Bibliography - J. Durachta
- Delworth, T. L., A. J. Broccoli, A. Rosati, R. J. Stouffer, V. Balaji, J. A. Beesley, W. F. Cooke, K. W. Dixon, J. P. Dunne, K. A. Dunne, J. Durachta, and K. L. Findell, et al., 2006: GFDL’s CM2 Global Coupled Climate Models. Part 1: Formulation and Simulation Characteristics. Journal of Climate, 19, doi:10.1175/JCLI3629.1 643-674
[ Abstract ]The formulation and simulation characteristics of two new global coupled climate models developed at
NOAA’s Geophysical Fluid Dynamics Laboratory (GFDL) are described. The models were designed to
simulate atmospheric and oceanic climate and variability from the diurnal time scale through multicentury
climate change, given our computational constraints. In particular, an important goal was to use the same
model for both experimental seasonal to interannual forecasting and the study of multicentury global
climate change, and this goal has been achieved.
Two versions of the coupled model are described, called CM2.0 and CM2.1. The versions differ primarily
in the dynamical core used in the atmospheric component, along with the cloud tuning and some details of
the land and ocean components. For both coupled models, the resolution of the land and atmospheric
components is 2° latitude X 2.5° longitude; the atmospheric model has 24 vertical levels. The ocean
resolution is 1° in latitude and longitude, with meridional resolution equatorward of 30° becoming progressively
finer, such that the meridional resolution is 1/3° at the equator. There are 50 vertical levels in the
ocean, with 22 evenly spaced levels within the top 220 m. The ocean component has poles over North
America and Eurasia to avoid polar filtering. Neither coupled model employs flux adjustments.
The control simulations have stable, realistic climates when integrated over multiple centuries. Both models have simulations of ENSO that are substantially improved relative to previous GFDL coupled
models. The CM2.0 model has been further evaluated as an ENSO forecast model and has good skill
(CM2.1 has not been evaluated as an ENSO forecast model). Generally reduced temperature and salinity
biases exist in CM2.1 relative to CM2.0. These reductions are associated with 1) improved simulations of
surface wind stress in CM2.1 and associated changes in oceanic gyre circulations; 2) changes in cloud tuning
and the land model, both of which act to increase the net surface shortwave radiation in CM2.1, thereby
reducing an overall cold bias present in CM2.0; and 3) a reduction of ocean lateral viscosity in the extratropics
in CM2.1, which reduces sea ice biases in the North Atlantic.
Both models have been used to conduct a suite of climate change simulations for the 2007 Intergovernmental
Panel on Climate Change (IPCC) assessment report and are able to simulate the main features of
the observed warming of the twentieth century. The climate sensitivities of the CM2.0 and CM2.1 models
are 2.9 and 3.4 K, respectively. These sensitivities are defined by coupling the atmospheric components of
CM2.0 and CM2.1 to a slab ocean model and allowing the model to come into equilibrium with a doubling
of atmospheric CO2. The output from a suite of integrations conducted with these models is freely available
online (see http://nomads.gfdl.noaa.gov/).
- Balaji, V., J. Anderson, I. Held, M. Winton, J. Durachta, S. Malyshev, and R. J. Stouffer, May 2005: The Exchange Grid: a mechanism for data exchange between Earth System components on independent grids. Parallel Computational Fluid Dynamics 2005 - Theory and Applications, Elsevier, http://www.gfdl.noaa.gov/~vb/pdf/xgridpaper.pdf, 179-188
[ Abstract ]We present a mechanism for exchange of quantities between components of a coupled Earth
system model, where each component is independently discretized. The exchange grid is
formed by overlaying two grids, such that each exchange grid cell has a unique parent cell
on each of its antecedent grids. In Earth System models in particular, processes occurring near
component surfaces require special surface boundary layer physical processes to be represented
on the exchange grid. The exchange grid is thus more than just a stage in a sequence of regridding
between component grids.
We present the design and use of a 2-dimensional exchange grid on a horizontal planetary
surface in the GFDL Flexible Modeling System (FMS), highlighting issues of parallelism and
performance.
Direct link to page: http://cmi.princeton.edu/bibliography/results.php?author=3942