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The Dynamics of Western Hemisphere Circulation Evolution in the MJO Naoko Sakaeda and Paul Roundy Dept. Atmospheric and Environmental Sciences
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From Roundy (2014, J. Atmos. Sci)
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Data Wind data from CFS Reanalysis data (Saha et al. 2010) Interpolated Outgoing Longwave Radiation (OLR) as proxy for tropical convection (Liebmann and Smith 1996) Period: 1980-2010 DJF
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Methodology: Composite MJO Events MJO Index: Derived similarly to RMM except using 20-100days filtered OLR only The Western Hemisphere Zonal Wind Index (WHZI): 20-100 days 200hPa zonal wind averaged 2.5 ° N to 2.5 ° S and 140 ° W to 40 ° W WHZI MJO
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Methodology: MJO Events Select MJO Phase 1 events with amplitude greater than or equal to 0.5 during DJF WHZI<0: Easterly Wind Events WHZI>0: Westerly Wind Events
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Methodology: Zonal Momentum Budget
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At 200 hPa: 10°S-5°N, 110°W-80°W
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10°S-5°N, 110°W-80°W Averaged Budget Terms: 200 hPa Kelvin wave in Shallow Water System Time Lag (Days)
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Methodology: Zonal Momentum Budget Time linear decomposition of zonal momentum equation : Background State (Seasonal Cycle + Periods longer than 100 days) : Intraseasonal Timescale (20-100 days) : Transient Timescale (Periods shorter than 20 days)
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10°S-5°N, 110°W-80°W Averaged Budget Terms 200 hPa acts to maintain and amplify but it is offset by the pressure gradient force
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10°S-5°N, 110°W-80°W Averaged Budget Terms 200 hPa
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10°S-5°N, 130°W-100°W Averaged Budget Terms, 100 hPa
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10°S-5°N, 130°W-100°W Averaged Budget Terms, 100 hPa
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10°S-5°N, 110°W-80°W Averaged Budget Terms Shading: Variance of 200hPa Intraseasonal Zonal Wind Black contour: Zonal Convergence of 200hPa Background Zonal Wind (2 x 10 6 s -1 interval)
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10°S-10°N Averaged Longitude-Pressure Cross Sections Shading: intraseasonal zonal wind anomaly Black contour: intraseasonal geopotential height anomaly at 2 m interval
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Eastward and Westward-Moving OLR, 100hPa Wind, and Geopotential Height Anomalies R R R R A A A A
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Summary Upper-tropospheric intraseasonal wind over the Western Hemisphere cannot simply be explained as a “free” Kelvin wave generated by MJO convection MJO H H Kelvin Suppressed MJO H H
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Additional Figures
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