stratospheric temperature trends in gfdl model runs skyhi am2 --- new model, atmosphere with...
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![Page 1: Stratospheric Temperature Trends in GFDL model runs SKYHI AM2 --- New model, atmosphere with specified SSTs. CM2 --- New model, coupled ocean (CM2.1 ---](https://reader035.vdocuments.net/reader035/viewer/2022062518/56649d3f5503460f94a1820e/html5/thumbnails/1.jpg)
Stratospheric Temperature Trends in GFDL model runs
• SKYHI
• AM2 --- New model, atmosphere with specified SSTs.
• CM2 --- New model, coupled ocean
• (CM2.1 --- New model, coupled ocean,
finite volume dynamical core)
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• SKYHI simulations [see the B-set which employs a more realistic background ozone] global-annual-mean; zonal-annual-mean; zonal-seasonal-mean.
• Fixed SSTs; prognostic clouds based on Manabe-Wetherald scheme.
• Equilibrium simulations for (a) 1979 and (b) 1997. • WMGGs (IPCC, WMO).• Ozone (Randel-Wu trend data).• One calculation with H2O trend estimate (based
on Haigh and co-workers).• Temperature trend (Randel; Austin; Berlin).• B1 (ozone-only); B2 (ozone+WMGGs).• Model stat. sig. based on “unforced” runs.
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Ramaswamy and Schwarzkopf (2002)Model’s unforced
variability
Model simulation (trace gas changes)
}Obs.
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Ramaswamy and Schwarzkopf (GRL, 2002)
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S-R (GRL,2002)
‘filled’ Stat. sig. in
model
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• SKYHI simulations….continued
• Transient (“trns”} integrations [1979-1997]; 4-member ensemble.
• Ozone change specified as a linear variable at each grid-box and in each month.
• Results compared with “B1-equilibrium” solution and MSU4.
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• Simulations with GFDL AM2 [Anderson et al., 2004]. Top at ~5 mb {lower top and stratos. resolution than SKYHI}.
• Prescribed SSTs [Hurrell, 1981-2000].• Transient 4-member ensemble runs [1981-2000]. • Temporal (3D monthly-means) forcings: WMGGs (IPCC,
WMO); Strat. O3 (Randel); Volcanic (Stenchikov data blended with Sato et al.); Solar (Lean); Trop. aerosol direct effect (sea-salt and dust held fixed; sulfate, black and organic carbon vary with time) and ozone (varies with time) from MOZART2 CTM runs.
• Runs with SSTs-only and with subsets of forcings.• Temperature obs. (Randel; LKS; Austin; Soden).• Trend is difference of the end-year values.
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Solar included in wmgg+o3, wmgg+o3+aero.
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Solar included in wmgg+o3, wmgg+o3+aero
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• Simulations with GFDL CM2 [Delworth et al., 2004]. Same atmosphere as in AM2.
• 1860-2000 simulations.• 3-member ensemble runs [CM2.0]; 4-member
ensemble runs [CM2.1]. • Temporal (3D monthly-means) forcings: WMGGs
(IPCC, WMO); Strat. O3 (Randel); Volcanic (Stenchikov data blended with Sato et al.); Solar (Lean); Trop. aerosol direct effect (sea-salt and dust held fixed; sulfate, black and organic carbon vary with time) and ozone (varies with time) from MOZART2 CTM runs.
• Temperature obs. (Randel; LKS; Austin; Soden).• Trend is difference of the end-year values.
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WMGhgO3 = WMGG + StratO3 + TropO3Anthro = WMGhgO3 + Trop. Aerosol
Natural = Solar + volcanic aero.
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Global Mean Stratospheric Temperature Trends: Global Mean Stratospheric Temperature Trends: MSU MSU vsvs GFDL GCM (AM2p13)GFDL GCM (AM2p13)
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Global Mean Stratospheric Temperature Trends: Global Mean Stratospheric Temperature Trends: MSU MSU vsvs GFDL GCM (CM2p0)GFDL GCM (CM2p0)
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Global Mean Stratospheric Temperature Trends: Global Mean Stratospheric Temperature Trends: MSU MSU vsvs GFDL GCM (CM2p1)GFDL GCM (CM2p1)
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Contributions from
J. AustinL. HorowitzK.LabitzkeJ. LanzanteJ. LeanV. RamaswamyW. RandelD. SchwarzkopfB. SodenG. Stenchikov