Minutes of the fourth International Radiative Transfer Workshop, July 2002

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-----===== TUESDAY 2002-07-09 =====-----

   a) Intercomparison paper
      
      The model named as MAES is in named in the plots as CRL and ss
      as FIP
     1.  case 0
       - Nikolay is giving description of the cases 
       - Moliere uses Kuntz implementation of the Voigt function.
       - DLR is not using the partition function but some software 
         called ATMOS so the line strength can be different.
         Franz is giving a short description of line strength
         calculation by ATMOS.
       * comment from Franz:
         + Kuntz is simply an optimized version of the Humlicek algorithm to
	   compute the Voigt profile / complex error function (Voigt=Re(cerf))
	   In general I use Humlicek as well, just with a different optimization.
	   for most of the case0 and 1 calculations submitted to Bremen, however, 
	   I used the wofz code of Poppe&Wijers which (according to the authors)
	   has an accuracy of 14 significant digits (Humlicek: 10^(-4)).
         + My line strength conversion is done according to the scheme
	   described in Norton&Rinsland:
	   @article{Norton91,
	    AUTHOR  = {R.H. Norton and C.P. Rinsland},
	    TITLE   = {ATMOS data processing and science analysis methods},
	    JOURNAL = AO,
	    VOLUME  = 30,
	    PAGES   = 389,
	    YEAR    = 1991}
           ATMOS is a FT spectrometer flown several times on the space shuttle.
           Atmospheric Trace Molecule Spectroscopy Experiment
           http://remus.jpl.nasa.gov




     2.  case-1A
       - Similar results as case0 except for FIP. 
       - Karlsruhe also uses ATMOS scheme for partition function
       
     3.  case-1B
       - MPM-93 has lot of discrepancies. 
     
     4.  case-2
       - Karlsruhe uses O2-Liebe98 model, so it can be the reason for
         discrepancy
       - Moliere uses MPM-93 for oxygen and nitrogen.
       - SMILES simulator is showing large discrepancy at higher alt.
     
     5.  case-3 Down
       - DLR and Moliere participate
       - coarse pressure grid and fine pressure grid:
         differences are some Kelvin (see paper)

     6.  case-3 Limb
       - In comparison with ARTS and MIRART ARTS is missing the
         peak(FS).
       
       
       - Deadline of the paper: August(to finalize the models and cases)
         and September(to do the final iteration of the results).
       - Wednesday there will be meeting people for each groups. 

     AMIL2DA(FS) 

       - Advanced MIPAS level 2 analysis (EU_FP5 project)
       - www.fzk.de/imk/imk2/ame/amil2da
       - main question:
         Are MIPAS level 2 data processed by different institutes/processors
	 comparable?
       - Strategy:
         1. forward radiative transfer model intercomparison
	 2. blind-test retrievals using synthetic spectra
         3. intercomparison of retrievals with real mipas data
       - Forward models:
         KOPRA (Karlsruhe), OFM (IROE, Florence), RFM (Oxford),  
         MIRART (FS), FM2D (RAL)
       - In the intercomp. 30 exercises each with only one spectra at one
         frequency range starting from simple settings and proceeding to 
         more complex/realistic cases.
       - non LTE implementation is also checked (Kopra and RFM only)
       - KOPRA is taken as the reference model
       - Transmission: large difference in the CO2 2400 - 2500 cm-1
         region (4 micrometer), 
         250mb, 256 K was coming from different line rejection criteria.
       - Radiance (incl. ILS and FoV effects):
         deviations for all models less than 1%
       - Blind test retrieval - first results:
         all codes giving reasonable/consistent results for ozone etc.


       
     Zeeman Splitting(NK)

       - contact Nikolay
       - Yasuko told BrO and ClO also has small Zeeman splitting
       - Ozone??

     RT through the atmosphere of other planets(JU)  

       - Moliere 
       - MAMBO - MARS ATMOSPHERIC MICROWAVE BRIGHTNESS TEMPERATURE
         EXPLORER, Limb looking 
       - Launch will be in sept 2007, Ariane5, arrival 2 years later
       - present and past Martian atm, temperature and winds, general
         circ, water cycle(0-60 km), photochemical state- CO, H2O2,
         surface(polarisation)
       - profiles H20 seasonal variation, temperature is decreasing
         with altitude
       - nadir operations also
       - Moliere is used to calculate spectra
       - wind is measured by Doppler shift in the CO line
       - Instrument description
       - different data levels upto level 4
       - mars radius - 3397?
       - ground pressure - 7hpa
       - H20 and CO2 continuum are implemented
       - LTE can be used???
       - surface emissivity can be a problem
       - strong variability of H2O can be a problem in the retrieval
       - retrieval of the temperature from two CO isotopes
       - for H2O 5 km grid is used
       - The first test retrievals shows temperature and water vapor
         can be retrieved, spectroscopy part is seemed to be more
         complicated

     Forward modeling in the Visible region(Ute)     
       
       - unpolarized source
       - Polarisation in remote sensing
       - Instruments: reflection, refraction, self polarisation
       - picture from POLDER to illustrate the effect of polarisation
       - polarising processes in nature:
	 - UV Rayleigh scattering

       - Rayleigh scattering - maximum at 90 degrees
       - scattering by cloud particles - degree of polarisation is
         very sensible to microphysics of the cloud
       - non sphericity can be measured through polarisation
       - reflection from sand is slightly polarised.
       - moist surfaces polarize more
       - polarized light from a canopy is coming from the specular
         reflection from the leaf surfaces	 
       - on water surface- Fresnel's law, angle dependence
       - ground is modeled as 
       - for aerosols types and optical thickness are retrieved

    ARTS Application

    Odin Inversions(PE)
     
       - Odin spectra
       - don't get exactly the pointing offset, has to be looked at
      
    Ground based inversions in Sweden(PE)
       
       - plot for measurements
       - mesospheric CO is measured
       - Vertical profiles of CO above Onsala, a downward transport of
         CO is seen
       - 

    SMILES Inversion(CV) 	 
	  
       - Instrumental description
       - three spectral bands
       - very low system noise temperature
       - nice spectrum
       - temperature retrieval is tried.
       - temperature weighting function(with and without HSE)
      
    AMSU Intercomparison(MK)

       - AMSU and Lindenberg data
       - comparison between ARTS and AMSU
       - plots for NOAA 15 and NOAA 16

    ARTS for AMSU(VOJ)

       - 

    Outgoing Longwave(SB/PE)

       - Balance of incoming and outgoing radiation
       - difference of real spectra from black body curve
       - plot of sensitivity to double H2O, maximum sensitivity 900
         hpa to 300 hpa
       - same plot for doubling of CO2, only in a narrow frequency
         range
       - H2O is more important than CO2.


    Tangent Linear and Adjoint Models(CM)

       - contact Christian
       - R M Errico "What is an adjoint model?" BAMS, 1997
       - C D Rodgers, "Inverse Methods for Atmospheric Sounding", 
         World Scientific, 2000.
       - Some web sites
       - Adjoint model compiler
       - Papers by .... told by Franz.
       Go to HTML and PDF version of the presentation.


    Retrieval Tool(PE)

       - Qpack
       - Implemented in matlab and uses ARTS as forward model
       - only OEM
       - example control file
       - How to call functions
       - creation of covariance matrices
       - Franz: 
         + PyReS: 'Python based retrieval system'
         + application: FOCUS, MIPAS, THOMAS,... 
         + forward models: MIRART, MODTRAN, .....
           (steered by PyReS using appropriate template file)
         + inversion codes: (standard) nonlinear least squares libraries, 
           Birger Schimpf's Tikhonov regularizatio code, ....
         + NOTE: only partially implemented right now 
           (currently works for Focus retrievals only)
       - Fully integrated systems: forward and inverse programs
         together: Moliere, Karlsruhe
      

    Retrieval Error Analysis for Spectroscopic Parameters(CV) 
       
       - Rodger's OEM algorithm
       - Linear mapping method
       - inverse model linearized around a priori state
       - OEM method will be better since the error covariance can be
         treated as Gaussian 

    Working Groups

       - intercomparison working group will be met and try to figure
         out problems regarding writing of the paper 
   


   ------------
   ACTION ITEMS
   ------------
   o Intercomparison paper:
     - iup/sat Bremen will unify the plotting style for all  the
       necessary plots of the paper
     - all participants of the intercomparison have to obey the 
       time schedule for the delivering of the model information 
       and final data sets.
     - main editor (one of the iup/sat Brmen member) of the paper 
       has to be named by iup/sat Brmen.
     - Franz will send the AMIL2DA paper and the template for the
       model description used in the AMIL2DA comparison to 
       iup/sat Bremen.
     
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