Lewis, S.; Lebonnois, S.; Covey, C.; Dawson, J.; Lee, C.; Parish, H.; Read, P. L.; Schubert, G.; Yamamoto, M.; Bengtsson, L.; Grinspoon, D.; Limaye, S.; Schmidt, H.; Svedhem, H. and Titov, D.
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Within the context of a working group supported by ISSI (Bern, Switzerland), we have made an intercomparison work between Global Circulation Models using simpli?ed parameterizations for radiative forcing and other physical processes. Even with similar schemes and parameters, the different GCMs produce different circulations, illustrating interesting differences between dynamical model cores.
|Item Type:||Conference Item|
|Copyright Holders:||2010 The Authors|
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Stephen Lewis|
|Date Deposited:||20 Dec 2010 09:28|
|Last Modified:||24 Feb 2016 10:00|
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