Presentation is loading. Please wait.

Presentation is loading. Please wait.

Atmospheric Environment Characterization in Support of the ESA ExoMars Mission Intercomparison LMD – SwRI models T. Bertrand, S. Rafkin, F. Forget, A.

Published byEleanore Preston Modified over 9 years ago

Similar presentations

Presentation on theme: "Atmospheric Environment Characterization in Support of the ESA ExoMars Mission Intercomparison LMD – SwRI models T. Bertrand, S. Rafkin, F. Forget, A."— Presentation transcript:

1 Atmospheric Environment Characterization in Support of the ESA ExoMars Mission Intercomparison LMD – SwRI models T. Bertrand, S. Rafkin, F. Forget, A. Spiga, E. Millour

2 Project status November – start Phase 1 : LMD built 1D version for SWRI for radiative transfer synchronisation LMD sent reference profiles December First SWRI profiles received Solving reference time issues (bug, LTST vs LMST, UT versus LT) Investigation on surface temperature disagreement Problem of shortwave flow LMD found a bug in SWRI latitude Tuning the right options in both model (philosophy: LMD fit SWRI)

3 Project status January Comparison of 1D reference profiles with dust opacities at 0.2, 1, 5 LMD tries to match SWRI dust radiative effects and radiative models by tuning: 1.Dust opacity 2.Dust visible single scaterring albedo ("brightness of the dust") 3.Dust thermal infrared opacity vs visible opacity

4 Radiative transfer setting – 1D configuration Note : the radiative transfer model used by SWRI (NASA Ames) is known to underestimate dust heating rates. They partly compensate that by using "dark" dust radiative properties. 1D Run parameters – 6 cases:  Comparison LMD – SwRI without tunning  Comparison LMD – SwRI with tunning of dust properties

5 Comparison LMD – SwRI without tunning Surface flux SW

6 Comparison LMD – SwRI without tunning Surface flux LW

7 Comparison LMD – SwRI without tunning Surface temperature

8 Comparison LMD – SwRI without tunning Temperature profiles

9 Comparison LMD – SwRI without tunning Temperature profiles

10 Comparison LMD – SwRI without tunning Temperature profiles

11 Comparison LMD – SwRI without tunning Temperature profiles

12 Comparison LMD – SwRI without tunning Temperature profiles

13 Comparison LMD – SwRI without tunning Temperature profiles

14 Sensibility to dust opacity Temperature profiles

15 Sensibility to dust opacity Temperature profiles

16 Sensibility to dust opacity Temperature profiles

17 Sensibility to dust brightness Temperature profiles

18 Sensibility to dust brightness Temperature profiles

19 Sensibility to dust brightness Temperature profiles

20 Sensibility to ratio dust thermal IR vs VIS opacity Temperature profiles

21 Fitting C1 case with the three parameters Temperature profiles

22 BEST FITS – Case A1 Temperature profiles

23 BEST FITS – Case A1 Surface temperature

24 BEST FITS – Case B1 Temperature profiles

25 BEST FITS – Case B1 Surface temperature

26 BEST FITS – Case C1 Temperature profiles

27 BEST FITS – Case C1 Surface temperature

28 / Many plots available on: http://www.lmd.jussieu.fr/~tblmd/Intercomparison/1D_plots

29 Conclusion 1D comparisons are globally ok Turbulent diffusion scheme in the boundary layer: fundamental model differences that should be kept in the intercomparison ? Green light has been given to SwRI to start running GCM, Mesoscale and LES models.

Download ppt "Atmospheric Environment Characterization in Support of the ESA ExoMars Mission Intercomparison LMD – SwRI models T. Bertrand, S. Rafkin, F. Forget, A."

Similar presentations

A thermodynamic model for estimating sea and lake ice thickness with optical satellite data Student presentation for GGS656 Sanmei Li April 17, 2012.

A thermodynamic model for estimating sea and lake ice thickness with optical satellite data Student presentation for GGS656 Sanmei Li April 17, 2012.
Radiative transfer simulations of the ATR-42 and Falcon 20 SW and LW radiation profiles above the ENEA Lampedusa supersite during the ChArMEx/ADRIMED SOP1a.

Radiative transfer simulations of the ATR-42 and Falcon 20 SW and LW radiation profiles above the ENEA Lampedusa supersite during the ChArMEx/ADRIMED SOP1a.
Climate change in 19-22 centuries in observational and model data Evgeny Volodin, Institute of Numerical Mathematics RAS, Moscow, Russia.

Climate change in centuries in observational and model data Evgeny Volodin, Institute of Numerical Mathematics RAS, Moscow, Russia.
Low clouds in the atmosphere: Never a dull moment Stephan de Roode (GRS) stratocumulus cumulus.

Low clouds in the atmosphere: Never a dull moment Stephan de Roode (GRS) stratocumulus cumulus.
Solar constant The solar constant is the amount of incoming solar radiation per unit area, measured on the outer surface of Earth's atmosphere, in a plane.

Solar constant The solar constant is the amount of incoming solar radiation per unit area, measured on the outer surface of Earth's atmosphere, in a plane.
Incoming Solar (Shortwave) at TOA DecemberMarch JuneSeptember.

Incoming Solar (Shortwave) at TOA DecemberMarch JuneSeptember.
John J. Cassano - University of Colorado Wieslaw Maslowski -Naval Postgraduate School William Gutowski - Iowa State University Dennis Lettenmaier – University.

John J. Cassano - University of Colorado Wieslaw Maslowski -Naval Postgraduate School William Gutowski - Iowa State University Dennis Lettenmaier – University.
1. weather or climate ? Annual mean temperature (red is warm, blue cold)

1. weather or climate ? Annual mean temperature (red is warm, blue cold)
Radiative Properties of Clouds ENVI3410 : Lecture 9 Ken Carslaw Lecture 3 of a series of 5 on clouds and climate Properties and distribution of clouds.

Radiative Properties of Clouds ENVI3410 : Lecture 9 Ken Carslaw Lecture 3 of a series of 5 on clouds and climate Properties and distribution of clouds.
Why Laminar Flow in Narrow Channels (Heat Transfer Analysis)

Why Laminar Flow in Narrow Channels (Heat Transfer Analysis)
Heat Energy Solar and gravitational energy are the fundamental sources of energy for the Earth's climate system. Air-sea exchanges of heat (& freshwater)

Heat Energy Solar and gravitational energy are the fundamental sources of energy for the Earth's climate system. Air-sea exchanges of heat (& freshwater)
Simulate Urban-induced Climate Change Via EOS Observations and Land Surface Model Dr. Menglin Jin, Meteorology Dept, U University of Maryland, College.

Simulate Urban-induced Climate Change Via EOS Observations and Land Surface Model Dr. Menglin Jin, Meteorology Dept, U University of Maryland, College.
© Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony.

© Crown copyright Met Office Electromagnetic and light scattering by atmospheric particulates: How well does theory compare against observation? Anthony.
Matt Robinson Thomas Tolman.  Describes Convective Heat Transfer  Needed for all external and internal flow situations.

Matt Robinson Thomas Tolman.  Describes Convective Heat Transfer  Needed for all external and internal flow situations.
Earth-Atmosphere Energy Balance Earth's surface absorbs the 51 units of shortwave and 96 more of longwave energy units from atmospheric gases and clouds.

Earth-Atmosphere Energy Balance Earth's surface absorbs the 51 units of shortwave and 96 more of longwave energy units from atmospheric gases and clouds.
Pat Arnott, ATMS 749 Atmospheric Radiation Transfer Chapter 6: Blackbody Radiation: Thermal Emission Blackbody radiation or cavity radiation refers.

Pat Arnott, ATMS 749 Atmospheric Radiation Transfer Chapter 6: Blackbody Radiation: Thermal Emission "Blackbody radiation" or "cavity radiation" refers.
1 TEC-MTT/2012/3788/In/SL LMD1D v1 and v2 Comparison with Phoenix Flight Data Prepared by Stéphane Lapensée ESA-ESTEC, TEC-MTT Keplerlaan 1, 2201 AZ Noordwijk.

1 TEC-MTT/2012/3788/In/SL LMD1D v1 and v2 Comparison with Phoenix Flight Data Prepared by Stéphane Lapensée ESA-ESTEC, TEC-MTT Keplerlaan 1, 2201 AZ Noordwijk.
Radiative transfers in complex geometry for CFD modelling the urban canopy Maya Milliez.

Radiative transfers in complex geometry for CFD modelling the urban canopy Maya Milliez.
Mesoscale Modeling Review the tutorial at: –In class.

Mesoscale Modeling Review the tutorial at: –In class.
Ozone Creation. Chapter 4 Atmosphere and Surface Energy Balances Geosystems 6e An Introduction to Physical Geography Robert W. Christopherson Charles.

Ozone Creation. Chapter 4 Atmosphere and Surface Energy Balances Geosystems 6e An Introduction to Physical Geography Robert W. Christopherson Charles.

Similar presentations

Ads by Google