Slimane BEKKI, LATMOS (Thank you to Daniel Jacob great website, - - PowerPoint PPT Presentation

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Slimane BEKKI, LATMOS (Thank you to Daniel Jacob great website, - - PowerPoint PPT Presentation

CHEMISTRY-TRANSPORT AND CHEMISTRY-CLIMATE MODELLING Slimane BEKKI, LATMOS (Thank you to Daniel Jacob great website, Harvard Univ.) PLAN 1/ Some basics about atmospheric modelling 2/ From simple (box) to complex chemistry- climate models 3/


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SLIDE 1

CHEMISTRY-TRANSPORT AND CHEMISTRY-CLIMATE MODELLING

Slimane BEKKI, LATMOS (Thank you to Daniel Jacob great website, Harvard Univ.)

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SLIDE 2

1/ Some basics about atmospheric modelling 2/ From simple (box) to complex chemistry- climate models 3/ Use of models in the analysis of observations

PLAN

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SLIDE 3

HOW TO MODEL ATMOSPHERIC COMPOSITION?

Solve continuity equation for chemical mixing ratios Ci(x, t) Fires Land biosphere Human activity Lightning Ocean Volcanoes Transport Eulerian form:

i i i i

C C P L t        U

Lagrangian form:

i i i

dC P L dt  

U = wind vector Pi = local source

  • f chemical i

Li = local sink

Chemistry Aerosol microphysics

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SLIDE 4

HOW TO SOLVE CONTINUITY EQUATION?

Define problem of interest Design model; make assumptions needed to simplify equations and make them solvable Evaluate model with

  • bservations

Apply model: make hypotheses, predictions Improve model, characterize its error The atmospheric evolution of a species X is given by the continuity equation This equation cannot be solved exactly e need to construct model (simplified representation of complex system) Design

  • bservational

system to test model

[ ] ( [ ])

X X X X

X E X P L D t        U

local change in concentration with time transport (flux divergence; U is wind vector) chemical production and loss (depends on concentrations

  • f other species)

emission Deposition (wet, dry)

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SLIDE 5

SIMPLEST MODEL: ONE-BOX MODEL

Inflow Fin Outflow Fout

X

E Emission Deposition D Chemical production P L Chemical loss Atmospheric “box”; spatial distribution of X within box is not resolved

  • ut

Atmospheric lifetime: m F L D    

Fraction lost by export:

  • ut
  • ut

F f F L D   

Lifetimes add in parallel:

export chem dep

1 1 1 1

  • ut

F L D m m m          

Loss rate constants add in series:

export chem dep

1 k k k k      Mass balance equation: sources - sinks

in

  • ut

dm F E P F L D dt       

 

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SLIDE 6

NO2 has atmospheric lifetime ~ 1 day: strong gradients away from combustion source regions

Satellite observations of tropospheric NO2 columns

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SLIDE 7

CO has atmospheric lifetime ~ 2 months: mixing around latitude bands

Satellite observations of CO mixing ratio at 850 hPa

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SLIDE 8

CO2 has atmospheric lifetime ~ 100 years: global mixing, very weak gradients

Assimilated observations of CO2 mixing ratio

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SLIDE 9

SIMPLEST MODEL: ONE-BOX MODEL

Inflow Fin Outflow Fout

X

E Emission Deposition D Chemical production P L Chemical loss Atmospheric “box”; spatial distribution of X within box is not resolved

  • ut

Atmospheric lifetime: m F L D    

Fraction lost by export:

  • ut
  • ut

F f F L D   

Lifetimes add in parallel:

export chem dep

1 1 1 1

  • ut

F L D m m m          

Loss rate constants add in series:

export chem dep

1 k k k k      Mass balance equation: sources - sinks

in

  • ut

dm F E P F L D dt       

 

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SLIDE 10

SPECIAL CASE: SPECIES WITH CONSTANT SOURCE & 1st ORDER SINK & NO TRANSPORT

  • > ANALYTICAL SOLUTION

( ) (0) (1 )

kt kt

dm S S km m t m e e dt k

 

     

Steady state solution (dm/dt = 0) Initial condition m(0) Characteristic time  = 1/k for

  • reaching steady state
  • decay of initial condition

If S, k are constant over t >> , then dm/dt g 0 and mg S/k: quasi steady state

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SLIDE 11

EXAMPLE : GLOBAL BOX MODEL FOR CO2 (Pg C yr-1) SIMPLE CASE: NO ATMOSPHERIC CHEMISTRY & NO TRANSPORT (GLOBAL)

IPCC [2001] IPCC [2001]

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SLIDE 12

PUFF MODEL: FOLLOW AIR PARCEL MOVING WITH WIND

CX(xo, to) CX(x, t) wind In the moving puff,

X

dC E P L D dt    

…no transport terms! (they’re implicit in the trajectory) Application to the chemical evolution of an isolated pollution plume:

CX CX,b

,

( )

X dilution X X b

dC E P L D k C C dt      

In pollution plume,

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SLIDE 13

TWO-BOX MODEL defines spatial gradient between two domains m1 m2 F12 F21

Mass balance equations:

1 1 1 1 1 12 21

dm E P L D F F dt      

If mass exchange between boxes is first-order:

1 1 1 1 1 12 1 21 2

dm E P L D k m k m dt      

e system of two coupled ODEs (or algebraic equations if system is assumed to be at steady state) (similar equation for dm2/dt)

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SLIDE 14

EULERIAN MODELS PARTITION ATMOSPHERIC DOMAIN INTO GRIDBOXES

Solve numerically continuity equation for individual grid-boxes

  • Detailed chemical/aerosol models can

presently afford -106 gridboxes

  • In global models, this implies a

horizontal resolution of ~ 1o (~100 km) in horizontal and ~ 1 km in vertical This discretizes the continuity equation in space

  • Chemical Transport Models (CTMs) use external meteorological data as input
  • General Circulation Models (GCMs) compute their own meteorological fields
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SLIDE 15

JUST AN INTERVAL ON LAGRANGIAN MODELS

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SLIDE 16

IN EULERIAN APPROACH, DESCRIBING THE EVOLUTION OF A POLLUTION PLUME REQUIRES A LARGE NUMBER OF GRIDBOXES

Fire plumes over southern California, 25 Oct. 2003 A Lagrangian “puff” model offers a much simpler alternative

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SLIDE 17

LAGRANGIAN APPROACH: TRACK TRANSPORT OF POINTS IN MODEL DOMAIN (NO GRID)

UDt U’Dt

  • Transport large number of points with trajectories

from input meteorological data base (U) + random turbulent component (U’) over time steps Dt

  • Points have mass but no volume
  • Determine local concentrations as the number of

points within a given volume

  • Nonlinear chemistry requires Eulerian mapping at

every time step (semi-Lagrangian) PROS over Eulerian models:

  • no Courant number restrictions
  • no numerical diffusion/dispersion
  • easily track air parcel histories
  • invertible with respect to time

CONS:

  • need very large # points for statistics
  • inhomogeneous representation of domain
  • convection is poorly represented
  • nonlinear chemistry is problematic

position to position to+Dt

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SLIDE 18

LAGRANGIAN RECEPTOR-ORIENTED MODELING

Run Lagrangian model backward from receptor location, with points released at receptor location only

  • Efficient cost-effective quantification of source

influence distribution on receptor (“footprint”) backward in time

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SLIDE 19

BACK ON EULERIAN MODELS…

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SLIDE 20
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SLIDE 21
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SLIDE 22
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SLIDE 23

OPERATOR SPLITTING IN EULERIAN MODELS

i i i TRANSPORT LOCAL

C C dC t t dt                  

… and integrate each process separately over discrete time steps:

( ) (Local)•(Transport) ( )

i

  • i
  • C t

t C t  D  

  • Split the continuity equation into contributions from transport and local terms:

Transport advection, convection: Local chemistry, emission, deposition, aerosol processes: (

i i TRANSPORT i i LOCAL

dC C dt dC P dt                   U ) ( )

i

L  C C

These operators can be split further:

  • split transport into 1-D advective and turbulent transport for x, y, z

(usually necessary)

  • split local into chemistry, emissions, deposition (usually not necessary)

Reduces dimensionality of problem

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SLIDE 24

SPLITTING THE TRANSPORT OPERATOR

  • Wind velocity U has turbulent fluctuations over time step Dt:

( ) '( ) t t   U U U

Time-averaged component (resolved) Fluctuating component (stochastic)

1 ( )

i i i xx

C C C u K t x x x            

  • Further split transport in x, y, and z to reduce dimensionality. In x direction:

( , , ) u v w  U

  • Split transport into advection (mean wind) and turbulent components:

1

i i i

C C C t          U K

air density turbulent diffusion matrix    K

advection turbulence (1st-order closure) advection

  • perator

turbulent

  • perator
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SLIDE 25

SOLVING THE EULERIAN ADVECTION EQUATION

  • Equation is conservative: need to avoid

diffusion or dispersion of features. Also need mass conservation, stability, positivity…

  • All schemes involve finite difference

approximation of derivatives : order of approximation → accuracy of solution

  • Classic schemes: leapfrog, Lax-Wendroff,

Crank-Nicholson, upwind, moments…

  • Stability requires Courant number uDt/Dx < 1

… limits size of time step

  • Addressing other requirements (e.g., positivity)

introduces non-linearity in advection scheme

i i

C C u t x      

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SLIDE 26

LOCAL (CHEMISTRY) OPERATOR: solves ODE system for n interacting species

 

1, i n 

1

( ) ( ) ( ,... )

i i i n

dC P L C C dt    C C C

System is typically “stiff” (lifetimes range over many orders of magnitude) → implicit solution method is necessary. Needs to be conservative and fast

  • Simplest method: backward Euler. Transform into system of n algebraic

equations with n unknowns

 

( ) ( ) ( ( )) ( ( )) 1,

i

  • i
  • i
  • i
  • C t

t C t P t t L t t i n t  D    D   D  D C C

( )

  • t

t  D C

Solve e.g., by Newton’s method. Backward Euler is stable, mass-conserving, flexible (can use other constraints such as steady-state, chemical family closure, etc… in lieu of DC/Dt ). But it is expensive. Most 3-D models use higher-order implicit schemes such as the Gear method. For each species

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SLIDE 27

SPECIFIC ISSUES FOR AEROSOL CONCENTRATIONS

  • A given aerosol particle is characterized by its size, shape, phases, and

chemical composition – large number of variables!

  • Aerosol size distribution in a model is either decomposed in size bins

(and so as many tracers) or only its moments (integrals over size) are treated by the model (assuming a certain shape for the size distribution, typically a log-normal).

  • If evolution of the size distribution is not resolved, continuity equation

for aerosol species can be applied in same way as for gases

  • Simulating the evolution of the aerosol size distribution requires

inclusion of nucleation/growth/coagulation terms in Pi and Li, and size characterization either through size bins or moments. Typical aerosol size distributions by volume nucleation condensation coagulation

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SLIDE 28

INFLUENCE DU SCENARIO GES SUR LA COUCHE D’O3

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SLIDE 29
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SLIDE 30
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SLIDE 31

“INTERACTIVE” ATMOSPHERIC CHEMICAL COMPOSITION

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SLIDE 32

MOVIE

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SLIDE 33

MODEL PROJECTIONS

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SLIDE 34

An other motivation …

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SLIDE 35

INFLUENCE OF CO2 ON STRATOSPHERIC O3

WMO, 1998

Temporal evolution of column O3

Projections by 2-D chemistry-climate model (Cambridge) Halogen  Halogen 

CO2  CO2 constant

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SLIDE 36

INFLUENCE OF IPCC GHG SCENARIOS ON O3 Temporal evolution of column ozone

Projections: multi-model mean (chemistry-climate) Different colours: different scenarios of greenhouse gases evolution (GHG: CO2, CH4, N2O) Eyring et al., 2014

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SLIDE 37

INFLUENCE OF STRATOSPHERIQUE O3 ON CLIMATE

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SLIDE 38

ON THE USE OF CTM IN THE ANALYSIS OF OBSERVATIONS

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SLIDE 39

TIME EVOLUTION OF HCl COLUMN (INDICATOR OF STRATOSPHERRIC CHLORINE LOADING) AT JUNGFRAUJOCH (47°N)

What is going on between 2004 and 2010?

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SLIDE 40

STRATOSPHERIC HCl ANOMALY DUE TO ATMOSPHERIC CIRCULATION CHANGES

CTM varying dyn. CTM fixed dynamics

JUNGFRAUJOCH NY-ALESUND

Anomaly found at all NH sites except tropics Nothing at SH sites

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SLIDE 41

ANTARCTIC OZONE MEASUREMENT STATIONS

(SAOZ, DOBSON, BREWER, DOAS)

How can we estimate ozone losses from these observations?

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SLIDE 42

TIME EVOLUTION OF PARAMETERS USED TO ESTIMATE OZONE LOSSES AT DDU IN 2007

Ozone loss = Measured ozone – CTM passive ozone

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SLIDE 43

TIME EVOLUTION OF VORTEX OZONE LOSS ESTIMATED AT DIFFERENT STATIONS

solid black line: mean ozone loss

Kuttippurath et al., ACP, 2010

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SLIDE 44

Anomalies relative to the 1964‐1978 reference period

Black (ODS): CTM with changing ODS Blue (cODS): CTM with ODS held constant at 1960s values Yellow: ground-based observations Good agreement between ODS CTM and observations. Attribution (halogen-induced loss) based on observations alone is difficult and risky

TIME EVOLUTION OF TOTAL OZONE ANOMALIES

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SLIDE 45

Shepherd et al., Nature, 2014

TIME EVOLUTION OF HALOGEN-INDUCED O3 LOSS

Halogen-induced O3 loss started in the 60s Big negative O3 anomaly after volcanic eruptions

  • nly in ODS CTM

Ozone recovery but very small (difficult to claim it because of decadal dynamical variability)

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SLIDE 46

TIME EVOLUTION OF TOTAL OZONE ANOMALIES

Anomalies relative to the 1964‐1978 reference period

Black (ODS): CTM with changing ODS Blue (cODS): CTM with ODS fixed to 60s Yellow: ground- based obs. Red: Satellite Good agreement between ODS CTM and

  • bs. -> attribution
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SLIDE 47

TIME SERIES OF MONTHLY ZONAL MEAN H2O AT 100 hPa OVER 20°S-20°N FOR 1988-2010

How can we correct biases to merge data & derive trend? Used CTM H2O as transfer function Note that no evidence of long- term trend in CTM with respect to SAGE or SCIA

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SLIDE 48

TIME SERIES OF MONTHLY ZONAL MEAN H2O AT 100 hPa OVER 20°S-20°N FOR 1988-2010

How can we correct biases to merge data & derive trend? Used CTM H2O as transfer function Note that no evidence of long- term trend in CTM with respect to SAGE or SCIA

Hegglin et al., Nature, 2014

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SLIDE 49

CONSISTENCY BETWEEN TROPICAL TEMPERATURE AND LOWER STRATOSPHERIC H2O

(16 months overlap)

T anomalies are correlated with CTM H2O anomalies and with merged satellite H2O anomalies Correlation drift with merged HALOE-MLS Temperature & H2O from CTM, Merged satellite, Merged HALOE/MLS

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SLIDE 50

THANK YOU