Conservative Dynamical Core (CDC)

Slides:



Advertisements
Similar presentations
(c) MSc Module MTMW14 : Numerical modelling of atmospheres and oceans Staggered schemes 3.1 Staggered time schemes.
Advertisements

Günther Zängl, DWD1 Improvements for idealized simulations with the COSMO model Günther Zängl Deutscher Wetterdienst, Offenbach, Germany.
ICONAM ICOsahedral Non-hydrostatic Atmospheric Model -
Page 1© Crown copyright 2007 High-resolution modelling in support of T-REX observations Simon Vosper and Peter Sheridan Met Office, UK T-REX Workshop,
Modeling Fluid Phenomena -Vinay Bondhugula (25 th & 27 th April 2006)
1 NGGPS Dynamic Core Requirements Workshop NCEP Future Global Model Requirements and Discussion Mark Iredell, Global Modeling and EMC August 4, 2014.
A TWO-FLUID NUMERICAL MODEL OF THE LIMPET OWC CG Mingham, L Qian, DM Causon and DM Ingram Centre for Mathematical Modelling and Flow Analysis Manchester.
Deutscher Wetterdienst 1 Status report of WG2 - Numerics and Dynamics COSMO General Meeting , Offenbach Michael Baldauf Deutscher Wetterdienst,
Tutorial 5: Numerical methods - buildings Q1. Identify three principal differences between a response function method and a numerical method when both.
M. Baldauf, DWD Numerical contributions to the Priority Project ‘Runge-Kutta’ COSMO General Meeting, Working Group 2 (Numerics) Bukarest,
A Look at High-Order Finite- Volume Schemes for Simulating Atmospheric Flows Paul Ullrich University of Michigan.
Aktionsprogramm 2003 AP 2003: LMK Properties of the dynamical core and the metric terms of the 3D turbulence in LMK COSMO- General Meeting.
C M C C Centro Euro-Mediterraneo per i Cambiamenti Climatici COSMO General Meeting - September 8th, 2009 COSMO WG 2 - CDC 1 An implicit solver based on.
Hans Burchard Leibniz Institute for Baltic Sea Research Warnemünde How to make a three-dimensional numerical model that.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss News from COSMO COSMO User Workshop 2010.
Comparison of convective boundary layer velocity spectra calculated from large eddy simulation and WRF model data Jeremy A. Gibbs and Evgeni Fedorovich.
Priority project CDC Overview Task 1 COSMO-GM, Sept. 2010, Moscow M. Baldauf (DWD)
A cell-integrated semi-Lagrangian dynamical scheme based on a step-function representation Eigil Kaas, Bennert Machenhauer and Peter Hjort Lauritzen Danish.
Status report of WG2 - Numerics and Dynamics COSMO General Meeting , Rome Michael Baldauf Deutscher Wetterdienst, Offenbach, Germany.
M. Baldauf (DWD)1 SMC-meeting, Bologna, 05/06. Feb with verification extensions for SMC-teleconf., 16. April 2014 Michael Baldauf (FE13) Proposed.
Michał Ziemiański, Marcin Kurowski, Zbigniew Piotrowski, Bogdan Rosa and Oliver Fuhrer Institute of Meteorology and Water Management (IMGW), MeteoSwiss.
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Atmosphere at rest experiments with the latest COSMO version.
Deutscher Wetterdienst 1FE 13 – Linear solutions of flow over mountains COSMO General Meeting WG2 'Numerics and Dynamics' Michael.
COSMO Sibiu 2013 Matthias Raschendorfer Towards Separated Turbulence Interacting with Circulations (STIC):
The equations of motion and their numerical solutions II by Nils Wedi (2006) contributions by Mike Cullen and Piotr Smolarkiewicz.
24-28 Sept. 2012Baldauf, Reinert, Zängl (DWD)1 Michael Baldauf, Daniel Reinert, Günther Zängl (DWD, Germany) PDEs on the sphere, Cambridge, Sept.
Numerical simulations of inertia-gravity waves and hydrostatic mountain waves using EULAG model Bogdan Rosa, Marcin Kurowski, Zbigniew Piotrowski and Michał.
Deutscher Wetterdienst 1FE 13 – An Improved Third Order Vertical Advection Scheme for the Runge-Kutta Dynamical Core Michael Baldauf (DWD) Bill.
Implementation of Grid Adaptation in CAM: Comparison of Dynamic Cores Babatunde J. Abiodun 1,2 William J. Gutowski 1, and Joseph M. Prusa 1,3 1 Iowa State.
M. Baldauf, U. Blahak (DWD)1 Status report of WG2 - Numerics and Dynamics COSMO General Meeting Sept. 2013, Sibiu M. Baldauf, U. Blahak (DWD)
Bogdan Rosa 1, Marcin Kurowski 1, Damian Wójcik 1, and Michał Ziemiański 1 Acknowledgements: Oliver Fuhrer 2, Zbigniew Piotrowski 1,3 1. Institute of Meteorology.
1 The Nonhydrostatic Icosahedral (NIM) Model: Description and Potential Use in Climate Prediction Alexander E. MacDonald Earth System Research Lab Climate.
Matthias Raschendorfer DWD Recent extensions of the COSMO TKE scheme related to the interaction with non turbulent scales COSMO Offenbach 2009 Matthias.
10-13 Sept. 2012M. Baldauf (DWD)1 Michael Baldauf Deutscher Wetterdienst, Offenbach, Germany Priority Project "Conservative Dynamical Core" Final report.
Gas-kineitc MHD Numerical Scheme and Its Applications to Solar Magneto-convection Tian Chunlin Beijing 2010.Dec.3.
1 Priority Project CDC Task 2: The compressible approach COSMO-GM, , Moscow Pier Luigi Vitagliano (CIRA), Michael Baldauf (DWD)
Bogdan Rosa 1, Marcin Kurowski 1 and Michał Ziemiański 1 1. Institute of Meteorology and Water Management (IMGW), Warsaw Podleśna, 61
Standardized Test Set for Nonhydrostatic Dynamical Cores of NWP Models
Mass Coordinate WRF Dynamical Core - Eulerian geometric height coordinate (z) core (in framework, parallel, tested in idealized, NWP applications) - Eulerian.
1 Reformulation of the LM fast- waves equation part including a radiative upper boundary condition Almut Gassmann and Hans-Joachim Herzog (Meteorological.
Governing Equations II
Modeling orographic flows on unstructured meshes Piotr Smolarkiewicz, National Center for Atmospheric Research*, USA; Joanna Szmelter, Loughborough University,
Federal Department of Home Affairs FDHA Federal Office of Meteorology and Climatology MeteoSwiss Component testing of the COSMO model’s turbulent diffusion.
Vincent N. Sakwa RSMC, Nairobi
Development of an Atmospheric Climate Model with Self-Adapting Grid and Physics Joyce E. Penner 1, Michael Herzog 2, Christiane Jablonowski 3, Bram van.
Deutscher Wetterdienst Flux form semi-Lagrangian transport in ICON: construction and results of idealised test cases Daniel Reinert Deutscher Wetterdienst.
Deutscher Wetterdienst 1FE 13 – Working group 2: Dynamics and Numerics report ‘Oct – Sept. 2008’ COSMO General Meeting, Krakau
Performance of a Semi-Implicit, Semi-Lagrangian Dynamical Core for High Resolution NWP over Complex Terrain L.Bonaventura D.Cesari.
Computational Modeling of 3D Turbulent Flows With MC2 Claude Pelletier Environment Canada MSC / MRB.
Representing Effects of Complex Terrain on Mountain Meteorology and Hydrology Steve Ghan, Ruby Leung, Teklu Tesfa, PNNL Steve Goldhaber, NCAR.
Priority project CDC Task 1.4: Choice of the anelastic equation system and Milestone 3.2: Suitability of fundamental approximations PP CDC-Meeting, ,
A revised formulation of the COSMO surface-to-atmosphere transfer scheme Matthias Raschendorfer COSMO Offenbach 2009 Matthias Raschendorfer.
Operational COSMO of MeteoSwiss
National Taiwan University, Taiwan
Convection-Dominated Problems
Kazushi Takemura, Ishioka Keiichi, Shoichi Shige
Development of nonhydrostatic models at the JMA
A TWO-FLUID NUMERICAL MODEL OF THE LIMPET OWC
Status of the COSMO-Software and Documentation
“Consolidation of the Surface-to-Atmosphere Transfer-scheme: ConSAT
Multiscale aspects of cloud-resolving simulations over complex terrain
Perturbation equations for all-scale atmospheric dynamics
Outlines of NICAM NICAM (Nonhydrostatic ICosahedral Atmospheric Model)
Terrain-following coordinates over steep and high orography
Models of atmospheric chemistry
COSMO-GM Rome, WG-2 Meeting, Sept. 5, 2011
Michael Baldauf Deutscher Wetterdienst, Offenbach, Germany
Bogdan Rosa1, Marcin Kurowski1, Damian Wójcik1,
Conservative Dynamical Core (CDC)
Semi-implicit predictor-corrector methods for atmospheric models
Presentation transcript:

Conservative Dynamical Core (CDC) COSMO Priority Project (2009 – 2011) Conservative Dynamical Core (CDC) Detlev Majewski for Michael Baldauf Deutscher Wetterdienst, Offenbach, Germany

Aims of the CDC priority project conservation properties of the dynamical core (Thuburn, 2008, JCP): mass !!! most important energy !! momentum probably increasing importance for smaller scales tracers !! important at least in convection resolving models should be able to handle steep orography and of course overall: accuracy efficiency stability

Current dynamical cores of COSMO model (Leapfrog, RK) have no conservation properties for the dynamic variables mass, energy, momentum Possible causes for limited use in steep terrain: Fast waves: not vertical implicit for metric terms (would go beyond tri-diagonal matrices) Metric tensor identities probably not fulfilled (Task 2.1 in CDC) Tracer advection: Bott-scheme is not multi-dimensional

COSMO Priority Project Conservative Dynamical Core (CDC) Task 1: The anelastic (EULAG) approach Testing the EULAG dynamical core as a prospective dynamical core of COSMO Task 1.1: Idealised tests of the EULAG dynamical core Simulate 2D and 3D idealized flows (flow over mountains, valley flows, ...) Compare with COSMO results, laboratory flows and analytic solutions. Test cases are defined in Task 3.1. This task should give a first insight into the capabilities of the EULAG dynamical core and its possible advantages towards the current COSMO model.

case studies for different weather regimes real / idealised inflow Task 1.2: Tests of the EULAG dynamical core for realistic flows over the Alpine topography case studies for different weather regimes real / idealised inflow with realistic orography (Alpine area, containing deep valleys) resolution ranging from 2.2 km, 1.1 km to 0.25 km No physics parameterizations! Perform EULAG simulations and compare with COSMO/RK and COSMO/Leapfrog. Test computational efficiency and scalability of EULAG core Adapt the implicit solver to the model resolution and orography. Due to the possibility of EULAG to use structured grids with an arbitrary distribution of horizontal grid points, the same grid as in COSMO with a rotated pole can be used. To perform COSMO/RK-runs probably improvements in the RK-scheme are needed. The simulation time should be decided by scale considerations and lies at about 2 days.

Apply simplified parameterizations of basic subgrid processes: Task 1.3: Tests of the EULAG dynamical core for realistic flows over the Alpine topography with simplified physics parameterisation Simulate realistic flows over the Alpine topography, with resolution ranging from 2.2, 1.1 km to 0.25 km Apply simplified parameterizations of basic subgrid processes: Moist processes: only simulated on explicit grid (i.e. no shallow convection parameterization, no moist turbulence) Simple microphysics (Kessler-scheme) in both models Turbulent diffusion with a one-equation (TKE)-model (not necessarily the same in both models) Simplified surface fluxes Compare results between EULAG and COSMO/RK and COSMO/Leapfrog simulations. Investigate the possible technical implications of an implementation of the EULAG core into COSMO (e.g. 1) EULAG is written for A- and B-grid, COSMO is C-grid. 2) EULAG is parallelized differently than COSMO)

Task 1.4: Choice of the anelastic equation system Several different soundproof sets of equations have been published and are available in EULAG. The possible errors implied should be investigated and a recommendation for the best approximation to use for NWP should be given. Special focus should be given to the conservation of mass (i.e. ambiguity in the determination of the full pressure field), flows with finite-amplitude and non-linear perturbations with respect to the base state profile and the presence of large vertical gradients in the temperature field (i.e. inversions, tropopause). The other conservation properties (i.e. which mass/energy variables are conserved by which equation sets) should also be investigated. Test the validity of conservation properties for mass, momentum and energy (possibly others like potential vorticity) in EULAG and COSMO. In COSMO a testing tool for conservation properties is available. Implementation of the Durran equations.

Task 2: The compressible approach Task 2.1: Metric tensor identities Clear up the role of the ‘metric tensor identities’ (Smolarkiewicz, Prusa, 2005) and if they can empower the model to handle steep orography. Can they be applied directly to improve the current COSMO model formulation? Task 2.3: Fully 3D, i.e. non-direction splitted, conservative advection scheme Implement a fully 3D, i.e. non-direction splitted, conservative advection scheme into COSMO, e.g. MPDATA from the EULAG model. Test this scheme with prescribed velocity fields in mountainous terrain, to show the transport properties also in terrain-following coordinates.

Task 2.2: Complete FV-solver for the EULER equations Starting point: Jameson (1991) Am. Inst. Aeronaut. Astron. Finite volume discretization of the Euler-equations  conservation of mass, momentum, energy(?) Implicit scheme  helps in steep orography This dynamical core is more in the state of an early-development stage model, therefore implementation into COSMO can be started relatively early after answering the most basic questions. Spatial scheme: Central schemes with added artificial viscosity and upwind schemes can be adopted for spatial discretisation. Higher order schemes are more accurate, but lower order schemes at higher resolution could turn out to be more efficient, particularly when implemented on vector hardware architectures.

Task 3: Assessment of dynamical cores Task 3.1: Maintenance of idealized test cases Several idealised test cases are already available. Carry out these tests ‘at the push of a button’ and compare automatically with reference solutions. 0. advection test + nonlinear dyn. (Schär et al. (2002)) Atmosphere at rest (G. Zängl (2004) MetZ) Cold bubble (Straka et al. (1993)) (unstationary density flow) 3. Mountain flow tests (stationary, orographic flows) 3.1 Schaer et al. (2002), sect. 5b (for EULAG cite Wedi ,Smolarkiewicz (2004)) 3.2 Bonaventura (2000) JCP, e.g. linear solution developed (Baldauf, 2008a) 4. Linear Gravity waves (Skamarock, Kemp (1994), Giraldo (2008)) 5. Warm bubble (Robert (1993), Giraldo (2008)) 6. Moist, warm bubble (Weisman, Klemp (1982) MWR) Probably it will be difficult to define idealised test cases which address all the issues of steep terrain (those could be very special mountain/valley distributions and inflow/stratification combinations). Nevertheless such additional idealised cases should be added to this list, too. Deliverables: all test cases including src_artifdata.f90, NAMELIST-parameters, run-scripts and scripts for evaluating and automatic reporting are delivered with the source code of the COSMO-model. Estimated resources: for technical work: 0.2 FTE by P. Prohl (DWD), 0.1 FTE by M. Baldauf (DWD), 0.1 FTE by O. Fuhrer (MeteoSwiss)

Test of the dynamical core: density current (Straka et al., 1993) ‘ after 900 s. (Reference) by Straka et al. (1993) COSMO with RK3 + upwind 5th order COSMO with RK2 + upwind 3rd order

Mountain flow (Schär et al. (2002) MWR) 12 km ~ z / 300m a = 5 km / l=4 km h= 25 m u=10 m/s T(z=0)=288 K N=0.01 1/s dx=500 m dz=300 m Comparison with analytic solution (black lines) from Baldauf (2008) COSMO-Newsl.

Task 3.2 Collection and maintenance of semi-idealized test cases A test bed with some semi-idealized (quasi-realistic) tests (steep mountains, valley flows, deep convection, …) should be maintained also with a documentation about the specific weather situation and what should be expected by the simulation. Input format: GRIBs from COSMO-model (e.g. 7 km) for the Alpine region. A competition between the current and newly developed dynamical cores by these tests will be essential to decide the further direction of developments. For a broad acceptance it is advisable to include several groups in these tests. This task collects the different approaches and serves to assess the properties of conservation, accuracy, and efficiency.

Task 3.3: Decision tree for Steering Committee In former projects concerning the development of a new dynamical core it has been proven to be rather difficult to decide about the continuation or the abort of the project, due to a lack of clear decision criteria. Here such a decision tree (a cascade of benchmarks) shall be set up. Task 3.4: Verification of the whole model A verification of the model by real observation data (Synop, upper air, radar data). Probably such a verification is only useful for a model with the full set of parameterizations.