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Antarctic Sea Ice Variability in the CCSM2 Control Simulation
Marika Holland National Center for Atmospheric Research Cecilia Bitz Polar Science Center, APL, Seattle Elizabeth Hunke Los Alamos National Laboratory
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Introduction/Motivation
550 years of CCSM2 Model simulation analyzed (yrs ) To assess the realism of the CCSM2 simulation To examine the physical processes driving simulated sea ice variability, including influence of simulated feedbacks To determine influence of large scale modes of variability on Antarctic sea ice conditions
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Mean Sea Ice Conditions
Ice Concentration Winter Average Summer Average
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Leading mode of winter variability
Ice Concentration Simulated (600 yrs) Observed ( )
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Advection of Anomalies
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Atmospheric Conditions Associated with Ice Dipole
Autumn Winter AMJ SAT AMJ SLP Consistent with anomalies being forced by both winds and SAT.
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Ocean Conditions Associated with Ice Dipole
SST Considerable SST anomalies also associated w/ice. Ocean velocity consistent with SLP. Contribute to dynamical forcing of ice anomalies and ocn heat transport anomalies.
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Forcing of Pacific variability
Enhanced Pacific ice driven by processes in preceding autumn Both thermodynamics and dynamics contribute In winter thermodynamics enhance, dynamics damps largest at 1 yr lag Suggests feedbacks prolong anomalies Dynamic Processes AMJ JAS Solid=thermo (ice growth) Dash=dynamics (advection, ridging) AMJ JAS Thermodynamic Processes Pacific ice area tendency terms regressed on Ice EOF
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Forcing of Atlantic variability
Dynamic Processes Reduced ice driven by processes in preceding autumn Both dynamics and thermodynamics contribute In winter, thermodynamic processes continue to increase anomalies. Less memory than Pacific Anomalies shorter-lived AMJ JAS Thermodynamic Processes AMJ JAS Atlantic ice area tendency terms regressed on Ice EOF
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“Memory” of Atmospheric Anomalies
Solid = max correlation Dash = -min correlation Solid=max r Dash=-min r Solid=max r Dash=-min r SLP SAT Largest correlations at lag=0 Indications of enhanced correlations preceding ice dipole Small correlations following ice dipole Highest correlation near lag=0 Enhanced correlations both lead and lag the ice dipole timeseries Positive feedbacks
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Associated Ocean SW absorption
Albedo feedback modifies SW absorption Helps prolong life of anomalies particularly in Pacific in Atlantic, ocean currents transport warm SSTs away from ice formation regions, reducing their influence
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Relationship to large scale modes of variability
Number of observational studies have looked at the influence of ENSO on southern hemisphere sea ice conditions results appear consistent with the ice dipole A recent modeling study (Hall and Visbeck, 2002) has suggested a relationship between Antarctic sea ice and the Southern Annular Mode (SAM) Wanted to determine whether these modes of variability play a role in forcing the sea ice dipole present in CCSM2
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Ice Area associated with ENSO
Ice anomalies small, but consistent with ADP. NINO3 and ADP correlate at r=-0.32 Forced by dynamics in Pacific, with thermo feedbacks amplifying in later years. Both dynamically and thermodynamically forced in Atlantic
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SLP and SAT associated with SAM
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Ice Conditions associated with SAM
Maximum at lag=1 Some similarities with ADP Correlates to ADP at r=0.35 Pacific and Indian - dynamically forced at lag=0 anomalous ice growth enhances at lag=1 Atlantic - largely thermo driven anomalies
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Conclusions As in observations, CCSM2 Antarctic ice variability exhibits a dipole pattern with enhanced Pacific ice associated with reduced Atlantic ice These are forced by both dynamical and thermodynamical processes, consistent with atmosphere and ocean conditions Albedo feedback prolongs anomalies in Pacific. Its influence in Atlantic is reduced due to transport of anomalous SST to regions where no ice formation occurs Both ENSO and SAM appear to weakly influence the ice dipole pattern
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