Intercomparison of SEVIRI data from MSG1 and MSG2 and implications for the GERB data processing

download Intercomparison of SEVIRI data from MSG1 and MSG2 and implications for the GERB data processing

If you can't read please download the document

description

Nicolas Clerbaux & RMIB GERB Team. GIST 26, RAL 3 and 4 May 2007. Intercomparison of SEVIRI data from MSG1 and MSG2 and implications for the GERB data processing. MSG1 -> MSG2 transition. New GERB instrument but also new SEVIRI imager Are the SEVIRI scene identifications consistent? - PowerPoint PPT Presentation

Transcript of Intercomparison of SEVIRI data from MSG1 and MSG2 and implications for the GERB data processing

  • Intercomparison of SEVIRI data from MSG1 and MSG2 and implications for the GERB data processingNicolas Clerbaux & RMIB GERB Team.

    GIST 26, RAL

    3 and 4 May 2007

  • MSG1 -> MSG2 transitionNew GERB instrument but also new SEVIRI imager

    Are the SEVIRI scene identifications consistent?GERB unfilteringGERB SW ADM selectionGERB LW angular modelling GERB scene identificationGERB dust flag and AOD retrieval

    Are the GERB-likes (SEVIRI NB-to-BB) consistent?RGP GERB geolocationGERB unfilteringGERB resolution enhancementuse of GERB-like data for monthly means

  • Structure of the talkIntercomparison of level 1.5 SEVIRI datareflectance for visible channelsBT and radiance for thermal channels

    Intercomparison of GERB scene identificationcloud fraction, cloud optical depth cloud phaseclear sky reflectanceLW anisotropic factordust flag and AOD retrieval

    Intercomparison of the GERB-like BB quantitiessolar and thermal radiancessolar and thermal fluxes

    Conclusions

  • The MSG1 and MSG2 data look very similar... natural colorair mass

  • Visible bands spectral response and effective central wavelength for MSG-1 and MSG-2MSGs=0.639mMSG2s=0.640m

    MSGs=0.809mMSG2s=0.807m

    MSGs=1.635mMSG2s=1.635m

  • 0.6 m reflectance intercomparisonratio MSG2/MSG1

  • 0.6 m reflectance intercomparison saturations for MSG2Max 0.6 m reflectance at nadir and d=1 A.U. is

    MSG1 : 1.082

    MSG2 : 0.942

    Software fix: accept saturation if SZA

  • 0.8 m reflectance intercomparisonratio MSG2/MSG1

  • 1.6 m reflectance intercomparisonratio MSG2/MSG1

  • 6.2 m brightness temperature intercomparisonratio MSG2/MSG1

  • 7.3 m brightness temperature intercomparisonratio MSG2/MSG1

  • 8.7 m brightness temperature intercomparisonratio MSG2/MSG1

  • 9.7 m brightness temperature intercomparisonratio MSG2/MSG1

  • 10.8 m brightness temperature intercomparisonratio MSG2/MSG1

  • 12 m brightness temperature intercomparisonratio MSG2/MSG1

  • 13.4 m brightness temperature intercomparisonratio MSG2/MSG1

  • Spectral radiance comparison

    ratio MSG2/MSG1WV 6.2 : 1.002WV 7.3 : 0.992IR 8.7 : 0.999IR 9.7 : 0.994IR 10.8 : 1.000 IR 12.0 : 0.996IR 13.4 : 0.974

    -> in general MSG-2 is close or a bit lower than MSG-1, CO2 is significantly lower

  • Summary for level 1.5 MSG-2/MSG-1 intercomparisonvisible 0.6m and 0.8m channels : 1 to 2% higher reflectancenear IR channel (1.6m): very closethermal channels: very close or a bit lower except the CO2 channel (13.4m) which is significantly colder (0.5% in BT , 2.5% in radiance)

    0.6m is often saturated over thick cloudresidual stripes in the WV 6.2m channel

  • Intercomparison of scene identificationsurface type is exactly the same (same rectification grid)cloud fractioncloud optical depthcloud phaseclear sky reflectance imagesLW angular modelingHelen Brindley 's dust flagAerosol retrieval with Ignatov look-up-table for the 0.6m, 0.8m and 1.6m channels

  • Cloud fraction

  • Cloud optical depth (log)

  • Cloud phase (0=pure water 1=pure ice)

  • Clear sky reflectance intercomparison (ratio to model)VIS 0.6VIS 0.8

  • LW ADM due to the change in NB radiances F=p L / R(q,L6.2, L10.8, L12,L13.4) FMSG1'/FMSG1

    Ratio of the flux for a same BB radiance L but for simulated differences between MSG1 and MSG2 NB radiances in the 6.2m, 10.8m, 12m, 13.4m channels

    Small increase of the anisotropy (0.2%).

  • Dust FlagMSG2MSG1

  • AOD in 0.6 m channel

  • AOD in 0.8 m channel

  • AOD in 1.6 m channel

  • Summary for scene identificationcloud fraction very similarcloud optical depth slightly higher (2%) due to the 0.6m and 0.8m reflectancescloud phase very similarLW angular modelling close, small difference in the good direction (increase of the limb-darkening). dust flag may differ in some semi-transparent situations AOD 2% higher at 0.6m , 0.6% higher at 0.8 m and 1.6% lower at 1.6 m. Ratio of AOD does not correspond to ratio in reflectance.

  • Intercomparison of broadband quantitiesGERB-like BB radiances (NB->BB)reflected solaremitted thermal

    GERB-like BB fluxes (NB->BB + ADMs) reflected solaremitted thermal

  • GERB-like Reflected Solar Radiance

  • GERB-like Emitted Thermal Radiance

  • GERB-like Reflected Solar Fluxratio MSG2/MSG1

  • GERB-like Emitted Thermal Fluxratio MSG2/MSG1

  • Summary for the broadband productssolar radiance MSG2/MSG1 = 1.012thermal radiance MSG2/MSG1 = 0.9964solar flux MSG2/MSG1 = 1.012thermal flux MSG2/MSG1 = 0.9954

  • Conclusions and future workstart of GERB-1 processing with SEVIRI on MSG2good consistency with MSG1, most of the differences are explained by the level 1.5 SEVIRI data intercomparison,GERB-like radiances and fluxes are a bit closer to the actual GERB productsTo be done: analysis of the influence of the SEVIRI radiance definition (change from spectral radiance to effective radiance in April 2008).