Title: The Whole Atmosphere Community Climate Model: Overview, Current Research and Future Plans
1The Whole Atmosphere Community Climate Model
Overview, Current Research and Future Plans
2Outline
- 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
3Acknowledgments
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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51. Overview of WACCM
6NCAR 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
7WACCM3 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
8Current 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
9Zonal-Mean T JULY
140 K
270 K
200 K
10Zonal-Mean U JULY
11Zonal-Mean O3 JULY
122. Research with WACCM
13Solar min/max simulations
- Fixed solar minimum and solar maximum conditions
(constant F10.7 and Kp typical of minimum/maximum)
14definition of solar variability
- Photolysis and heating rates are parameterized
in terms of f10.7 and Kp
15Stratospheric temperature response
SSU/MSU4 (1979-2003)
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17Ozone column vs. f10.7 regressions WACCM and
observations
181950-2003 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)
19Calculated and Observed Ozone Trends
20Total Column Ozone Trends (Global)
21Calculated and Observed Temperature Trends
22Temperature Trends (Global), K / Decade
23Whole-atmosphere zonal-mean T trend 1950-2003
CO2 increase (greenhouse effect)
2421st 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.
25Global-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
26Global-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.
27Stratospheric age of air is also affected by
changing GHG
28Upper 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
29Similar spectral behavior in WACCM calculations
as in SABER data
Wavenumber/frequency T spectra at 36N and 80 km
(July)
WACCM T Spectrum
30Components of 2-day wave in SABER data and WACCM
simulation
SABER observations and WACCM results for July
31 more components of 2-day wave in SABER data
and WACCM
323. 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
33To 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