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Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 1 AE Mode Dec06 Anu Dudhia University of.

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Presentation on theme: "Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 1 AE Mode Dec06 Anu Dudhia University of."— Presentation transcript:

1 Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 1 AE Mode Dec06 Anu Dudhia University of Oxford

2 Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 2  26-29 Dec 2006 mixed NOM and AE mode data  Single L1B files contain complete orbit (unlike orig May’05)

3 Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 3

4 Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 4  26-29 Dec 2006 mixed NOM and AE mode data  Single L1B files contain complete orbit (unlike orig May’05)  There might be a problem with AE mode being activated while still viewing along track (to be confirmed)  Also: last sweep of last scan of each orbit flagged as corrupt

5 Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 5

6 Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 6

7 Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 7

8 Atmospheric, Oceanic & Planetary Physics, University of Oxford A Dudhia MIPAS ST5 Granada 25-26 Jan 2007 Page 8 Still appear to have the same problems with AE mode as in original May’05 data:  L1B (engineering) altitudes are 2 km lower than given in mission planning document (5,7.5…km instead of 7,8.5…km)  Actual tangent altitudes (based on retrieved tangent pressure) appear to be 5 km higher than L1B altitudes Conclusions

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