the ecmwf approach to ensemble prediction

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The ECMWF Approach to Ensemble Prediction Tim Palmer University of Oxford, ECMWF.

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Page 1: The ECMWF Approach to Ensemble Prediction

The ECMWF Approach to Ensemble Prediction

Tim Palmer

University of Oxford, ECMWF.

Page 2: The ECMWF Approach to Ensemble Prediction

With particular thanks to

Jan Barkmeijer, Roberto Buizza, Philippe Chapelet, Dennis Hartmann, Renate Hagedorn, Martin Leutbecher, Jean-Francois Mahfouf, Martin Miller, Franco Molteni, Robert Mureau, Thomas Petroliagis, Kamal Puri, David Richardson, Glenn Shutts, Stefano Tibaldi, Joe Tribbia….

… and all of ECMWF RD and OD

Page 3: The ECMWF Approach to Ensemble Prediction

With thanks to Met Office staff

Doug Mansfield, James Murphy

1985: The First Semi-Operational Real-Time Ensemble Forecast

Page 4: The ECMWF Approach to Ensemble Prediction

Cf Miyakoda et al, 1982

Page 5: The ECMWF Approach to Ensemble Prediction

PNA+

PNA-

DAY 4 DAY 2 DAY 9 DAY 30

Integrations with a Barotropic Vorticity Equation Model

Page 6: The ECMWF Approach to Ensemble Prediction

If eigenvectors are not normal (operator not self-

adjoint), perturbation growth is not bounded by the

dominant eigenvalue

n0 = ax1 -bx2

g = 1cosq

q

g -PNA >> g +PNA

Zhang c. 1989

Page 7: The ECMWF Approach to Ensemble Prediction

From Buizza and Palmer, 1995

Page 8: The ECMWF Approach to Ensemble Prediction

Use SVs to initialise EPS. Why?

1. Meteorologically balanced perturbations

2. Initial-time perturbations with amplitudes focussed on sub-synoptic wavenumbers where analysis errors (observation error and model error) are likely to be significant, and final-time perturbations on synoptic and smaller wavenumbers where forecast error is dominant.

3. Perturbations with growth rates that would compensate for the overly dissipative nature of the model at large wavenumbers.

4. Since we don’t have a good quantification of initial error (esp impact of model error on initial error - see below), focussing on potential worse-case perturbations is no bad thing. The main problem with ensemble prediction (to the present day) is underdispersion -overconfidence.

Page 9: The ECMWF Approach to Ensemble Prediction
Page 10: The ECMWF Approach to Ensemble Prediction
Page 11: The ECMWF Approach to Ensemble Prediction

But now …. Perturbations produced by Ensemble Data Assimilation (EDA)…. Surely

no need for SVs any more??

Page 12: The ECMWF Approach to Ensemble Prediction

Simon Lang: Personal Communication

Page 13: The ECMWF Approach to Ensemble Prediction

Stochastic Physics

Page 14: The ECMWF Approach to Ensemble Prediction

Workshop on New

Insights and Approaches

to Convective

Parametrization

4-7 November 1996

Probability of an “on”cell

proportional to CAPE and

number of adjacent “on”

cells – “on” cells feedback

to the resolved flow

Page 15: The ECMWF Approach to Ensemble Prediction

Stochastically Perturbed Parameterisation Tendencies (SPPT)

A Holistic Scientifically Justified Approach to Representing Model Uncertainty

• Operational scheme in ECMWF’s ensemble prediction system

• Perturbations to total parametrised tendency of physical processes with multiplicative noise

for X={u,v,T,q}

• r is a uni-variate random number described through a spectral pattern generator which is smooth in space and time

• Spectral coefficients of r are described with an AR(1) process

• Gaussian distribution, truncated at ±2s

Page 16: The ECMWF Approach to Ensemble Prediction
Page 17: The ECMWF Approach to Ensemble Prediction
Page 18: The ECMWF Approach to Ensemble Prediction

0 1 2 3 4 5 6 7 8 9 100

5

10

15

lead time

en

se

mble

sp

rea

d

L63 st

L63 det

Spread L63 and L63 stoch.

Spread decreases (not increases!) with stochastic noise

Kwasniok, 2014

s=0

s=3.2

s=8

Page 19: The ECMWF Approach to Ensemble Prediction

0 10 20 30 40 50 60 70 80

m

12

34

56

78

9Forecast Day

Mean m

ethod: standard | Population: 691,688,686,685,682,681,679,2*671,670 (averaged)

oper_an ti enfo prod

Date: 20160101 00UTC to 20161231 12UTC

NHem Extratropics (lat 20.0 to 90.0, lon -180.0 to 180.0)

500hPa geopotential

Annual mean 2016

spread ECMW

F

EMrm

se ECMW

F

spread UKMO

EMrm

se UKMO

spread NCEP

EMrm

se NCEP

Martin Janousek: Personal Communication

ECMWF EPS spread/skill better balanced than other operational ensembles.

Page 20: The ECMWF Approach to Ensemble Prediction

The Future: More Interaction Between SVs and SPPT?

Use EDA to set SV amplitudes regionally?

Page 21: The ECMWF Approach to Ensemble Prediction

Ensemble Size vs Resolution

• We must not drop below 50 members. Needed to optimiseprobabilistic scores for high-impact weather (see Martin Leutbecher’s talk).

• Two complementary routes to developing high-resolution (e.g. 5km) 50 member ensembles….

Page 22: The ECMWF Approach to Ensemble Prediction

Stochastic Parametrisation

Triangular

Truncation

Partially Stochastic

Double precision

Single precision

Half precision?

Quarter precision?

1. State-dependent precision….

… a job for scientists

Page 23: The ECMWF Approach to Ensemble Prediction

25/08/17 00:00850hP wind speedT511L91

n = 0 52-bit significand

0 < n £160 11-bit significand

160<n £ 320 9-bit significand

320<n £ 511 7-bit significand

Matthew Chantry, Oxford – Peter Düben, ECMWF.

HurricaneHarvey

Page 24: The ECMWF Approach to Ensemble Prediction

2. Make the case for much greater computing capability, so ECMWF can remain the World No 1.

… a job for management

Page 25: The ECMWF Approach to Ensemble Prediction

Extra Slides

Page 26: The ECMWF Approach to Ensemble Prediction

The application of ensemble ideas to monthly (and seasonal) forecasting was not controversial.

What was more controversial is that ensemble forecast methods should be developed within what was referred to as “the limit of deterministic predictability”. Medium-range ensemble forecasting was treated with scepticism.

Instead of probabilistic prediction, the thought at the time was that we should be trying to “forecast the forecast skill” of the deterministic forecast.

This turned out to be a forlorn hope, though it led to some very important scientific spin offs, such as how to perturb the initial conditions in a medium-range ensemble forecast.

Page 27: The ECMWF Approach to Ensemble Prediction

Mesoscale Area of Interest1-km AGL Reflect. >40 dBZ

20160502-2016060300Z cycle; fh013-030

40-km Radius of Influence10 grid-point Gaussian smoothing parameter

Neighborhood Reflectivity Verification: CLUE Comparison to SSEO: Reliability

SSEO: 7-member multi-model

CLUE_M10: 5 ARW, 5 NMMB

CAPSEnKF: 9-member ARW

NCAREnKF:10-member ARW

no resolution

NOAA Hazardous Weather Testbed Spring

Forecasting Experiment (I. Jirak and A. Clark)

Page 28: The ECMWF Approach to Ensemble Prediction

x '(t) = L(t,t0 ) ¢x (t0 )

Let || x || denote the perturbation's energy.

Let (x;y) denote the corresponding inner product.

Then

maxx(t0 )¹0 (|| x(t) || / || x(t0 )) = s 1

where s1 is the largest eigenvalue for

(LL*)v i (t) = s i

2v i (t)

i.e. the largest singular value of L

The corresponding singular vectors, ranked by the size of s i

define the fastest growing perturbations

Page 29: The ECMWF Approach to Ensemble Prediction

“If more realistic models with many

thousand variables also have the

property that a few of the eigenvalues

of AAT are much larger than the

remaining, a study based upon a small

ensemble of initial errors should..give a

reasonable estimate of the growth rate

of random error.” Lorenz (1965)

Lorenz (1965): A Study of the Predictability of a 28-Variable

Atmospheric Model, Tellus.