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EOS-Aura MLS Validation Using Radiosonde Profiles During the WAVES Campaign Cassie Stearns August 10,2006 Dr. Bojan Bojkov and Dr. David Whiteman, Advisors.

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Presentation on theme: "EOS-Aura MLS Validation Using Radiosonde Profiles During the WAVES Campaign Cassie Stearns August 10,2006 Dr. Bojan Bojkov and Dr. David Whiteman, Advisors."— Presentation transcript:

1 EOS-Aura MLS Validation Using Radiosonde Profiles During the WAVES Campaign Cassie Stearns August 10,2006 Dr. Bojan Bojkov and Dr. David Whiteman, Advisors

2 WAVES campaign, Howard University Research Campus, Beltsville MD Inter-instrumental Aqua/Aura Validation Campaign with 2 major ground components: –Meteorological balloon with:  Vaisala RS-92 and RS-80, ATM, Intermet, and MODEM for PTU  Electrochemical cell (ECC) ozonesondes  Cryogenic frost point hygrometer (CFH) for water vapor. –4 LIDAR systems for aerosols and 3 for water vapor

3 Weather Balloon with RS-92 CFH/ECC RS-92 ATM Intermet

4 Sonde Launches Coordinated with Aura

5 The Aura MLS (Microwave Limb Sounder) Instrument 20 second vertical scan (every ~1.5˚), 7 min ahead 5 spectral regions: 118,190,240,640,GHz; 2.5 THz Scan Values averaged and reported at 37 pressure levels 705 km orbit height

6 Typical temperature sounding (MLS vs RS92)

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9 MLS-Sonde ozone comparison

10 MLS-sonde T differences (preliminary) Few points High variability 215 hPa 146 hPa 10 hPa

11 MLS-sonde ozone differences (preliminary) High variability Few Points/Mechanical Uncertainty 146 hPa 10 hPa

12 Conclusions  The MLS profiles are in good agreement with the WAVES soundings, within uncertainty  Measurements are within error estimates specified in MLS documentation, including the temperature warm biases  210 and 146 hPa levels are heavily variable due to tropopause variation, and may fall outside expected error.  10 hPa level data contains fewer points of the RS-92 profile, and should be weighted less heavily; with the O3 sonde, there is also mechanical error introduced at low pressure.  Ongoing work: –Complete analysis to completed shortly (campaign is ongoing) –Aura HIRDLS and TES products to be investigated also

13 A Special Thanks to:  Dr. Bojan Bojkov, and Dr. David Whiteman, my advisors  Dr. Everett Joseph, Dr. Demetrius Venable, and the Howard University Beltsville crew  My fellow RS-92 radiosonde launchers: Eduardo, Ani, Scott, and Pat; and everyone else helping with WAVES!  UNH/GSFC Research and Discover Program

14 Questions?


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