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Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

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Page 1: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Climate Model Observing System Simulation Experiments

Bill Collins

UC Berkeley and LBL

with A. Lacis and V. Ramaswamy

Page 2: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Topics

• Motivation for climate modeling applications

• Goals of the observing system simulation

• Major components of the OSSE

• Proposed emulators

• Description of the OSSE

Page 3: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Reductions in Arctic sea ice

• Arctic summer sea ice extent is shrinking at 7.4+2.4% per decade.

IPCC AR4, 2007

NASA & NSIDC

Page 4: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Further reductions in Arctic sea ice

2000

2100

IPCC AR4, 2007

Page 5: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Trends in N. hemisphere snow cover

• Since 1988, snow cover has declined by 5%.• Linear trend is -0.9+0.4% per decade.

IPCC AR4, 2007

Page 6: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Projections for snow cover: 2000 to 2100

IPCC AR4, 2007 Supplementary Figure S10.1. Multi model mean snow cover and projected changes over the 21st century from 12 (a and b) and 11 (c) AOGCMs, respectively. a) Contours mark the locations where the December to February (DJF) snow area fraction exceeds 50%, blue for the period 1980–1999, and red for 2080–2099, dashed for the individual models and solid for the multi model mean. b) Projected multi model mean change in snow area fraction over the period 2080–2099, relative to 1980-1999. Shading denotes regions where the ensemble mean divided by the ensemble standard deviation exceeds 1.0 (in magnitude),

Supplementary Figure S10.1. Multi model mean snow cover and projected changes over the 21st century from 12 (a and b) and 11 (c) AOGCMs, respectively. a) Contours mark the locations where the December to February (DJF) snow area fraction exceeds 50%, blue for the period 1980–1999, and red for 2080–2099, dashed for the individual models and solid for the multi model mean. b) Projected multi model mean change in snow area fraction over the period 2080–2099, relative to 1980-1999. Shading denotes regions where the ensemble mean divided by the ensemble standard deviation exceeds 1.0 (in magnitude),

Snow Cover Snow Cover Change

Page 7: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Low confidence in cloud evolution

IPCC AR4, 2007

Change in cloud amount in 21st century: A1B Scenario

Page 8: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Uncertain cloud radiative response

• Models do not converge on sign of change in cloud radiative effects.

• Trends in cloud radiative effects have magnitude < 0.2 Wm-2 decade-1.

Change from 1980-1999 to 2080-2099

Change in cloud radiative effects in 21st century: A1B Scenario

IPCC AR4, 2007

Page 9: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Low confidence in cloud feedbacks

IPCC AR4, 2007

Change in cloud radiative effects: 1% CO2/year simulations

Page 10: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Goals of the OSSEs

• Test the detection and attribution of radiative forcings and feedbacks from the CLARREO data:

• Determine feasibility of separating changes in clouds from changes in the rest of the climate system

• In solar wavelengths, examine feasibility of isolating forcings and feedbacks

• Quantify the improvement in detection and attribution skill relative to existing instruments

Page 11: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Role of climate models in OSSEs

• Goals of OSSEs require projections of climate change.

• Sole source of these projections: climate models

• Advantages of climate models for this application:• Identification of forcings for each radiatively active species

• Separation of feedbacks associated with water vapor, lapse rate, clouds

• Tests of CLARREO concept with climate models• To what extent can forcings and feedbacks can be separated and quantified

using simulated CLARREO data?

• What are the time scales for unambiguous detection and attribution?

Page 12: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Schematic of Tests

ForcingForcing Climate ModelsClimate Models

CLARREOEmulator

CLARREOEmulator

CLARREOForcing

CLARREOForcing

Compare

ForcingForcing Climate ModelsClimate Models

CLARREOEmulator

CLARREOEmulator

CLARREOFeedbackCLARREOFeedback

Compare

Model Feedback

Model Feedback

Page 13: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Individual forcings in Climate Models

IPCC AR4, 2007 MIROC+SPRINTARS

Page 14: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Individual feedbacks in Climate Models

IPCC AR4, 2007

Page 15: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Major steps in Climate OSSEs

1. Conduct OSSEs with 3 models analyzed in the IPCC AR4

2. Add adding two new components to these models :A. Emulators for the shortwave and infrared CLARREO

B. More advanced spectrally resolved treatments of surface spectral albedos

3. Results from emulators serve as surrogate CLARREO data

4. Estimate the forcings and feedbacks from emulators

5. Compare to forcings / feedbacks calculated directly from model physics

Page 16: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Models for Climate OSSEs

Three models for OSSEs: • NASA Goddard Institute for Space Studies (GISS) modelE (Schmidt et al, 2006) • NOAA Geophysical Fluid Dynamics Laboratory (GFDL) Coupled Model CM-2 and CM-2.1 (Delworth et al, 2006) • NCAR Community Climate System Model CCSM3 (Collins et al, 2006).

Page 17: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Model Simulations for Climate OSSEs

Three classes of simulations for OSSEs: • Pre-industrial conditions with constant atmospheric composition • 21st century with the IPCC emissions scenarios• 20th and/or 21st centuries with single forcings, e.g., just CO2(t)

IPCC AR4, 2007

Page 18: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Candidate CLARREO Emulator

MODerate spectral resolution atmospheric TRANSmittance (Modtran4) version 3 (Berk et al, 1999)

Spectral resolution of Modtran4: • 0 to 50,000 cm-1: 1 cm-1 • Blue and UV: 15 cm-1

Relationship to CLARREO: • Infrared: 1X • UV/Blue/NIR: 10-100X

Alternate emulators:• GISS, GFDL, and NCAR LBL codes

Berk et al, 1999

Page 19: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Features of Modtran4

Modtran4 includes:

• Correlated-k treatment of atmospheric transmission• BDRFs for non-Lambertian surfaces• Line parameters obtained from Hitran 2002 database

Berk et al, 1999

Page 20: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Advantages of Modtran4

• Economical compromise among resolution, accuracy, and speed• Team members have experience using Modtran to simulate AIRS• Modtran is a community-standard radiative transfer code

Huang et al, 2007

Page 21: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Timing of Modtran4

• CPU time for IR calculations:• Resolution: 1 cm-1

• Range: 100-3333.0 cm-1

• CPU time for IR calculations:• Resolution: 15 cm-1

• Range: 3333.0-33333.0 cm-1

•Calculation specs:• 25-level standard cloud-free tropical profile• CPU = Intel Dual-core 1862.166 MHz processor

• Implications: ~Few hours CPU time per simulated month

Total (s) User (s) System (s) Utilization

0.73 0.46 0.01 64%

Total (s) User (s) System (s) Utilization

1.16 0.91 0.01 79%

Page 22: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Primary steps in the OSSE

Phases for the study:

• Linking the CLARREO emulator Modtran4 with the climate models• Adoption of spectral surface emissivity and BDRF models• Simulations for a constant composition to determine the natural variability • Simulations of CLARREO measurements for transient climate change

ModelArchive ModelArchive

CLARREOEmulator

CLARREOEmulator

Emulation ValidationEmulation Validation

Page 23: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Natural variability in the spectra

Huang et al, 2002

25-day Variability, Central Pacific

25-day Variability, Western Pacific

• Goal: quantify signal-to-noise ratios for forcings and feedbacks (cf Leroy et al, 2007)

• .Calculations: pre-industrial conditions for “background” radiance field

• Goal: quantify signal-to-noise ratios for forcings and feedbacks (cf Leroy et al, 2007)

• .Calculations: pre-industrial conditions for “background” radiance field

Page 24: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Issues for the Emulation

• For speed and expediency, we recommend using using the existing IPCC AR4 archive for emulation.

• The reason? Centennial length simulations are very expensive.

• The trade-offs:• Highest temporal sampling: daily means of model state• Nominal temporal sampling: monthly means of model state• This precludes reproducing the space-time track of CLARREO’s orbit• For solar, we can reproduce monthly-mean solar_zenith (latitude)

• Result: Our results are an upper bound on detection/attribution skill• Our results would reflect perfect diurnal sampling at each model grid point.

• Alternate, but very remote, possibility: “time-slice” experiments• Advantage: interactive coupling and capture space-time sampling

1950 1960 1970 1980 1990 2000 2010 2020 2030 2040 2050

TimeSlice

TimeSlice

TimeSlice

TimeSlice

Page 25: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Issues for the Emulation, part 2

• Atmospheric conditions:• All-sky: predominant condition for 100-km pixels• Clear-sky: sets upper bound for detection-attribution skill for non-cloud forcings and feedbacks

• Detection and attribution: projection onto spectral “basis functions” for single forcings and feedbacks

Anderson et al, 2007

Page 26: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

First Six Months

Objective: Configuration and initiation of the OSSEs • Acquisition of licenses and software for Modtran 4, the CLARREO simulator• Development of interfaces between IPCC models and Modtran 4• Automation of software for analysis of IPCC simulations with Modtran 4• Introduction of spectral surface emissivity and bi-directional albedo models• Simulation of CLARREO measurements from IPCC model results, including:

- Calculations for pre-industrial conditions- Calculations for transient climate change with all forcings

• Perform parallel calculations for all-sky and clear-sky conditions• Estimation of natural (unforced) variability in the simulated CLARREO data

Page 27: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Second Six Months

Objective: Detection and estimation of radiative forcings • Simulation of CLARREO measurements from IPCC model results, including:

- Calculations for transient climate change from single forcings• Calculation of spectral signatures of shortwave and longwave forcings from reference radiative transfer calculations with Modtran 4• Estimation of radiative climate forcing from simulated clear-sky CLARREO data

- Projection global CLARREO simulations onto single-forcing spectral signatures to isolate time-dependent forcings- Comparison of estimates with actual forcing of the climate models- Derivation of signal-to-noise ratio using unforced variability in simulated clear-sky radiances as the noise- Characterize improvements, if any, in estimates and time-to-detection relative to existing satellite instruments

• Repeat forcing estimation for all-sky fluxes- Quantify degradation in forcing estimates and time-to-detection from the substitution of all-sky for clear-sky observations

Page 28: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Final Six Months

Objective: Detection and estimation of radiative feedbacks • Estimation of radiative climate feedbacks from the simulated CLARREO data

- Estimation of surface-albedo feedbacks for clear and all-sky data- Estimation of water-vapor/lapse-rate feedbacks for clear and all-sky data- Estimation of cloud feedbacks from all-sky data only- Comparison of estimates with feedback estimates derived independently

• Characterize improvements in estimates and time-to-detection relative to existing satellite instruments

Page 29: Climate Model Observing System Simulation Experiments Bill Collins UC Berkeley and LBL with A. Lacis and V. Ramaswamy

Key questions for Climate OSSEs

•Can the forcings from aerosols and land-use change and the feedbacks from snow and ice be detected and quantified using CLARREO data?

•Can the indirect shortwave forcings from aerosol-cloud interactions and the feedbacks from clouds be detected and quantified using CLARREO data?

•What are the implications of pixel size for the detection and quantification of forcings and feedbacks in clear-sky versus all-sky observations?

•To what extent is it possible to isolate forcings and feedbacks associated with changes in specific species and processes in the CLARREO measurements?

•Can changes in and longwave feedbacks from low, middle, high clouds be detected and quantified using the CLARREO infrared data?