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On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation Office Earth Sciences Directorate 28th Annual Climate Diagnostics and Prediction Workshop Reno, Nevada 20-24 October 2003
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Page 1: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

On the Causes of the 1930s Dust Bowl

Siegfried Schubert, Max Suarez, Philip Pegion,

Randal Koster and Julio Bacmeister

Global Modeling and Assimilation Office

Earth Sciences Directorate

28th Annual Climate Diagnostics and Prediction WorkshopReno, Nevada

20-24 October 2003

Page 2: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

The Dust Bowl

I. What is the role of SSTs?

- different ocean basins

- extratropical versus tropical

II. Are land/atmosphere feedbacks important?

III. How is it different from other Great Plains droughts of the 20th century?

IV. Can we predict the next one?

Page 3: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

AGCM: NSIPP-1 (NASA S-I Prediction Project)

Climatology and Skill (Bacmeister et al. 2000, Pegion et al. 2000, Schubert et al. 2002)

Global grid point dynamical core, 4rth Order (Suarez and Takacs 1995)

Relaxed Arakawa-Schubert Convection (Moorthi and Suarez 1992)

Shortwave/Longwave Radiation (Chou et al. 1994, 1999)

Mosaic interactive land model (Koster and Suarez 1992, 1996)

1st Order PBL Turbulence Closure (Louis et al. 1982)

AGCM runs with Specified SST (C20C project)

HadISST and sea ice dataset (1902-1999)

14 ensemble members - same SST, different ICs

Model resolution: 3 degree latitude by 3.75 degree longitude (34 levels)

Page 4: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

The Dust Bowl

Page 5: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
Page 6: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
Page 7: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
Page 8: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
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Page 10: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
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Page 12: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
Page 13: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
Page 14: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
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Other Droughts

Page 16: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

Corr=0.57

?

Page 17: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
Page 18: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

PPP ENSO

Trend

Low Pass EOF 1 (Trend) Low Pass EOF 2 (PPP)

Residual EOF 1 (ENSO) PC Time Series

Page 19: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

Correlation between PPP and Great Plains Precipitation (low frequency -> 6 years and longer)

Individual ensemble member precipitation

Min = 0.31 max = 0.70,

Ensemble mean precipitation (= 0.74)

Observed precipitation (= 0.41)

Page 20: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

1970s Dust Bowl?

Page 21: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

Borchert, John R. “The Dust Bowl of the 1970s”, AAAG, vol 61, March 1971

ABSTRACT: Major droughts in the Grassland region of the central United States have occurred rhythmically during the period of the instrumental record. The time for the next one may be near. ….

Page 22: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

“By mid February of 1977 the midwestern US was experiencing one of the most severe droughts in its recorded history … dramatic dust storms blew up in eastern Colorado and western Kansas and Oklahoma …drought was actually most severe in Minnesota and Dakotas …”

“By the fall of 1977 the general drought picture …. had changed significantly”

Symposium on North American Droughts - February 21 1977 (Introduction by Norman Rosenberg, AAAS Selected Symposium 15)

Page 23: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.
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Page 25: On the Causes of the 1930s Dust Bowl Siegfried Schubert, Max Suarez, Philip Pegion, Randal Koster and Julio Bacmeister Global Modeling and Assimilation.

Conclusions based AGCM Results• Tropical SST anomalies and land/atmosphere feedbacks

caused the 1930s dust bowl• All three tropical ocean basins played a role

– Cool Pacific and Indian (remote response - upper level flow)– Warm Atlantic (local response - upper and low level flow)– Extra-tropical SSTs acted to extend the drought to the east

• The SST forcing of the Dust Bowl differs from that of other major droughts (1910s and 1950s where the Pan Pacific Pattern of SST is the main driver)

• Predicting future Dust Bowls/droughts: need better coupled models with improved simulation of decadal ocean variability, and reduced uncertainty in land/atmosphere coupling; also need better understanding of role of ENSO and global warming


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