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m ichard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) ierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4) ean de Grandpré (1) lain Robichaud (1) ves Rochon (2) Dr Thomas von Clarmann (5) écillien Charette (1) artin Charron (1) Dr Paul Vaillancourt (1) lexander Kallaur (1) Dr Monique Tanguay (1) an Yang (2) M. Michel Roch (1) the participation of Paul-André Beaulieu (1) , Quentin Errera (3) , Sylvain Ménard (1) , Mike Neish (2) , Bin He (1) and Cathy Xie (1) ronment Canada (3) Belgisch Instituut voor Ru 121 Transcanada Highway (2) 4905 Dufferin Street Institut d’Aéronomie de Belgique (BIRA-IASB) Dorval, Qc, H9P 1J3 Toronto, Ont., M3H 5T4 3, avenue Circulaire CANADA CANADA 1180 Brussels, ork University (5) Institut für Meteorologie und Klimaforsc Department of Earth and Atmospheric Science Universität Karlsruhe 4700 Keele Street, Toronto, Ont. M3J 1P3 Forschungszentrum Karlruhe CANADA GERMANY Le couplage dynamique-chimique en assimilation: Compte rendu du contrat avec l'Agence Spatiale Européenne. Partie II: Assimilation de l'ozone stratosphérique dans GEM
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Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Mar 28, 2015

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Page 1: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

TeamDr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4)

Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Dr Jean de Grandpré (1)

M. Alain Robichaud (1)

Dr Yves Rochon (2) Dr Thomas von Clarmann (5)

M. Cécillien Charette (1)

Dr Martin Charron (1) Dr Paul Vaillancourt (1) M. Alexander Kallaur (1) Dr Monique Tanguay (1)

Dr Yan Yang (2) M. Michel Roch (1)

With the participation of Paul-André Beaulieu(1), Quentin Errera(3), Sylvain Ménard(1), Mike Neish(2) , Bin He(1) and Cathy Xie(1)

Environment Canada (3) Belgisch Instituut voor Ruimte-Aëronomie

(1) 2121 Transcanada Highway (2) 4905 Dufferin Street Institut d’Aéronomie de Belgique (BIRA-IASB)

Dorval, Qc, H9P 1J3 Toronto, Ont., M3H 5T4 3, avenue Circulaire CANADA CANADA 1180 Brussels, BELGIUM

(4) York University (5) Institut für Meteorologie und Klimaforschung

Department of Earth and Atmospheric Science Universität Karlsruhe 4700 Keele Street, Toronto, Ont. M3J 1P3 Forschungszentrum Karlruhe

CANADA GERMANY

Le couplage dynamique-chimique en assimilation: Compte rendu du contrat avec l'Agence Spatiale Européenne. Partie II: Assimilation de l'ozone stratosphérique dans GEM

Page 2: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Introduction

1. Ozone stratosphérique et la question environnementale2 . Cycles d’assimilations a) analyse d’ozone (avec et sans assimilation

chimique) b) Impact radiatif - analyses et prédictabilité

3. Projet Bachus (Richard Ménard)

Page 3: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 4: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Chapman, 1930

Page 5: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 6: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Nitrogen catalytic cycle (Crutzen, 1970)

NO + O3 → NO2 + O2

NO2+ O → NO + O2

______________________Net result: O + O3 → 2 O2

Page 7: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Molina et Rowland(1974)

Page 8: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

From the WMO ozone assessment (2006)

Page 9: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 10: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 11: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 12: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 13: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 14: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

From the WMO ozone assessment (2006)

Page 15: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 16: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

GEM-BACH

Based on GEM-Strato (GEM 3.2.2 – PHY 4.4) Non-orographic Gravity Wave Drag (Hines, 1997) Correlated-K radiation scheme Resolution : L80 120x240 with a lid at 0.1 hPa 45 min time step On-line & interactive ozone and water vapour Ozone climatology: Fortuin & Kelder (1000-0.5 hPa) HALOE (0.5 – 0.1 hPa)

Page 17: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

BASCOE CTM

• 57 chemical species, all advected (S-L)

• Ox, HOx, NOx, ClOx, BrOx and few hydrocarbons

• Source species: N2O, CH4, H2O, CFCs, HCFCs and Halons

• 142 gas-phase reactions; 7 heterogeneous reactions

• 52 photodissociation reactions, J interp from tables

• Photochemical rates are taken from JPL-2002

• Solver generated by KPP (Sandu and Sander, ACP, 2006)

• Numerical method: 3rd – order Rosenbrock

• 45-min timesteps divided into sub-timesteps (can be as short as 1 μs)

Page 18: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

CMC Assimilation System

• 3D-Var FGAT and 4D-var (Gauthier et al., 1999, 2007)

• Use conventional meteorological observations (radiosondes, surface observations, aircraft winds, AMSU radiances)

• ESA project: MIPAS observations (T, O3 , CH4, N2O, HNO3,

NO2)

– Observation and background error statistics:• Univariate background error covariances

• Characterization of the chemistry component done with the Hollingsworth-Lönnberg method

• MIPAS temperatures used as reference for the bias correction of AMSU-a stratospheric channels

Page 19: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 20: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

TOMS GEM-BACH 30 Sep. 2003

Page 21: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 22: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 23: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 24: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Comparaison des prévisions avec les RAOBS.

Hemisphere Nord

O-P 240 hrs

Page 25: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Comparaison des prévisions avec les RAOBS.

Hemisphere Nord

O-P 240 hrs

Page 26: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Comparaison des prévisions avec les RAOBS.

Hemisphere Sud

O-P 240 hrs

Page 27: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Temperature anomaly correlation August 11 - Sept 5, 2003

North Hemisphere (20-90N)

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

0 1 2 3 4 5 6 7 8 9 10

Forecast day

3D dyn - 70 hPa

3D chem - 70 hPa

3D dyn - 50 hPa

3D chem - 50 hPa

3D dyn - 100 hPa

3D chem - 100 hPa

3D dyn - 200 hPa

3D chem - 200hPa

Temperature anomaly correlation August 11 - Sept 5, 2003

South Hemisphere (20-90S)

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

0 1 2 3 4 5 6 7 8 9 10

Forecast day

3D dyn - 70 hPa

3D chem - 70 hPa

3D dyn - 50 hPa

3D chem - 50 hPa

3D dyn - 100 hPa

3D chem - 100 hPa

3D dyn - 200 hPa

3D chem - 200hPa

Page 28: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

Conclusion• The comparison of GEM-BACH prognostic ozone against MIPAS measurements shows

that the chemistry module has an ozone deficit in the upper stratosphere. It increases with height from 10 hPa and reach ~15% at the stratopause.

• The assimilation of ozone using MIPAS measurements produce analyses which are within observation uncertainties in all regions from 100 to 2 hPa. In the stratopause region analyses are largely weighted by the model due to the fact that the ozone photochemical lifetime is much shorter than 6 hr.

• The comparison against independent measurements shows that the radiative feedback from ozone analyses contributes to improve temperature analyses

globally above 3 hPa. However, the radiative impact of ozone analyses can have a negative impact in specific regions as the NH stratopause region.

• The ozone radiative feedback has a significant impact on the model predictability in the lower stratosphere. At 50 hPa where ozone is dynamically driven, ozone assimilation increase the temperature predictability by ~1 day. The comparison against RAOBS in the region shows that ozone interactive forecasts also produce a smaller temperature drift in the region. Above 30 hPa, the ozone photochemical lifetime decrease rapidly and the impact of ozone assimilation is lost after several days. In this region, non-interactive forecasts have a smaller bias against RAOBS in comparison with ozone interactive forecasts.

Page 29: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 30: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

without ozone-radiation interaction

with ozone-radiation interaction

Cross-error covariance Temperature-Ozone

Method: 6-hr differences (CQC)

Radiative time scale (days) - August

Page 31: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)
Page 32: Team Dr Richard Ménard (P.I.) (1) Dr Simon Chabrillat (3) Prof Jack McConnell (4) Dr Pierre Gauthier (1) Dr Dominique Fonteyn (3) Dr Jacek Kaminski (4)

04/10/23 Dynamical and Radiative aspects