The Low-Resolution CCSM3Source: Journal of Climate:;2006:;volume( 019 ):;issue: 011::page 2545DOI: 10.1175/JCLI3744.1Publisher: American Meteorological Society
Abstract: The low-resolution fully coupled configuration of the Community Climate System Model version 3 (CCSM3) is described and evaluated. In this most economical configuration, an ocean at nominal 3° resolution is coupled to an atmosphere model at T31 resolution. There are climate biases associated with the relatively coarse grids, yet the coupled solution remains comparable to higher-resolution CCSM3 results. There are marked improvements in the new solution compared to the low-resolution configuration of CCSM2. In particular, the CCSM3 simulation maintains a robust meridional overturning circulation in the ocean, and it generates more realistic El Niño variability. The improved ocean solution was achieved with no increase in computational cost by redistributing deep ocean and midlatitude resolution into the upper ocean and the key water formation regions of the North Atlantic, respectively. Given its significantly lower resource demands compared to higher resolutions, this configuration shows promise for studies of paleoclimate and other applications requiring long, equilibrated solutions.
|
Collections
Show full item record
contributor author | Yeager, Stephen G. | |
contributor author | Shields, Christine A. | |
contributor author | Large, William G. | |
contributor author | Hack, James J. | |
date accessioned | 2017-06-09T17:01:51Z | |
date available | 2017-06-09T17:01:51Z | |
date copyright | 2006/06/01 | |
date issued | 2006 | |
identifier issn | 0894-8755 | |
identifier other | ams-78212.pdf | |
identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4220857 | |
description abstract | The low-resolution fully coupled configuration of the Community Climate System Model version 3 (CCSM3) is described and evaluated. In this most economical configuration, an ocean at nominal 3° resolution is coupled to an atmosphere model at T31 resolution. There are climate biases associated with the relatively coarse grids, yet the coupled solution remains comparable to higher-resolution CCSM3 results. There are marked improvements in the new solution compared to the low-resolution configuration of CCSM2. In particular, the CCSM3 simulation maintains a robust meridional overturning circulation in the ocean, and it generates more realistic El Niño variability. The improved ocean solution was achieved with no increase in computational cost by redistributing deep ocean and midlatitude resolution into the upper ocean and the key water formation regions of the North Atlantic, respectively. Given its significantly lower resource demands compared to higher resolutions, this configuration shows promise for studies of paleoclimate and other applications requiring long, equilibrated solutions. | |
publisher | American Meteorological Society | |
title | The Low-Resolution CCSM3 | |
type | Journal Paper | |
journal volume | 19 | |
journal issue | 11 | |
journal title | Journal of Climate | |
identifier doi | 10.1175/JCLI3744.1 | |
journal fristpage | 2545 | |
journal lastpage | 2566 | |
tree | Journal of Climate:;2006:;volume( 019 ):;issue: 011 | |
contenttype | Fulltext |