lessons learned with the airs hyperspectral sensor · asl overview rta update (sarta/kcarta)...
TRANSCRIPT
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL
Lessons Learned with the AIRSHyperspectral Sensor
L.Larrabee Strow
Atmospheric Spectroscopy Laboratory (ASL)UMBC Physics Department
and theJoint Center for Earth Systems Technology
April 26, 2006
Thanks to: ASL Group Members: Scott Hannon, Sergio De Souza-Machado, and
Howard Motteler.
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Overview
RTA update (SARTA/kCARTA)Non-LTEClear sky
Minor gases
Progress on detecting, modeling mineral dust withscattering RTA
Doing climate with hyperspectral sensors
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Bias summary of Non-LTE: Ignore black line
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Global Behavior of Non-LTE (July 1-15)
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Zoom of Bias and Std’s for Non-LTE
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Bias vs Solar Angle: No Non-LTE Fix
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Bias vs Solar Angle with Non-LTE Fix
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL15 µm Bias vs Solar Angle, No Non-LTEEmission
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL RTA Validation: AIRS Radiometric Stability: <0.01K/year
Work by H. Aumann (NASA/JPL)
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL SRF Shape (fringes) Introduce Bias: Understood, notfullly implemented
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Slight frequency shifts: Important for climate
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL A great RTA validation dataset exists
Table: Number sonde launches, LIDAR observations, coincident with AIRS.
Name Technique # of CoincidentSondes
ARM TWP Phase1 RS-90 154ARM TWP Phase2 RS-90 178ARM TWP Phase3 RS-90 163ARM SGP Phase1 RS-90 125ARM SGP Phase2 RS-90 171ARM SGP Phase3 RS-90 160Mcmillan/ABOVE RS-90 195Minnett RS-90 146aVömel FP 29Whiteman/LIDAR SRL 23
a. Includes RS-80 sondes not used here.
Table: Summary of number of clear observations over ocean at night.
Name % Clear # Sonde/LidarProfiles
ARM TWP 15 38Mcmillan/ABOVE 7 7Minnett 25 23
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL RS-90 Validation Campaign Bias Results
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL RS-90 vs ECMWF Biases: 24 Month Avg
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASLBUT (the bad news): We had to empiricallyadjust transmittances (using ARM-TWP 1)
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Adjustments in units of optical depths
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASLAdjustments in units of optical depths: Zoomof Fixed Gases (CO2)
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day/Night RS-90 and Frost-Point Differences
Mean night vs day biases for a. all RS-90 sondes, b. Vömel’s (NOAA/CMDL) frost-point hygrometers
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Minor Gases Impact RTA Validation
Minor gases need to be well understood to:1 Validate the RTA2 Use hyperspectral sensors for climate
Plus, we might find something interesting.
Stratospheric “interference” a big problem? (Especiallyimportant for polar work with hyperspectral.)
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Variable CO2: ECMWF for T(z)
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL And it’s global variation
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASLCO2 Variability Important for Weather andClimate
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Latest CO2 from AIRS, 38 Months: ∼25-45 Deg
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL CH4 Interferes with H2O
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL CH4
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Volcanic SO2 and Ash are seen
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May 2004 Monthly Means of HNO3
RTA modified to include variable HNO3
Used L2 retrievals, just varied scalar multiplier of HNO3
column
HNO3 unit is (observed column)/(reference column).Reference column is ≈ 1014 mol/cm2
Ocean only
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HNO3 Signal in Polar Granule Residuals
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Very Rough Validation versus MIPAS
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GEOS-CHEM: Sept. 20-21, 2004, 220 and 310 mbar
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GEOS-CHEM: Sept. 20-21, 2004, 430 and 600 mbar
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B(T) Influence for 1X Change in HNO3, Channel 1440
About 5 channels this sensitive189 AIRS channels have dB(T)/d(HNO3 = 1X) > 0.1K
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL AIRS Dust Observations: Scattering SARTA
We have observed many dust outbreaks, with quantitativeanalysis over oceans using SARTA-scattering
Paper in GRL on Medit. case (comparisons to MODIS)
Some differences in spectral structure (index of refraction)
Observed volcanic ash clouds
Hyperspectral IR sees dust througout tropical Atlantic insummer: Important to include in assimilation/retrieval forhurricane applications?
Developing a dust flag for next AIRS processing cycle. Hopefullyfuture reprocessing will include dust optical depth. More workneeded on how to handle dust vertical structure and interferingclouds.
SARTA/kCARTA now has scattering based on paper by Chou,Lee, Tsay, Fu; Parameterization for Cloud Longwave Scatteringfor use in Atmospheric Models in Journal of Climate, vol 12, pg159 (January 1999)
Two layer clouds possible, so can have water plus ice, or waterplus dust. Very fast with analytic Jacobians.
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Mediterranean Dust Storm
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASLDerived Optical Depths at 900 cm−1:Scattering SARTA
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL MODIS vs AIRS-derived Optical Depths
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Spectral Effects of Dust
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day 1: Dust Flag
May 2005 AIRS-STM
Global Score : July 16, 2005
SSM, UMBC 6
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day 2: Dust Flag
May 2005 AIRS-STM
Global Score : July 17, 2005
SSM, UMBC 7
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day 3: Dust Flag
May 2005 AIRS-STM
Global Score : July 18, 2005
SSM, UMBC 8
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day 4: Dust Flag
May 2005 AIRS-STM
Global Score : July 19, 2005
SSM, UMBC 9
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day 5: Dust Flag
May 2005 AIRS-STM
Global Score : July 20, 2005
SSM, UMBC 10
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day 6: Dust Flag
May 2005 AIRS-STM
Global Score : July 21, 2005
SSM, UMBC 11
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day 7: Dust Flag
May 2005 AIRS-STM
Global Score : July 22, 2005
SSM, UMBC 12
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Day 8: Dust Flag
May 2005 AIRS-STM
Global Score : July 23, 2005
SSM, UMBC 13
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April 8, 2006
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April 9, 2006
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April 10, 2006
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April 11, 2006
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April 12, 2006
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April 13, 2006
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April 14, 2006
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April 15, 2006
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April 16, 2006
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April 17, 2006
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April 18, 2006
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL AEROSE Dust StudyMay 2005 AIRS-STM
March 7, 2004 : (AEROSE) Duststorm off W.Africa
• “X” marks location of ship
• Lots of cloud contaminating the scene
• Weight ∆ BT(900cm-1,961 cm-1) more strongly
SSM, UMBC 18
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL AEROSE March 07, 2004
Left slide is false color visible image
Right slide is log10(red/blue), so higher values imply AIRSis looking at something other than warm blue ocean!
“X” marks position of ship
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL AEROSE March 07, 2004
Photometer indicates “dusty” skyCannot simultaneously fit AIRS and MAERI dataAlso might have sunglint problems??blue = obs, green = clear calc, red = cloudy calcAIRS sim : dust from 900 mb down, D ' 1.5 um,τ(900cm−1) ' 1.02MAERI sim : dust from 900 mb down, D ' 2.5 um,τ(900cm−1) ' 0.4
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Climate with Hyperspectral IR
Can we use hyperspectral IR sensors for climate studies
Lot’s of issuesSampling errors with clear?How do climate with cloudy FOVS?Tie sensor’s radiometric cal (AIRS to IASI to CrIS)Minor gasesDifferent spectral response functions
We have sub-setted “clear” ocean-only FOVS since AIRSstarted operation. Now have 38 month data set (alwaysgrowing).
A quick look at what this data set sees:
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASLBiases versus ECMWF have SST and TCW“retrieved”
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Bias/Obs Differences, ∆t = 2 Years: Mid Lat
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASLBias/Obs Differences, ∆t = 2 Years: MidLat:Zoom
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASLBias/Obs Differences, ∆t = 2 Years: MidLat:Zoom
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Bias/Obs Differences, ∆t = 2 Years: High Lat
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HyperspectralRTA
L. Strow
Non-LTEEmission
AIRS RTA andL1b Validation
Minor Gases
Dust:ScatteringApps
Climate withHyperspectralIR
ASL Conclusion
Doing climate with hyperspectral sensors will require a lot ofwork, but we have the capability to produce an excellentradiometric record with AIRS.
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