Evalua&ng)Surface)Flux)Results)from)FLASHFlux)Version…€¦ ·...

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Evalua&ng  Surface  Flux  Results  from  FLASHFlux  Version  3A   Anne C. Wilber1, David P. Kratz2, Paul W. Stackhouse, Jr.2, Shashi K. Gupta1,

and Parnchai K. Sawaengphokhai1 1Science Systems and Applications, Inc., Hampton, Virginia

2NASA Langley Research Center, Hampton, Virginia "

Conclusions: !Shortwave : : Replacing the WCP-55 aerosol properties in the SW algorithm with monthly climatological properties based on -year monthly averages of MATCH aerosol optical depths made considerable difference in the resulting fluxes. Though the comparison with the ground measurements shows little improvement, the use of the more up-to-date optical depths correspond to an improvement in the ground measurement/FLASHFlux difference histograms shown above. For further improvement in the SW model, it is planned to use near real time aerosols in place of the climatology. Also, work continues on the cloud transmission algorithm. "

Longwave: The use of the new GEOS 5.9.1 meteorology with change in the lower atmospheric temperature, humidity and skin temperature made the largest difference in the surface LW results. FLASHFlux LW fluxes overall showed a slightly larger bias but a slightly improved RMSE. The most improved surface types were the the Island and Desert sites."

Continued assessment of the FLASHFlux data products is on-going. The TOA flux products are being successfully used to evaluate radiative flux variability for the annual “State of Climate” report published annually in BAMS (see poster 147). Year-to-year regional changes in the surface fluxes over oceans have also been used to assess changes in ocean energy fluxes for the same annual report. The data products are available through the “HDF” portion of the CERES ordering page or more directly through the FLASHFlux homepage: http://flashflux.larc.nasa.gov."

Summary  of  Changes  Between  Version  2H  and  Version  3A  

Version  2H     Version  3A    

Spectral  Correc4on  Coefficients  

CERES  Ed2   CERES  Ed3  

Solar  Constant   1365  W  m-­‐2   1361  W  m-­‐2  

Aerosols   WCP-­‐55   MATCH  Climatology  

Rayleigh  ScaEering   Original  LPSA    New  based  on  Bodhaine  et  

al.  (1999)  

Meteorology   GEOS-­‐5.2.0   GEOS  5.9.1  (FP-­‐IT)  

Temperature  Inversions   No  special  treatment   Improved  Algorithm    

Cloud  Transmission  Coefficient  

0.80   0.75  

B

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-180 -150 -120 -90 -60 -30 0 30 60 90 120 150 18048.31N, 105.10W Fort Peck, MT

40.72N, 77.93W Penn State, PA

40.05N, 88.37W Bondville, IL

40.13N, 105.24W Boulder, CO

34.25N, 89.87W Goodwin Creek, MS

43.73N, 96.92W Sioux Falls, SD

36.60N, 97.48W SGP ARM

45.03S, 169.7E New Zealand

44 N, 5.1E Carpentras, FR

48.71N 2.20W Palaiseau, FR

58.3N, 26.5E Toravere, Estonia

29.44S 53.82W São Martinho da Serra, Brazil

32.30N, 64.77W Bermuda

24.28N, 153.98E Minami-Torishima

2.06S, 147.42 E Manus

0.52S, 166.9 E, Nauru

12S 97E Cocos Isl

36.05N, 140.13E Tatano

36.9N, 75.71W Ches Light

51.97N, 4.9E Cabauw, Netherlands

12.43S, 130.8E Darwin, AU

33.58N, 130.37E Fukuoka, Japan

24.33N, 124.16E Ishigakijima,Japan

71.32N, 156.61W Barrow, AK

90.00S, 0.00 South Pole

69.00S, 39.58E Syowa

70.65S, 8.25W Georg von Neumayer

78.9N, 11.95E Ny Alesund

72.57N, !38.5W Greenland Summit

B 23.70S, 133.87E Alice Springs

J 36.63N, 116.02W Desert Rock, NV

H 22.78N, 5.52E Algeria

H 30.9N , 34.8E Sede Boger, Israel

H 23.56S, 15.04N Gobabeb Namib Desert

B 12.0N, 23.0W PIRATA Buoy

J 0.0N, 23W PIRATA Buoy

19.0S, 34W PIRATA Buoy

15.0N, 90.0E RAMA Buoy

0.00 80.5E RAMA Buoy

Locations of Ground Measurement Sites "

Sites Color-coded by Type"Surface Measurements from http://www-cave.larc.nasa.gov/"

Downward Shortwave Flux" Downward Longwave Flux"

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1 2 - 5 6 - 20 21 - 40 41 - 50 > 50

N = 6669Bias = -1.2 W m-2

R.E. = 32.2 W m-2

N = 6669Bias = -5.9 W m-2

R.E. = 33.2 W m-2

N = 6669Bias = -4.7 W m-2

R.E. = 13.7 W m-2

Version 2H Version 3A 3A vs 2HGlobal

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1 2 - 5 6 - 10 11 - 15 16 - 20 > 20

N = 829Bias = 15.7 W m-2

R.E. = 32.6 W m-2

N = 829Bias = 8.1 W m-2

R.E. = 34.4 W m-2

N = 829Bias = -7.6 W m-2

R.E. = 4.8 W m-2

Version 2H Version 3A 3A vs 2HIsland

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1 2 - 10 11 - 15 16 - 20 21 - 25 > 25

N = 2402Bias = -4.8 W m-2

R.E. = 24.7 W m-2

N = 2402Bias = -8.4 W m-2

R.E. = 26.4 W m-2

N = 2402Bias = -3.6 W m-2

R.E. = 6.8 W m-2

Version 2H Version 3A 3A vs 2HContinental

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1 2 - 10 11 - 15 16 - 20 21 - 25 > 25

N = 1246Bias = -5.9 W m-2

R.E. = 20.5 W m-2

N = 1246Bias = 0.6 W m-2

R.E. = 19.3 W m-2

N = 1246Bias = 5.2 W m-2

R.E. = 7.3 W m-2

Version 2H Version 3A 3A vs 2HDesert

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1 2 - 5 6 - 10 11 - 15 16 - 20 > 20

N = 1564Bias = 10.3 W m-2

R.E. = 24.2 W m-2

N = 1564Bias = 0.3 W m-2

R.E. = 24.8 W m-2

N = 1564Bias = -9.9 W m-2

R.E. = 7.8 W m-2

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Ground Measured DSF (W m-2)

1 2 - 5 6 - 10 11 - 15 16 - 20 > 20

N = 630Bias = -28.9 W m-2

R.E. = 55.8 W m-2

N = 630Bias = -40.8 W m-2

R.E. = 54.8 W m-2

N = 829Bias = -11.9 W m-2

R.E. = 34.0 W m-2

Version 2H Version 3A 3A vs 2HHigh Latitude

Introduction :! The Fast Longwave and Shortwave Radiative Flux (FLASHFlux) data product was developed to provide a rapid release version of the Clouds and Earth's Radiant Energy System (CERES) results, which could be made available to the research and applications communities within one week of the satellite observations by exchanging some accuracy for speed of processing. Unlike standard CERES products, FLASHFlux does not maintain a long-term consistent dataset. Therefore the latest changes in algorithms and input data can be incorporated into processing. FLASHFlux transitioned from Version 2H to Version 3A in January 2013 changing to the latest meteorological product from Global Modeling and Assimilation Office (GMAO), GEOS FP-IT (5.9.1), latest spectral response functions and gains for the CERES instruments, and aerosol climatology based on the latest MATCH data. Some algorithm changes were made in the cloud transmission coefficient and Rayleigh attenuation for the shortwave flux computation. Typically FLASHFlux does not reprocess when a new version is released. However, in order to investigate the effects of the changes in algorithms and input data, nine months (201207 – 201303) were processed with both Version2H and Version3A. The Time Interpolated Space Averaged (TISA) surface flux results from these overlap months have been compared to the ground-based measurements. The effects of the changes on the calculated surface fluxes were evaluated. "

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N = 8423Bias = -1.4 W m-2

R.E. = 17.0 W m-2

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R.E. = 18.1 W m-2

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R.E. = 11.8 W m-2

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N = 829Bias = 15.7 W m-2

R.E. = 32.6 W m-2

N = 829Bias = 8.1 W m-2

R.E. = 34.4 W m-2

N = 829Bias = -7.6 W m-2

R.E. = 4.8 W m-2

Version 2H Version 3A 3A vs 2HIsland

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N = 1246Bias = -5.9 W m-2

R.E. = 20.5 W m-2

N = 1246Bias = 0.6 W m-2

R.E. = 19.3 W m-2

N = 1246Bias = 5.2 W m-2

R.E. = 7.3 W m-2

Version 2H Version 3A 3A vs 2HDesert

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N = 1179Bias = 7.3 W m-2

R.E. = 18.2 W m-2

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R.E. = 17.7 W m-20

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Acknowledgements: !

The CERES FLASHFlux data products are part of the CERES production system and we acknowledge the CERES working groups at LaRC for their role in providing algorithms and the Atmospheric Science Data Center (ASDC) for their role in providing mechanisms to archive and distribute the data products."

Comparison to Ground Measurements Comparison to Ground Measurements"