Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca 17-19 Mar 2008 Page 1 Recent MIPAS L2 Data Retrieved at Oxford.

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Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 1 Recent MIPAS L2 Data Retrieved at Oxford Anu Dudhia University of Oxford

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 2  Oxford processor MORSE uses same L1B/microwindows as ESA data, but optimal estimation algorithm.  Routinely processing all ESA L1B consolidated spectra (available about 2 weeks after acquisition)  Now also processing NRT data (available ~ hours after acquisition) - only NOM mode pT, H2O and O3 /

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 3 Temperature 10mb

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 4 Temperature 65S-90S 10mb

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 5 Temperature 65N-90N 10mb

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 7 Comparison of NRT and “Off-Line’’ Data  Identical OXF L2 processing used for both  Since NRT data started on 19 Feb 08 and latest OFL data completed for 24 Feb 08, only 6 days overlap so far

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 8 L1B Altitude

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 9 Temperature

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 10 Pressure

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 11 H2O

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 12 O3

Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST7 Salamanca Mar 2008 Page 13 NRT Data - Preliminary Conclusions  1 second difference in data  Small biases wrt OFL data  Surprisingly large scatter (~noise error)  Need to compare radiances

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