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ASL AIRS contributions Using AIRS data in the presence of dust L2 - PowerPoint PPT Presentation

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ASL AIRS contributions Using AIRS data in the presence of dust L2 : dust impact OLR forcing : Fast estimate February 2007 Sergio DeSouza-Machado and Larrabee Strow duststorm Future Work Conclusions Atmospheric Spectroscopy Laboratory

  1. ASL AIRS contributions Using AIRS data in the presence of dust L2 : dust impact OLR forcing : Fast estimate February 2007 Sergio DeSouza-Machado and Larrabee Strow duststorm Future Work Conclusions Atmospheric Spectroscopy Laboratory (ASL) University of Maryland Baltimore County Physics Department Backup slides and the Joint Center for Earth Systems Technology ASL Group Members : Scott Hannon, Breno Imbiriba, Howard Motteler April 15, 2008 1 / 44

  2. ASL Introduction AIRS can play major role in addressing the largest uncertainty in atmospheric radiative forcing a/c to IPCC AIRS 2007 report: aerosol radiative forcing. contributions L2 : dust Ignoring dust is impacting AIRS L2 products during impact important weather/climate events. OLR forcing : Fast estimate Validation: UMBC dust optical depth retrievals compare February 2007 duststorm very well against other A-Train instruments (MODIS, Future Work CALIPSO, OMI and PARASOL). AIRS can often retrieve Conclusions reasonable dust heights, although climatology will work Backup slides for dust radiative forcing. We have a win-win situation, we improve standard L2 products while producing an important component of a new, very important climate measurement that is highly uncertain: longwave dust radiative forcing. 2 / 44

  3. ASL IPCC Radiative Forcings AIRS contributions L2 : dust impact OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 3 / 44

  4. ASL Unique AIRS Contributions AIRS can detect and retrieve dust day or night (unlike other instruments) AIRS contributions AIRS has some sensitivity to dust height, but OLR forcing L2 : dust and L2 retrievals relatively insensitive to height, unlike impact dust optical depth. OLR forcing : Fast estimate AIRS dust detection (flag) works well over clear ocean February 2007 duststorm (which happens quite often) and reasonably well over land Future Work (will improve with better emissivity product). MODIS and Conclusions OMI have higher sensitivities, but that is relatively Backup slides unimportant for dust radiative forcing. MODIS Deep Blue has problems over bright surfaces (deserts) and OMI may not detect low-altitude dust. AIRS retrieved ODs compare very well with other A-Train instruments 4 / 44

  5. ASL Approach for AIRS L2 : Dust affecting atmospheric profiles Retrieve dust optical depths from cloud-cleared radiances AIRS to improve L2 products, esp. SST,LST. contributions BUT, dust optical depths retrieved in this fashion may be of L2 : dust impact little scientific use - cloud clearing “removes” OLR forcing : in-homogenous component of dust. Fast estimate Only done on FOVs where dust flag is set February 2007 duststorm L2 : OLR forcing for climate Future Work This product is similar to existing AIRS cloud products Conclusions If dust flag is set using CC’d radiances, then Backup slides Examine 3x3 L1B FOVs for dust, and if evident Retrieve dust optical depth if clear enough, (not required!!) Then compute OLR dust forcing = R_Observed - R_Computed (with no dust, but using L2 clear and cloudy products). Very simple if dust has not contaminated cloud retrievals. If so, need to avoid dust channels for cloud retrieval (use 1231 cm − 1 for window channel for example). Most dust observations, and radiative forcing, are under otherwise clear conditions. 5 / 44

  6. ASL How does dust affect AIRS L2 products? Large duststorms can have uniform enough dust to adversely impact AIRS retrievals AIRS This is an issue for L2 products, and needs to be contributions L2 : dust considered for L2 improvements impact About 10% AIRS observations in certain regions can be OLR forcing : Fast estimate dust contaminated seasonally eg Atlantic during hurricane February 2007 duststorm season, Pacific in spring time Future Work Examining AIRS L2 products shows retrievals avoid dust Conclusions regions and/or do not retrieve all the way to the surface Backup slides Improve AIRS retrieval products by including dust as a retrieved variable in the future (probably not feasible for v6) easiest done on cloud cleared radiances? (needs to be tested) BUT nonuniform dust will be removed from the radiances, so this would lead to physically inaccurate dust optical depths 6 / 44

  7. ASL Looking at AIRS L2 in presence of dust UMBC retrievals used Optimal Estimation to simultaneously retrieve AIRS Temperature upto 200 mb (ECMWF first guess) contributions Water vapor upto 200 mb (ECMWF first guess) L2 : dust impact Surface Temperature (ECMWF first guess) OLR forcing : Dust loading (UMBC first guess) Fast estimate Dust top height (GOCART climatology or CALIPSO) February 2007 duststorm Dust effective diameter (4 um first guess) Future Work 1d VAR method Conclusions ≃ 1 minute per profile Backup slides 7 / 44

  8. ASL Looking at AIRS L2 in presence of dust AIRS L2 retrievals chosen had Quality Flags set good or best for AIRS Cloud_OLR contributions Temp_Profile_Bot L2 : dust impact H2O OLR forcing : Surf (not used in some plots) Fast estimate Guess_PSurf February 2007 duststorm Future Work Conclusions Backup slides 8 / 44

  9. ASL Feb 24, 2007 : Area coverage and biases Left plot shows retrieved τ( 900 cm − 1 ) Right plot shows biases and std deviations over the channels AIRS used contributions L2 : dust impact OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 9 / 44

  10. ASL Feb 24, 2007 : Area coverage Left plot shows retrieved τ( 900 cm − 1 ) Right plot shows coincident AIRS retrievals (Red = surface AIRS quality best or good, Blue = ignore surface quality) contributions L2 : dust (far fewer FOVs!) impact OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 10 / 44

  11. ASL Feb 24, 2007 : T(z) and Q(z) Solid = mean, dashed = std deviation Crosses show the position of the mean dust layer AIRS Blue = UMBC compared to ECMWF contributions Red = “Good2Surface” AIRS L2 compared to ECMWF L2 : dust impact AIRS L2 is much drier in trop, and much cooler at surface OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 11 / 44

  12. ASL Feb 24, 2007 : Stemp and colwater Histograms of SST differences and col water ratios (upto 200mb) AIRS Blue = UMBC compared to ECMWF contributions Red = “Good” AIRS L2 compared to ECMWF L2 : dust impact AIRS L2 has higher SST, and is overall drier OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 12 / 44

  13. ASL Feb 24, 2007 : Stemp grids Left = ECMWF, top right = AIRS, bottom right = UMBC AIRS contributions L2 : dust impact OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 13 / 44

  14. ASL Feb 24, 2007 : Col Water grids Left = ECMWF, top right = AIRS, bottom right = UMBC AIRS contributions L2 : dust impact OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 14 / 44

  15. Outgoing Longwave Radiation and ASL Clouds/Aerosols Aerosols and clouds affect outgoing radiation eg look at Tropical Profile with dust and cirrus AIRS SW forcing can be about ≃ 10 W/m2 contributions L2 : dust OLR forcing over ocean can be ( ≃ 5 W/m2) impact OLR forcing over land can much larger ( ≃ 20 W/m2) OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 15 / 44

  16. ASL OLR forcing over land/sea Feb 2007 over Sahara (L) over Med Sea (R) over land and sea the dots are coded according to (L) latitude (R) land fraction AIRS contributions L2 : dust impact OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 16 / 44

  17. ASL Feb 24, 2007 : OLR forcing Histograms of OLR(obs) - OLR(calc) AIRS L2 “Good2Surface” has almost zero dust forcings while AIRS UMBC, ECMWF have negative dust forcings contributions L2 : dust impact OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 17 / 44

  18. ASL List of collaborators to be submitted to JGR soon AIRS : Sergio DeSouza-Machado, Larrabee Strow, Scott AIRS contributions Hannon, Breno Imbiriba L2 : dust Dept of Physics and JCET, UMBC impact OLR forcing : CALIPSO : Kevin McCann and Ray Hoff Fast estimate Dept of Physics and JCET, UMBC February 2007 duststorm PARASOL : D. Tanré, J.L. Deuzé, F. Ducos Future Work Atmospheric Laboratory of Optics, Universite of Sciences Conclusions and Technologies of Lille, Lille, France Backup slides MODIS : J. Vanderlei Martins Dept of Physics and JCET, UMBC OMI : Omar Torres Department of Atmospheric and Planetary Sciences, Hampton University, VA 18 / 44

  19. ASL The A Train AIRS contributions L2 : dust impact OLR forcing : Fast estimate February 2007 duststorm Future Work Conclusions Backup slides 19 / 44

  20. ASL Instrument Characteristics AIRS Instrument Footprint Retrieval Swath Available Retrieval contributions (km) (km) (km) channels reported at L2 : dust 900 cm − 1 AIRS 15 15 2000 IR impact CALIPSO 0.1 15 0 532,1064 nm 532 nm OLR forcing : MODIS 1 10 2330 Vis,NIR,IR 550 nm Fast estimate PARASOL 7x6 20 2400 UV, Vis,NIR 865 nm February 2007 duststorm OMI 13 × 24 13 × 24 2600 UV 500 nm Future Work AERONET point point ground VIS 550 nm Conclusions Backup slides 20 / 44

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