Latest thoughts on stochastic kinetic energy backscatter - good and bad

Similar documents
Stochastic methods for representing atmospheric model uncertainties in ECMWF's IFS model

Kinetic energy backscatter for NWP models and its calibration

Stochastic Parametrization and Model Uncertainty

Stochastic parameterization in NWP and climate models Judith Berner,, ECMWF

Representing model error in the Met Office convection permitting ensemble prediction system

DTC & NUOPC Ensemble Design Workshop, Sep 10-13, Boulder, CO

Motivation for stochastic parameterizations

Model error and parameter estimation

Working group 3: What are and how do we measure the pros and cons of existing approaches?

Towards the Seamless Prediction of Weather and Climate

Representing deep convective organization in a high resolution NWP LAM model using cellular automata

Blurring the boundary between dynamics and physics. Tim Palmer, Peter Düben, Hugh McNamara University of Oxford

The ECMWF Hybrid 4D-Var and Ensemble of Data Assimilations

Model error and seasonal forecasting

More Accuracy with Less Precision. Recognising the crucial role of uncertainty for developing high-resolution NWP systems

The Canadian approach to ensemble prediction

ACCESS AGREPS Ensemble Prediction System

Ensemble forecasting and flow-dependent estimates of initial uncertainty. Martin Leutbecher

The Use of a Self-Evolving Additive Inflation in the CNMCA Ensemble Data Assimilation System

A Stochastic Parameterization for Deep Convection

Exploring stochastic model uncertainty representations

TIGGE at ECMWF. David Richardson, Head, Meteorological Operations Section Slide 1. Slide 1

Exploring and extending the limits of weather predictability? Antje Weisheimer

Numerical Weather prediction at the European Centre for Medium-Range Weather Forecasts (2)

Report on the Joint SRNWP workshop on DA-EPS Bologna, March. Nils Gustafsson Alex Deckmyn.

Winds of convection. Tropical wind workshop : Convective winds

Diagnostics of the prediction and maintenance of Euro-Atlantic blocking

Background Error Covariance Modelling

Operational and research activities at ECMWF now and in the future

Nesting and LBCs, Predictability and EPS

Representing model uncertainty using multi-parametrisation methods

MODEL TYPE (Adapted from COMET online NWP modules) 1. Introduction

Focus on parameter variation results

Understanding the local and global impacts of model physics changes

Computational challenges in Numerical Weather Prediction

The Impact of Background Error on Incomplete Observations for 4D-Var Data Assimilation with the FSU GSM

The spectral transform method

The Shallow Water Equations

TC/PR/RB Lecture 3 - Simulation of Random Model Errors

Ensemble of Data Assimilations methods for the initialization of EPS

SPECIAL PROJECT PROGRESS REPORT

Synoptic systems: Flowdependent. predictability

Mesoscale meteorological models. Claire L. Vincent, Caroline Draxl and Joakim R. Nielsen

MOGREPS Met Office Global and Regional Ensemble Prediction System

Recent developments for CNMCA LETKF

New variables in spherical geometry. David G. Dritschel. Mathematical Institute University of St Andrews.

Model Error Diagnosis across Timescales

BALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere. Potential temperature θ. Rossby Ertel potential vorticity

The ECMWF Extended range forecasts

Chapter (3) TURBULENCE KINETIC ENERGY

Internal Wave Generation and Scattering from Rough Topography

Current and future configurations of MOGREPS-UK. Susanna Hagelin EWGLAM/SRNWP, Rome, 4 Oct 2016

Contents. Parti Fundamentals. 1. Introduction. 2. The Coriolis Force. Preface Preface of the First Edition

A Global Atmospheric Model. Joe Tribbia NCAR Turbulence Summer School July 2008

Motivation & Goal. We investigate a way to generate PDFs from a single deterministic run

Medium-range Ensemble Forecasts at the Met Office

Turbulence. 2. Reynolds number is an indicator for turbulence in a fluid stream

Predicting rainfall using ensemble forecasts

A Bayesian approach to non-gaussian model error modeling

Growth of forecast uncertainties in global prediction systems and IG wave dynamics

1 Introduction to Governing Equations 2 1a Methodology... 2

The last few decades have seen a considerable. Stochastic climate theory and modeling

Chapter 3. Stability theory for zonal flows :formulation

Upgrade of JMA s Typhoon Ensemble Prediction System

State and Parameter Estimation in Stochastic Dynamical Models

UNCERTAINTY IN WEATHER AND CLIMATE PREDICTION

Current Issues and Challenges in Ensemble Forecasting

Ensemble Prediction Systems

Lecture 3. Turbulent fluxes and TKE budgets (Garratt, Ch 2)

Stochastic representations of model uncertainties at ECMWF: State of the art and future vision

WWRP working group meeting. on Predictability, Dynamics & Ensemble Forecasting

Stochastic Parametrisations and Model Uncertainty in the Lorenz 96 System

Evaluating Methods to Account for System Errors in Ensemble Data Assimilation

Tangent-linear and adjoint models in data assimilation

Non-local Momentum Transport Parameterizations. Joe Tribbia NCAR.ESSL.CGD.AMP

PUBLICATIONS. Journal of Advances in Modeling Earth Systems

The Canadian Regional Ensemble Prediction System (REPS)

Dynamical impacts of convection and stochastic approaches

The Plant-Craig stochastic Convection scheme in MOGREPS

Comparison between Wavenumber Truncation and Horizontal Diffusion Methods in Spectral Models

2D.4 THE STRUCTURE AND SENSITIVITY OF SINGULAR VECTORS ASSOCIATED WITH EXTRATROPICAL TRANSITION OF TROPICAL CYCLONES

LAM-EPS activities in LACE

2. Outline of the MRI-EPS

Prof. Simon Tett, Chair of Earth System Dynamics & Modelling: The University of Edinburgh

Description of the ET of Super Typhoon Choi-Wan (2009) based on the YOTC-dataset

Recent activities related to EPS (operational aspects)

Challenges in model development

The Spectral Method (MAPH 40260)

Monthly forecasting system

Chapter 1. Introduction

Data Assimilation: Finding the Initial Conditions in Large Dynamical Systems. Eric Kostelich Data Mining Seminar, Feb. 6, 2006

NOTES AND CORRESPONDENCE. On Ensemble Prediction Using Singular Vectors Started from Forecasts

Development of a stochastic convection scheme

EnKF Review. P.L. Houtekamer 7th EnKF workshop Introduction to the EnKF. Challenges. The ultimate global EnKF algorithm

The Madden Julian Oscillation in the ECMWF monthly forecasting system

Modal view of atmospheric predictability

Introduction to Mesoscale Meteorology

Hydrodynamic conservation laws and turbulent friction in atmospheric circulation models

The forecast skill horizon

The Atmospheric Boundary Layer. The Surface Energy Balance (9.2)

Transcription:

Latest thoughts on stochastic kinetic energy backscatter - good and bad by Glenn Shutts DARC Reading University May 15 2013

Acknowledgments ECMWF for supporting this work Martin Leutbecher Martin Steinheimer Alfons Callado Pallares

Table of Contents What is Stochastic Kinetic Energy Backscatter? History behind the use of stochastic backscatter in NWP the search for kinetic energy backscatter using coarsegraining new (simple) convective backscatter scheme summary

What is Stochastic Kinetic Energy Backscatter? random pattern of momentum forcing introduced to represent statistical fluctuations in unresolved momentum transfer pattern is designed to give the correct KE input power spectrum (space & time) strength of the KE input proportional to some measure of model energy dissipation (or generation by parametrized convection) size of the fluctuations set by number of eddies per gridbox (boundary layer eddies ignored for gridlengths > 10 km)

Why do we need it? from a practical viewpoint: to increase ensemble system spread which improves skill to reduce systematic error resulting from missing nonlinear rectification effects -> climate error model error representation in data assimilation a natural component of eddy viscosity parametrizations (Frederiksen and Davies, 1997) or more generally, the governing equations are intrinsically stochastic?

History of stochastic KE backscatter use of random noise in the simulation of boundary layer turbulence. Mason and Thomson, 1992 eddy viscosity and backscatter in 2D turbulence on the sphere. Frederiksen and Davies, 1997 simple isotropic vorticity forcing noise scheme tested in the Met Office Unified Model (1998) ECMWF develop simple parametrization tendency perturbation scheme (Buizza et al, 1999) Stochastic KE Backscatter (SKEB) scheme developed at ECMWF (Shutts, 2005) SKEB scheme developed and operational in Met Office MOGREPS (2006) SKEB implemented in Environment Canada EPS (2007) SKEB implemented in ECMWF IFS (2009)

SKEB - Spectral Kinetic Energy Backscatter Rationale: A fraction of the dissipated energy is backscattered upscale and acts as streamfunction forcing for the resolved-scale flow (Shutts and Palmer 2004, Shutts 2005, Berner et al 2009) Streamfunction forcing is given by: Streamfunction forcing Backscatter ratio Total dissipation rate Pattern generator

SKEB pattern Streamfunction forcing Vorticity forcing

SKEB The total dissipation rate the total dissipation rate is the sum of Numerical dissipation (loss of KE by numerical diffusion + interpolation in semi-lagrangian advection) Dissipation from gravity wave/orographic drag parametrization (not included in Met Office SKEB) Deep convective KE production spatial smoothing required

Impact of stochastic parametrizations in T399 EPS (20 cases) 1. no stochastic physics (red curve) 2. SKEB only (green curve) 3. SPPT only (blue curve) (i.e. the perturbed parametrization tendency scheme) 1. SKEB + SPPT (black curve)

lines with crosses are the error of the ensemble mean uncrossed lines are the spread about the ensemble mean (r.m.s.)

Coarse-graining the vorticity equation in the ECMWF forecast model Use the IFS s spectral-gridpoint transforms to compute terms in the vorticity equation at : Full resolution (e.g. T1279) to be regarded as truth A lower target resolution (e.g. T159) Define error in the target resolution to be the difference Compute the KE input spectrum implied by the error (or residual) forcing function Gives the KE input from scales for 159 < n < 1279

Vorticity equation terms ( ) ζv ψ Vorticity Flux Divergence by the rotational wind (VFD) ( ) ζv χ η V η 4 ζ Vorticity flux divergence by the divergent wind (Rossby Wave Source or RWS) Curl (vertical advection of momentum) called TIP here biharmonic horizontal diffusion - DIFF

mean KE tendency at 250 hpa due to rotational wind contributions in the wavenumber range 159 < n < 1279 from 30 forecasts backscatter biharmonic diffusion KE sink in the sub-synoptic scales (for an actual T159 forecast) KE sink due to exchange with waves having n>159

Work by Thuburn et al (2011) (ECMWF workshop on model error) Use barotropic vorticity equation looked at the effect of spectral truncation w.r.t a reference solution backscatter energy sink from unresolved scales

KE input from SKEB at 250 hpa (using default settings for T159) SKEB Residual fluctuations after averaging 30 cases of the 24 hr-accumulated KE input not realistic! Met Office SKEB chops out waves with n < 6

spectrum of KE dissipation due to biharmonic diffusion versus horizontal resolution

Backscatter by rotational wind vs the sum of RWS and TIP backscatter Dissipative effect of eddies/waves with 159 < n < 1279 through vertical transport. n

Resolution dependence of dissipation rate 0.7 T159 global-mean dissipation rate (Wm -2 ) backscatter energy input 0.5 0.3 0.1 T255 T399 T319 T511 T639 T799 T1279 spectral truncation order (N) 200 600 1000 1400 wavenumber n

summary of current view of SKEB heuristic formulation that doesn t derive from theory independent phases of waves in the spherical harmonic pattern generator current formulations don t scale with resolution properly coarse-graining suggests 2D turbulence backscatter should be small for resolution higher than T159 global-mean numerical dissipation rate drops sharply from T159 to T511 perturbed parametrization tendency scheme seems more effective but questions remain concerning its justification

short-term plan for SKEB in the Met Office move low wavenumber limit for the pattern generator from n=5 to 20 (avoid low wavenumber noisy KE input) include a variant of the vorticity confinement scheme to represent the deterministic component of backscatter and counteract numerical diffusion extend the SKEB formulation to include temperature increments (already successfully tested by Warren Tennant)

why IS EPS spread too small? where does the greatest uncertainty lie in current NWP/climate model? tropical convection? cloud variability e.g. thin medium-level cloud? radiation stress from inertia-gravity waves? convection parametrization is a likely candidate insufficiently sensitive to environmental state KE generated by buoyancy forces is lost PV generation by convective mass transfer deficient? include slantwise convection?

new SKEB scheme based on convective backscatter alone provides divergence or vorticity forcing field n F ς random numbers M c =convective mass flux 1 F n+ 1 = αf n + β r ς ς n ρ dm dz c 0 < α <1 Fˆ ς n ς n+ 1 = = Ο ς [ ] F n n ς + (...) + α fixes the memory time scale O[..] is a spatial transformation operator (like those in image processing) ˆ F n ς F n ς evolve the model vorticity field (done in spectral space in the ECMWF IFS)

impact of Convective Vorticity Forcing (CVF) scheme on spread and ensemble-mean error for T850 in the tropics ECMWF EPS T399 51 members 21 cases

impact of Convective Vorticity Forcing (CVF) scheme on Continuous Ranked Probability Skill Score

preliminary conclusions from convective divergence/vorticity forcing tests non-stochastic convective divergence forcing version can reduce r.m.s. error in T399 forecasts stochastic divergence forcing ineffective in generating spread stochastic convective vorticity forcing is effective at generating spread and improving probabilistic skill

Conclusions: backscatter 2D turbulent backscatter to low wavenumbers evident at T159 though rather weak ECMWF SKEB has a weak wavenumber dependence and crudely counteracts the diffusion KE backscatter to low wavenumbers is dominated by a non-random element that is poorly represented by SKEB (-> remove for n < 20 and use vorticity confinement) SKEB formulation should focus on convective vorticity generation with more realistic representation of associated error structure

Questions and answers