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Direct aerosol radiative effects based on combined A-Train observations Jens Redemann, Y. Shinozuka, J. Livingston, M. Vaughan, P. Russell, M.Kacenelenbogen,

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Presentation on theme: "Direct aerosol radiative effects based on combined A-Train observations Jens Redemann, Y. Shinozuka, J. Livingston, M. Vaughan, P. Russell, M.Kacenelenbogen,"— Presentation transcript:

1 Direct aerosol radiative effects based on combined A-Train observations Jens Redemann, Y. Shinozuka, J. Livingston, M. Vaughan, P. Russell, M.Kacenelenbogen, O. Torres, L. Remer BAERI – NASA Langley - NASA Ames – SRI – NASA Goddard http://geo.arc.nasa.gov/AATS-website/ email: Jens.Redemann-1@nasa.govJens.Redemann-1@nasa.gov

2 Outline   Goal: To devise a new, methodology to derive direct aerosol radiative effects -  F aerosol (z) based on CALIOP, OMI and MODIS   Motivation, data sets and role of field observations   Methodology for combining CALIOP, OMI and MODIS data   Checking consistency of input data   Proof of concept for 4-month data set – Jan., Apr., Jul., Oct. 2007   Impact of input data sets   Comparisons to AERONET and CERES flux products   Conclusions

3 MODIS OMI CALIOP Goal: To use A-Train aerosol obs to constrain aerosol radiative properties to calculate  F aerosol (z) Myhre, Science, July 10, 2009: 1) 1)Observation-based methods too large 2) 2)Models show great divergence in regional and vertical distribution of DARF. 3) 3)“remaining uncertainty (in DARF) is probably related to the vertical profiles of the aerosols and their location in relation to clouds”.

4 Target:  F aerosol (z) +  F aerosol (z) Constraints/Input: - MODIS AOD (7/2 ) +  AOD - OMI AAOD (388 nm) +  AAOD - CALIPSO ext (532, 1064 nm) +  ext - CALIPSO back (532, 1064 nm) +  back Goal: To use A-Train aerosol obs to constrain aerosol radiative properties to calculate  F aerosol (z) Retrieval: ext (, z) +  ext ssa (, z) +  ssa g (, z) +  g MODIS aerosol models: 7 fine and 3 coarse mode distribution models define size and refractive indices of bi-modal log-normal size distribution → 100 combinations Free parameters: N fine, N coarse Issues to consider - Differences in data quality land/ocean - - Impact of model assumptions - - Spatial variability - - Aerosols above & near clouds Rtx code

5 Methodology: Role of field observations Use suborbital observations to: 1) 1) Guide choices in aerosol models 2) 2)Test retrievals of aerosol radiative properties 3) 3)Test calculated radiative fluxes 4) 4)Study spatial variability = uncertainty involved in extrapolating to data- sparse regions (e.g., above clouds) See poster A43A-0127 Kacenelenbogen et al. Re 4): Shinozuka and Redemann, ACP, 2011

6 Solution space: expansion from over-ocean MODIS models

7 ARCTAS data are corrected after Virkkula [2010]. Role of suborbital observations: 1) Test realism of aerosol models

8 7 fine + 3 coarse modes SSA and EAELidar Ratio and EAE

9 : retrieved parameters : observables : uncertainties in obs. : weighting factors Current choices in retrieval method: 1) 1)Metric / error / cost function 2) 2)4 Observables x i = AOD 550nm (±0.03±5%) AOD 1240 nm (±0.03±5%) - MODIS AAOD 388 nm ±(0.05+30%) - OMI  532 ±(0.1Mm -1 sr -1 +30%), - CALIOP 3) 3)Minimize X and select the top 3% of solutions that meet for all i

10 Example of successful retrieval from actual collocated MODIS, OMI, CALIOP (V3) data: Oct. 23, 2007

11 Consistency issues: AOD comparisons (CALIOP V3)   Eight months of data: January, April, July and October 2007 and 2009   Use CALIOP 5/40km-avg. (V3/V2) aerosol extinction profiles, and 5km aerosol and cloud layer products   Find all instantaneously collocated, MODIS MYD04_L2 (10x10km) aerosol retrievals traversed by 5km/40km CALIPSO track   Judicious use of data quality flags   Break down geographically → zonal mean AOD   See Redemann et al., ACPD for details   See Kacenelenbogen et al., ACP 2011 for potential explanations for CALIOP-MODIS differences

12 Latitudinal distribution of AOD differences between MODIS and CALIOP V3 MODIS-CALIOP AOD Latitude Redemann et al., ACPD Main findings, ocean: 1. 1.bias differences of 0.03 - 0.04 (with CALIOP<MODIS for all months), 2. 2.RMS  of 0.09 – 0.12 3. 3.r 2 is ~ 0.4-0.5 …all after judicious use of quality flags Shinozuka and Redemann, ACP, 2011

13 OMAERUV (Torres group)OMAERO (KNMI group) AOD 380nm ssa 380nm Consistency issues: Choice of OMI data

14 OMAERO data collocated with MODIS and CALIOP is a reasonable representation of global OMAERO data OMAERUV data collocated with MODIS and CALIOP is a poor representation of global OMAERUV

15 OMAERO data collocated with MODIS and CALIOP is a reasonable representation of global OMAERO data OMAERUV data collocated with MODIS and CALIOP is a poor representation of global OMAERUV

16 Target:  F aerosol (z) +  F aerosol (z) Constraints/Input: - MODIS AOD (7/2 ) +  AOD - OMI AAOD (388 nm) +  AAOD - CALIPSO ext (532, 1064 nm) +  ext - CALIPSO back (532, 1064 nm) +  back Retrieval of aerosol radiative properties from A-Train observations Retrieval: ext (, z) +  ext ssa (, z) +  ssa g (, z) +  g MODIS aerosol models: 7 fine and 3 coarse mode distributions define standard deviation and refractive indices of bi-modal log-normal size distribution → 100 combinations Free parameters: N fine, N coarse Rtx code

17 Target:  F aerosol (z) +  F aerosol (z) Constraints/Input: - MODIS AOD (7/2 ) +  AOD - OMI AAOD (388 nm) +  AAOD - CALIPSO ext (532, 1064 nm) +  ext - CALIPSO back (532, 1064 nm) +  back Retrieval of aerosol radiative properties from A-Train observations Retrieval: ext (, z) +  ext ssa (, z) +  ssa g (, z) +  g MODIS aerosol models: 7 fine and 3 coarse mode distributions define standard deviation and refractive indices of bi-modal log-normal size distribution → 100 combinations Free parameters: N fine, N coarse Rtx code Comparison: CERES F clear Airborne F clear Comparison: AERONET AOD, ssa, g Airborne test bed data

18 AERONET Inversion collocation with MODIS-OMI(OMAERO)-CALIPSO AERONET V2.0 (circles): ~68,200 collocated MODIS- OMI-CALIPSO obs in 4 months of data 93-96% of those have valid MOC retrieval 576 of those have collocated AERONET AOD measurements (±100km, ±1h) Only 45 of those have collocated AERONET SSA (V2/L2) retrieval

19 The top 3% X for all 4 months. Xavg=0.1640 Xstd= 0.0968 Xavg+Xstd=0.2608

20 AOD and SSA retrievals from MODIS – OMI - CALIPSO AOD ~540nm SSA ~540nm

21 24h avg direct radiative forcing from MODIS – OMI - CALIPSO Surface TOA

22 Conclusions A.MODIS-CALIOP AOD comparisons: bias differences of 0.03 - 0.04 (CAL<MOD), RMS differences of 0.09 – 0.12 after judicious use of quality flags. B.A methodology for the retrieval of aerosol radiative properties from MODIS AOD, OMI AAOD and CALIOP  532 has been devised. Proof of concept study complete for January+April+July+October 2007: –Results sensitive to choice of OMI data (OMAERUV vs. OMAERO) –OMAERUV possibly more accurate, but data collocated with MODIS+CALIOP not representative of global OMAERUV data set –Tests with collocated AERONET observations sparse –Tests with CERES irradiance measurements difficult to interpret C.Next questions to answer: 1)What is the trade-off between uncertainty and spatial sampling in input satellite data sets for calculating aerosol-induced changes in TOA or surface fluxes, i.e., how much uncertainty is involved in spatial extrapolation to data-sparse regions? 2)How to test the “consistency” between various satellite input data sets? 3)How do uncertainties in satellite data propagate to retrievals and flux estimates? D.Next steps to take: 1)Continue to investigate spatial variability in suborbital data to extend the MOC retrievals to aerosol above cloud (AAC) based on reduced data set 2)Extend study to use more MODIS channels and more OMI retrievals 3)Constrain OMI AAOD retrievals with CALIOP height input 4)Compare vertical distribution of direct forcing to models


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