1 / 16

Brewer Ozone Spectrophotometer

Brewer Ozone Spectrophotometer. Ozone Cross-section Issues. Vladimir Savastiouk Vitali Fioletov Tom McElroy. - Some points for discussion. Topics for Today. Ozone measurement methodology Differential cross-sections Instrumental stray light Progress on a Brewer relational database

jarvis
Télécharger la présentation

Brewer Ozone Spectrophotometer

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Brewer Ozone Spectrophotometer Ozone Cross-section Issues Vladimir Savastiouk Vitali Fioletov Tom McElroy - Some points for discussion

  2. Topics for Today • Ozone measurement methodology • Differential cross-sections • Instrumental stray light • Progress on a Brewer relational database • Implications for the WOUDC • Conclusions 13th Brewer Workshop

  3. Brewer Mathematics • Brewer ozone measurements are based on a differential measurement method using 4 wavelengths Absorption Function (of intensities on slits 3 to 6): F = -log(I3) + 0.5log(I4) + 2.2log(I5) -1.7log(I6) (Suppresses absorptions linear with wavelength, makes the result independent of absolute intensity is insensitive to SO2 and minimizes changes due to small wavelength shifts) • High-resolution laboratory cross-sections are used and effective cross-sections determined at each wavelength using accurate dispersion information and measured slit functions (ILS) for each instrument 13th Brewer Workshop

  4. Different Cross-sections • Differential cross-sections: dF/dozone = differential cross-section were computed using different laboratory data at various temperatures…. 13th Brewer Workshop

  5. Sciamachy Ozone These cross-sections agree with the composite ones very well on this plot. but the composite file seems to fit the data a little better. John Burrows’ group is looking at this comparison. But no news…. 13th Brewer Workshop

  6. EffectiveCross-sections 13th Brewer Workshop

  7. Differential Cross-sections for 32 Brewers GOME 10% Brion Sciamachy Bass & Paur 13th Brewer Workshop Temperature [C]

  8. Impact • Satellites determine the ozone profile including the height-dependent effects of temperature on apparent absorption • Columns are summed up from these data • Ground-based UV instruments directly infer a total column ozone • If the differential cross-section has a zero temperature coefficient the results will be temperature independent 13th Brewer Workshop

  9. The Brewers USE B&P at -45C! GOME 10% Brion Sciamachy Bass & Paur The Brewer is believed to produce ozone values with a small temperature dependence between -55 and -35 C based on the Bass & Paur data 13th Brewer Workshop Temperature [C]

  10. The Brewer • Because the Brewer characterizes its own ILS, each Brewer will have its own, accurate differential cross-section • This will be a primary reference for the satellite system 13th Brewer Workshop

  11. Calibrating Single Brewers • It has been demonstrated that Brewers can be independently characterized and absolutely calibrated and be in excellent agreement • This makes the absolute reference robust since it does not rely on one instrument remaining ‘stable’ 13th Brewer Workshop

  12. Agreement? • Some satellite data agree well with the Brewer data over a range of latitudes • But the cross-sections are different – the Brewer uses Bass & Paur (-45 C) currently • Satellite data may have been inadvertently ‘tuned’ to agree in the quest for better data • Also, there are systematic errors in both single Brewer data and Dobson data (AD) at large slant column amounts (e.g.: high latitude, winter) because of instrumental stray light 13th Brewer Workshop

  13. Conclusion • At this time it is not clear what cross-sections should be chosen • Very high spectral resolution is an advantage to bring together satellites, ground based and Lidar measurements • It is difficult, experimentally, to collect absolute cross-section data that can be ratioed with the accuracy needed to define consistent differential cross-sections with the required accuracy (for the Brewer, the absolute cross-section at the shortest wavelength is about 5 times larger than the differential cross-section) 13th Brewer Workshop

  14. Data Handling • Changes to both Brewer and Dobson data are likely to be required • Brewer data should also be recalculated with instrument-specific weighting coefficients • The Dobson and Brewer data will likely be dependent to some degree on the local ozone profiles and temperature profiles 13th Brewer Workshop

  15. WOUDC • Database capable of multiple versions of the data required • Transparency with respect to correction algorithms • Track method used for the re-analysis of each station’s data • In order of priority: • Resubmit corrected data • Reprocess from raw data at the WOUDC • Correct data in the WOUDC 13th Brewer Workshop

  16. The End Thank you…. 13th Brewer Workshop

More Related