The impact of antarctic cloud radiative properties on a GCM climate simulation

A sensitivity study to evaluate the impact upon regional and hemispheric climate caused by changing the optical properties of clouds over the Antarctic continent is conducted with the NCAR Community Model version 2 (CCM2). Sensitivity runs are performed in which radiation interacts with ice clouds w...

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Bibliographic Details
Main Authors: Dan Lubin, Biao Chen, David H. Bromwich, Richard C. J. Somerville, Wan-ho Lee, Keith M. Hines
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 1998
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.668.5467
http://polarmet.osu.edu/PMG_publications/lubin_chen_jc_1998.pdf
Description
Summary:A sensitivity study to evaluate the impact upon regional and hemispheric climate caused by changing the optical properties of clouds over the Antarctic continent is conducted with the NCAR Community Model version 2 (CCM2). Sensitivity runs are performed in which radiation interacts with ice clouds with particle sizes of 10 and 40 mm rather than with the standard 10-mm water clouds. The experiments are carried out for perpetual January conditions with the diurnal cycle considered. The effects of these cloud changes on the Antarctic radiation budget are examined by considering cloud forcing at the top of the atmosphere and net radiation at the surface. Changes of the cloud radiative properties to those of 10-mm ice clouds over Antarctica have significant impacts on regional climate: temperature increases throughout the Antarctic troposphere by 18–28C and total cloud fraction over Antarctica is smaller than that of the control at low levels but is larger than that of the control in the mid-to upper troposphere. As a result of Antarctic warming and changes in the north–south temperature gradient, the drainage flows at the surface as well as the meridional mass circulation are weakened. Similarly, the circumpolar trough weakens significantly by 4–8 hPa and moves northward by about 48–58 latitude. This regional mass field adjustment halves the strength of the simulated surface westerly winds. As a result of indirect thermodynamic and dynamic effects, significant changes are observed in the zonal mean circulation and eddies