0 to 1 from top to bottom

tyxsstsyx T ,,),,,( 21 General hybrid coordinate

Page 5: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

1p

Third Eq. of motion

Integral of nonhydrostatic continuity Eq.

vkv fpdtd

ss )1( Momentum Eq.

p

ssp

tp

cT

ssT

tT

sp

s vv Thermodynamic Eq.

ws

swtw

gdtdwg s

sv

11Vertical acceleration

Inviscid Adiabatic Equations, contd.

Page 6: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Nonhydrostatic Dynamics Specifics

F, w, e are not independent, no independent prognostic equation for w!More complex highly implicit numerical algorithm, but no over-specification of wNo computation of 3D divergence e <<1 in meso and large scale atmospheric flows

Impact of nonhydrostatic dynamics becomes detectable at resolutions <10km, important at 1km.

Page 7: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Page 8: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Conservation of important properties of the continuous system aka “mimetic” approach in Comp. Math. (Arakawa 1966, 1972, …; Jacobson 2001; Janjic 1977, 1984, …; Sadourny, 1968, … ; Tripoli, 1992 …)

Nonlinear energy cascade controlled through energy and enstrophy conservationA number of properties of differential operators preservedQuadratic conservative finite differencingA number of first order (including momentum) and quadratic quantities conservedOmega-alpha term, transformations between KE and PEErrors associated with representation of orography minimizedMass conserving positive definite monotone Eulerian tracer advection

Discretization Principles

Page 9: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Horizontal E grid

h v h v hv h v h vh v h v hv h v h vh v h v h

h v

v h

ddy

dx

Page 10: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Vertical Coordinate

PDsgPDsgPp TOPT 21

TP

TOPT PDP

PDPDP TOPT

TOPPD

PD

rangepressure

rangesigma

0

10

2

1

sg

sg

10

1

2

1

sg

sg

Sangster, 1960; Arakawa & Lamb, 1977

Page 11: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Nonhydrostatic Multiscale Modelon the B grid (NMMB)

Coordinate system and gridGlobal lat-lonRegional rotated lat-lon, more uniform grid sizeArakawa B grid

h h h v vh h h v vh h h

Lorenz vertical gridPressure-sigma hybrid (Simmons & Burridge 1981, Eckermann 2008)

h h

h hVdy

dx tyxsstsyx T ,,),,,( 21

tyxsstsyx ,,)(),,,( 2

Page 12: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

0

500

1000

1500

2000

2500

3000

010000

2000030000

4000050000

6000070000

8000090000

100000

Layer thicknesses

Pressure

0

500

1000

1500

2000

2500

3000

010000

2000030000

4000050000

6000070000

8000090000

100000

Layer thicknesses

Pressure

ps=1000 hPa

0

500

1000

1500

2000

2500

3000

010000

2000030000

4000050000

6000070000

8000090000

100000

Layer thicknesses

Pressure

0.7

0.75 0.8

0.85 0.9

0.95 1

16

1116

2126

3136

4146

5156

Cumulative topography height

100 m bins

ps=750 hPa

ps=500 hPa

Figure 7. Examples of thicknesses of 64 NMMB layers in Pa depending on surface pressure, 1000 hPa (upper left panel), 750 hPa (upper right panel) and 500 hPa (lower left panel). Transition to hydrostatic pressure coordinate occurs at about 300 hPa, and the top of the model atmosphere is at 10 hPa. Cumulative distribution of topography height in medium resolution global NMMB is also shown in 100 m bins (lower right panel).

Page 13: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Nonhydrostatic Multiscale Modelon the B grid (NMMB)

Time steppingNo splittingAdams-Bashforth for horizontal advection of u, v, T (no iterations) and Coriolis forceCrank-Nicholson for vertical advection of u, v, T (implicit)Forward-Backward (Ames, 1968; Gadd, 1978; Janjic and Wiin-Nielsen, 1977, JAS) fast wavesImplicit for vertically propagating sound waves (Janjic et al., 2001, MWR; Janjic, 2003, MAP, 2011, ECMWF)

Page 14: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

WRF NMM Lateral Boundary Conditions

Specified from the driving model along external boundaries4-point averaging along first internal row (Mesinger and Janjic, 1974; Miyakoda and Rosati, 1977; Mesinger, 1977)Upstream advection area next to the boundaries from 2nd internal row

Advection well posed along the boundaries, no computational boundary condition neededDissipative

HWRF internal nesting discussed elsewhere

Page 15: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

WRF NMM Lateral Boundary Conditions

h v h v h v h v h v h v h v h v h v h v h v h

v h v h v h v h v h v h v h v h v h v h v h v

h v h v h v h v h v h v h v h v h v h v h v h

v h v h v h v h v h v h v h v h v h v h v h v

h v h v h v h v h v h v h v h v h v h v h v h

v h v h v h v h v h v h v h v h v h v h v h v

h v h v h v h v h v h v h v h v h v h v h v h

v h v h v h v h v h v h v h v h v h v h v h v

h v h v h v h v h v h v h v h v h v h v h v h

v h v h v h v h v h v h v h v h v h v h v h v

h v h v h v h v h v h v h v h v h v h v h v h

Domain Interior

External Boundary1st Internal Row, 4 Pt Averaging

Upstream Advection Area

Page 16: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Nonhydrostatic Multiscale Modelon the B grid (NMMB)

Regional domain lateral boundariesNarrow zone with upstream advection, no computational outflow BC for advectionNo 4-point averaging, not neededBlending zoneNMMB internal lateral boundaries addressed elsewhere

Page 17: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

NMMB Lateral Boundaries

Regional domain lateral boundaries

outer boundary for mass variables

outer boundary for wind variables

blending zoneupstream advection

Page 18: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

NMMB Physics

Upgraded NCEP WRF NMM “standard” physical package

RRTM, GFDL radiationNOAH, LISS land surface modelsMellor-Yamada-Janjic turbulenceFerrier microphysicsBetts-Miller-Janjic convection

ExtensionsNEMS GFS physicsSeparate SAS, Zhao, Thompson, GFS PBL, WSM6 ...

Page 19: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Atmospheric Spectrum

Reformulating advection terms from E to B grid was most difficult False nonlinear energy cascade (Phillips, 1954; Arakawa, 1966 … ; Sadourny 1975; …) major generator of excessive small scale noise

Other computational errors

Historically, problem controlled by:Removing spurious small scale energy by numerical filtering, dissipationPreventing excessive noise generation by enstrophy and energy conservation (Arakawa, 1966 …)

Page 20: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Atmospheric Spectrum

Classical paper by Sadourny, 1975, JAS:

Filtering just cosmetics, atmospheric model not needed for “correct” atmospheric spectrum!

Page 21: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Atmospheric Spectrum

Instead (Sadourny, 1975, JAS):

Philosophy built into the design of the compact nonlinear momentum advection schemes for semi-staggered grids (Janjic, 1984, MWR; Janjic, 2004, AMS; Janjic and Gall, 2012, NCAR)

Page 22: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Formal accuracy does not solve the problemBlue – Janjic, 1984, MWR; red – controlled energy cascade, but not enstrophy conserving, Arakawa, 1972, UCLA; green – energy and (alternative) enstrophy conserving Different nonlinear noise levels (green scheme) with identical formal accuracy and truncation error (Janjic et al. 2011, MWR)Enhanced formal accuracy of well behaved conservative nonlinear advection scheme did not add measurable value to global forecasts in terms of Anomaly Correlation Coefficient.

Second order schemes

Fourth order schemes

116 days

Page 23: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Anomaly correlation coefficients calculated over the globe averaged over 111 cases for the second order scheme c2 (blue diamonds) and the fourth order scheme c4 (purple squares).

Page 24: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Atmospheric SpectrumNastrom-Gage (1985, JAS) 1D spectra in upper troposphere and lower stratosphere from commercial aircraft dataNo spectral gapTransition at few hundred kilometers from –3 to –5/3 slope in the 102-103 km (mesoscale) rangeInertial range, 0.01-0.3 m s-1 in the –5/3 range, not to be confused with severe mesoscale phenomena!

104

108

103

105

102

102 101103

-3

-5/3

Page 25: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

No Physics With Physics

-5/3 -5/3

-3 -3

● Spectrum in agreement with observed spun-up given physical (or spurious, e.g. sigma) sources on small scales.

● Small scale energy in short regional runs with controlled nonlinear cascade and controlled noise sources, where from?

Flat bottom (Atlantic), NMMB, 15km, 32 levels, 48h run (Loops)

Page 26: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Loop,decaying 3D turbulence, Fort Sill storm, 05/20/77.

NMM-B, Ferrier microphysics, 1km resolution, 32 levels,112km by 112km by 16.4km, double periodic, Smagorinsky constant 0.32.

Note the hump with active convection

Spectrum of w2 at 700 hPa.

Page 27: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

-5/3

Hours 3-4 average decaying 3D turbulence, Fort Sill storm, 05/20/77.

NMM-B, Ferrier microphysics, 1km resolution, 32 levels,112km by 112km by 16.4km, double periodic. Smagorinsky constant 0.32.

Spectrum of w2 at 700 hPa.

Page 28: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

2D very high resolution tests

0 0

0

0

0

0

0

0

0

Warm bubble, 100 m resolution

10

0

0

Cold bubble, 100 m resolution

-2.5

-2.5-2.5

-2.5

00000

00

0 0000

00

00 000

0

0 0 0 0

00

00

000

000 0 0 00000 000

00

000

0

0000

00

00

000 000

00

00

00

0

000

00

00

00

00

00

00

000 0

00

0

0

0

0

000 00

0

00

0

00

0

00

00

00000000

0

0

0

0

00

0

0

0

0

00

00

00

00000

00

000

0

00

0000 000

00

2.52.5

2.5

2.5

2.5

2.5

2.5

Full compressible NMM Analytical (Boussinesque) ARPS (Boussinesque)

Nonlinear mountain wave 400 m resolution

0.00

1.00

1000

.00

1295

.77

1591

.55

1887

.32

2183

.10

2478

.87

2774

.65

3070

.42

3366

.20

3661

.97

3957

.75

4253

.52

4549

.30

4845

.07

5140

.85

5436

.62

5732

.39

6028

.17

6323

.94

9000

17000

Normalized vertical momentum flux, 400 m resolution

Page 29: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Mountain waves, 8 km resolution

Convection, 1 km resolution

Page 30: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

22nd Conference on Severe Local Storms, October 3-8, 2004, Hyannis, MA.

WRF-NMM

WRF-NMM

WRF-NMM

Eta Eta Eta

20044km resolution, no parameterized convection

Breakthrough that lead to application of “convection allowing” resolution for storm prediction

Page 31: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

4 km 1.33 km Observed

A difficult tornadic situation from spring 2011, impact of resolution, courtesy of Aligo, Jovic and Ferrier

Page 32: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

27 km Global NMMB27 km Global NMMB

12 km NAM NMMB

12 km NAM NMMB

4 km NAM-nest NMMB

9 km Igor NMMB

9 km Julia NMMB

Hypothetical NMMB Simultaneous Run Global [with Igor & Julia] and NAM [with CONUS nest]

Courtesy of DiMego et al.

Page 33: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Meso Scales

Regional NMMB replaced WRF NMM in the NAM slot in 2011Hierarchy of nests running simultaneously, 12 km, 6 km, 4 km, 1.33 km (fire weather on the fly) resolutions (DiMego et al.)Hurricane runs with NMMB using HWRF set-up primarily to test the NMMB infrastructure (initialization, mechanics of nest movements, telescoping and 2-way interactions …)

Page 34: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Summary and Conclusions

Significant improvements of regional forecasts still possibleUnified model offers consistency in applications on various scales and reduced development and maintenance effort and costLimits of deterministic forecasting have not been reached yet

Page 35: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Differences between Global and Regional Versions of NMMB

Zavisa Janjic, Ratko Vasic, Tom BlackNOAA/NWS/NCEP/EMC, College Park, MD

Page 36: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Differences

Coordinate systemRegional (“basin scale”): rotated lat-lonGlobal: lat-lon

Polar boundary conditionPolar filterPolar points averagingEast-west periodicity

Page 37: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Variables near the North Pole

Conservative global polar boundary conditionsSpatial differencing as anywhere elsePolar averaging

North Pole,mass variables

ghost line,wind variables

ghost line,mass variables

wind variables

mass variables

Page 38: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Specifying Ghost Line Variables

Change sign of across the pole wind components along the ghost lineNo change at scalar points

ghost line

Page 39: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Polar Filter

Polar points singularConvergence of meridiansCoriolis force tends to infinity due to curvature terms

Polar filter“Decelerator,” tendencies of T, u, v, Eulerian tracers, divergence, dw/dtWaves in the zonal direction faster than waves with the same wavelength in the latitudinal direction slowed downNo impact on amplitudes of basic variablesPhysics not filtered

Page 40: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Polar Filter

Current set-upFiltering north of 450 N and south of 450 SAt 450 N and 450 S , considered as representative resolutionCan be changed

yx

Page 41: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Physics

Unified model offers consistency in applications on various scales and reduced development and maintenance effort and costUnified physics across the scales desirableParameterizations depend on scales and have to be differently tuned, but the same parameterization schemes still can be used

Page 42: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Physics

Upgraded NCEP WRF NMM “standard” physical package

RRTM, GFDL radiationNOAH, LISS land surface modelsMellor-Yamada-Janjic turbulenceFerrier microphysicsBetts-Miller-Janjic convection

ExtensionsGFS physicsSeparate SAS, Zhao, Thompson, GFS PBL, WSM6 ...

Page 43: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Data assimilation

Spectral GFS analysis not a good long term choiceGFS analysis even more GFS specific with GFS ensemble cross correlationsIndigenous NMMB analysis neededWork under way

Page 44: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Computational Considerations

Spherical geometry is an issue, no matter which grid topology is chosen~ 50% waste (compared to regional)Polar filter based on FFT

Serial, nonlocal FFT usedFFT fast, but requires transposition to take advantage of parallel processing

Hindrance for scaling?

Page 45: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Global, nonhydrostatic, full physicsEasily satisfies NCEP operational requirementsResolution 1149 x 811 x 64, ~ 24 km

500 processors, 7.9 wall clock min/day4000 processors, 1 year of simulation in < 17 hours, climate studies

Resolution 2305 x 1623 x 64, ~ 12 km8 x more work than 1149 x 811 x 64, ~ 24 km3600 processors, 7.6 wall clock min/day7.2 times more processors for 8 times bigger job in less time!

Operational global ~ 10 km resolution forecasts possible

Scaling on Zeus

Page 46: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Scaling

Scaling not critical at present with reasonable resolution and number of coresDepends on size and shape of sub domainsSlows down with less than 200-250 grid points per coreParallel FFT now available, presumably will reduce communications significantly

Page 48: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Long verification periods needed to obtain robust scores.To save on resources and time, a sample of 105 cases over one year at three and a half day intervals (code maintenance, launcher scripts, verification and graphics courtesy of Vasic)Both 00Z and 12Z initial data equally represented Sample cases chosen randomly, results should be reasonably representative for a full year population

Global Scales

Page 49: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Global NMMB 1149 x 811 x 64 pts. vs. GFS T574 x 64

105 randomly chosen cases from 1 year

500 hPa Height Anomaly Correlation Coefficient vs. forecast time

NMMB initialized and verified using GFS analyses and climatology

Zeus test

Global NMMB 1149 x 811 x 64 pts. vs. GFS T574 x 64

105 randomly chosen 00Z and 12Z cases over 1 year

Zhao, BMJ, mixed shallow, momentum transport

500 hPa Height Anomaly Correlation vs. forecast time

NMMB initialized and verified using GFS analyses and climatology

Page 50: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Global NMMB 1149 x 811 x 64 pts. vs. GFS T574 x 64

105 randomly chosen cases from 1 year

500 hPa Height Anomaly Correlation Coefficient vs. forecast time

NMMB initialized and verified using GFS analyses and climatology

Zeus test

Global NMMB 1149 x 811 x 64 pts. vs. GFS T574 x 64

105 randomly chosen 00Z and 12Z cases over 1 year

Zhao, BMJ, mixed shallow, momentum transport

500 hPa RMSE differences vs. forecast time

NMMB initialized and verified using GFS analyses and climatology

Recent test

RMSE difference generally remains within bounds of initial interpolation errors

Page 51: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Not usual measure in the

tropics, but what is going on there?

RMS difference NMMB-GFS (m)

AC die-off NMMB & GFS NH convective season NMMB better

July ITCZ

January ITCZ

Tropics

Global NMMB 1149 x 811 x 64 pts. vs. GFS T574 x 64

105 randomly chosen 00Z and 12Z cases over 1 year

Zhao, BMJ, mixed shallow, momentum transport

500 hPa differences vs. forecast time

NMMB initialized and verified using GFS analyses and climatology

Recent test

~ difference between two analyses

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Tropics

What is the truth?Each model has its own “convection scheme climatology”Insufficient data, more weight on model in DAS for satellite dataDifferent gravity-inertia frequency errors and geostrophic adjustment (semi-implicit vs. explicit)4-5 days oscillation (Riehl, 1954)?Each model with its own DAS needed for a fair comparison (under development for the global NMMB)

Page 53: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

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Global NMMB, Hydrometeorological Service of Serbia, Scores for 2011 and 2012, 00Z Cycle

0.47o x 0.33o , ~37km 769x541 x 64 pts.128 cores, ~12 min/day

GFS analysesVerified vs. ECMWF

(Djurdjevic et al., 2013, EGU)

Page 54: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Global NMMB, Hydrometeorological Service of Serbia, Scores for 2011 and 2012, 00Z Cycle

0.47o x 0.33o , ~37km 769x541 x 64 pts.128 cores, ~12 min/day

GFS analysesVerified vs. ECMWF

(Djurdjevic et al., 2013, EGU)

Page 55: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Global NMMB, Hydrometeorological Service of Serbia, Scores for 2011 and 2012, 00Z Cycle

0.47o x 0.33o , ~37km 769x541 x 64 pts.128 cores, ~12 min/day

GFS analysesVerified vs. ECMWF

(Djurdjevic et al., 2013, EGU)

Page 56: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

NMMB-global; GFS Dropouts cases 2011

DATE GFS NMMB(GFS)

NMMB (ECMWF)

20110304 0.72 0.77 0.85

20110317 0.71 0.79 0.89

20110430 0.69 0.88 0.89

20110616 0.75 0.84 0.83

20110617 0.74 0.73 0.84

20110618 0.73 0.81 0.88

20110619 0.62 0.64 0.81

20110620 0.70 0.61 0.72

20110629 0.63 0.79 0.88

20110702 0.63 0.90 0.94

20110713 0.71 0.38 0.55

20110718 0.68 0.59 0.58

20110806 0.72 0.83 0.84

20110807 0.71 0.73 0.83

20110808 0.73 0.87 0.91

20110813 0.69 0.84 0.85

20110912 0.71 0.76 0.81

DATE GFS NMMB(GFS)

NMMB (ECMWF)

20110131 0.75 0.81 0.87

20110209 0.75 0.77 0.88

20110222 0.70 0.75 0.81

20110306 0.65 0.69 0.84

20110320 0.71 0.86 0.88

20110325 0.62 0.69 0.70

20110327 0.72 0.66 0.76

20110403 0.75 0.64 0.74

20110414 0.72 0.72 0.75

20110421 0.75 0.78 0.90

20110506 0.68 0.66 0.90

20110507 0.72 0.84 0.88

20110725 0.75 0.88 0.90

20110728 0.72 0.88 0.90

20110925 0.73 0.73 0.84

North Hemisphere South HemisphereAnomaly correlation day-5 forecast

• 11/32 significant improvement with both analyses

• 12/32 significant improvement

with ECMWF analysis in comparison with run with GFS analysis• 17/32 improvement in

comparison to GFS with same analysis

• 2/32 score remain less then then 0.7 with both analyses

• On average better scores with ECMWF analyses

Page 57: Zavisa Janjic Introduction to NMMB Dynamics: How it differs from WRF-NMM Dynamics Zavisa Janjic NOAA/NWS/NCEP/EMC, College Park, MD

Zavisa Janjic

Barcelona Supercomputing Center Aerosol Climatology

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Zavisa Janjic

Courtesy Dusan Jovic

Global NMMB

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Zavisa Janjic

Summary and ConclusionsSignificant improvements of regional forecasts still possibleGlobal NMMB competitive with other major medium range forecasting models Unified model offers consistency in applications on various scales and reduced development and maintenance effort ~10 km resolution medium range global forecasts and high resolution climate studies possible with global NMMBLimits of deterministic forecasting have not been reached yetFuture work on the global scales

Issues with radiation cloud-interactionsVariable surface emissivityPrecipitation, near surface variables …Data assimilation

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Zavisa Janjic