The Whole Atmosphere Community Climate Model: Overview, Current Research and Future Plans PowerPoint PPT Presentation

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Title: The Whole Atmosphere Community Climate Model: Overview, Current Research and Future Plans


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The Whole Atmosphere Community Climate Model
Overview, Current Research and Future Plans
  • Rolando Garcia

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Outline
  • WACCM overview
  • Research with WACCM
  • Solar cycle impacts
  • 1950-2003 trend simulations
  • 21st century prognostic simulations
  • Upper atmosphere dynamics (2-day wave)
  • 3. Future work

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Acknowledgments
the following colleagues contributed to the work
presented in this talk . . .
  • Doug Kinnison (ACD)
  • Dan Marsh (ACD)
  • Katja Matthes (Free University Berlin)
  • Astrid Maute (HAO)
  • Jadwiga Richter (CGD)
  • Fabrizio Sassi (CGD)
  • Stan Solomon (HAO)

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1. Overview of WACCM
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NCAR Whole Atmosphere Community Climate Model
  • Based on The Community Atmosphere Model (CAM3)
  • 0-140 km (66 levels Dz 1.3 km in lower
    stratosphere to 3 km in thermosphere)
  • Finite-volume dynamics
  • 30 minute time step
  • MOZART-3 chemistry package (55 species)
  • Upper atmosphere extensions
  • Lindzen GW parameterization
  • Molecular diffusion
  • NO cooling
  • non-LTE long-wave heating in the 15 µm band of
    CO2 and the 9.6 µm band of O3

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WACCM3 additions
  • The following processes are now dealt with in a
    self-consistent manner in WACCM
  • Solar variability
  • Chemical heating
  • Airglow
  • Ion chemistry (5 ion species electrons)
  • EUV and X-ray ionization
  • Auroral processes
  • Particle precipitation
  • Ion drag
  • Joule heating
  • Chemistry is completely interactive with dynamics

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Current interdivisional collaborators
  • Current external collaborations
  • Mark Baldwin (NWRA)
  • annular modes
  • Natalia Calvo (U. of Madrid) and Marco Giorgetta
    (MPI, Hamburg)
  • effects of ENSO on the middle atmosphere
    comparison of models and reanalysis data
  • Charlie Jackman (NASA/Goddard)
  • impacts of solar proton events on ozone
  • Judith Perlwitz and Martin Hoerling
    (NOAA/Boulder)
  • climate impacts of changing chemistry and SST
  • Cora Randall et al. (CU/LASP) plus John Gille
    (ACD/HIRDLS) and Laura Pan (ACD/UTLS initiative)
  • process-oriented evaluation of
    chemistry-climate models vs. observations

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Zonal-Mean T JULY
140 K
270 K
200 K
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Zonal-Mean U JULY
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Zonal-Mean O3 JULY
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2. Research with WACCM
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Solar min/max simulations
  • Fixed solar minimum and solar maximum conditions
    (constant F10.7 and Kp typical of minimum/maximum)

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definition of solar variability
  • Photolysis and heating rates are parameterized
    in terms of f10.7 and Kp

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Stratospheric temperature response
SSU/MSU4 (1979-2003)
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Ozone column vs. f10.7 regressions WACCM and
observations
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1950-2003 trends simulation
  • An ensemble of retrospective runs, 1950-2003,
    including solar variability, observed SST,
    observed trends in GHG and halogen species, and
    observed aerosol surface area densities (for
    heterogeneous chemistry)

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Calculated and Observed Ozone Trends
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Total Column Ozone Trends (Global)
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Calculated and Observed Temperature Trends
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Temperature Trends (Global), K / Decade
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Whole-atmosphere zonal-mean T trend 1950-2003
CO2 increase (greenhouse effect)
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21st century prognostic simulations
  • An ensemble of prognostic runs, 1975-2050, to
    look at climate change and ozone recovery in the
    21st century. Follows WMO A1B scenario.
  • An additional ensemble assumed constant CO2, CH4,
    N2O to assess the role of stratospheric cooling
    by these gases.

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Global-mean ozone column
recovery to 1980 values 2040
1950-2003 sim
1980-2050 sim (A1B scenario)
smoothed with 12-month running mean
column minimum 2000-2010
  • 21st century prognostic simulation (red) shown
    together with the results of the 19502003
    simulation (black) discussed earlier

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Global-mean ozone column
  • A1B scenario produces super-recovery compared
    to no climate change simulation wherein CO2,
    N2O, CH4 are held at 1995 values.
  • This is due to colder stratospheric T in A1B
    scenario.

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Stratospheric age of air is also affected by
changing GHG
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Upper atmosphere dynamics The 2-day wave
  • Apart from the tides, the 2-day wave dominates
    high-frequency variability in the MLT
  • Has large amplitude at solstice, especially in
    the summer hemisphere
  • Has been interpreted as a normal mode (e.g.,
    Salby, 1981), a result of baroclinic instability
    (e.g., Plumb, 1983), and a combination of both
    (e.g., Randel, 1994)
  • Comparison of WACCM simulations and observations
    by the SABER instrument on the TIMED satellite

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Similar spectral behavior in WACCM calculations
as in SABER data
Wavenumber/frequency T spectra at 36N and 80 km
(July)
WACCM T Spectrum
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Components of 2-day wave in SABER data and WACCM
simulation
SABER observations and WACCM results for July
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more components of 2-day wave in SABER data
and WACCM
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3. Future Work
  • Climate sensitivity to doubling CO2 CAM vs.
    WACCM
  • Impact of ozone hole and changing tropical SST
    on Arctic/Antarctic surface climate
  • Climatology of stratospheric sudden warmings
    impacts of resolution, gravity wave
    parameterization, SST variability relationship
    to annular modes
  • Process-oriented evaluation of model chemistry
    (comparisons with EOS/Aura observations)
  • Impact of solar proton events on mesospheric and
    stratospheric composition
  • Energy budget and dynamics of the MLT
    comparison with SABER observations

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To keep in touch . WACCM website and new model
release
  • WACCM website is being hosted under ACD
    (http//waccm.acd.ucar.edu/index.shtml)
  • Website has been updated and reformatted
  • 2006 CSL proposal posted on site
  • WACCM3 description to be completed
  • Release WACCM3 in summer 2006
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