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Determination of atmospheric temperature, water vapor, and heating rates from mid- and far- infrared hyperspectral measurements

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Title: Determination of atmospheric temperature, water vapor, and heating rates from mid- and far- infrared hyperspectral measurements


1
Determination of atmospheric temperature, water
vapor, and heating rates from mid- and far-
infrared hyperspectral measurements
  • AGU Fall Meeting, Wednesday, December 12, 2007
  • GC34A-02
  • D.R. Feldman (Caltech)
  • K.N. Liou (UCLA) Y.L. Yung (Caltech)
  • D. G. Johnson (LaRC) M. L. Mlynczak (LaRC)

2
Presentation Outline
  • Motivation for studying the far-infrared
  • FIRST instrument description
  • Sensitivity tests of mid-IR vs far-IR
    capabilities
  • Clear-sky
  • Cloudy-sky
  • Multi-instrument data comparison
  • Climate model considerations
  • Conclusions
  • Outline

3
The Far-Infrared Frontier
  • Current EOS A-Train measure 3.4 to 15 µm, dont
    measure 15-100 µm
  • IRIS-D measured to 25 µm in 1970
  • Far-IR, through H2O rotational band, affects OLR,
    tropospheric cooling rates
  • Far-IR processes inferred from other spectral
    regions
  • Mid-IR, Microwave, Vis/NIR
  • Interaction between UT H2O and cirrus clouds
    requires knowledge of both
  • Currently inferred from measurements in other
    spectral regions

No spectral measurements to the right of line
Figures derived from Mlynczak et al, SPIE, 2002
  • Motivation

4
FIRST Far Infrared Spectroscopy of the
Troposphere
  • FTS w/ 0.6 cm-1 unapodized resolution, 0.8 cm
    scan length
  • Multilayer beamsplitter
  • Germanium on polypropylene
  • Good performance over broad spectral ranges in
    the far-infrared
  • 5-200 µm (50 2000 cm-1) spectral range
  • NeDT goal 0.2 K (10-60 µm), 0.5 K (60-100 µm)
  • 10 km IFOV, 10 multiplexed detectors
  • Cooling
  • Spectrometer LN2 cooled
  • Detectors liquid He cooled
  • Scan time 1.4-8.5 sec
  • Balloon-borne ground-based observations
  • FIRST instrument

5
Retrieval Sensitivity TestFlow Chart
Random Perturbations
Model Atmosphere
A priori Atmospheric State)
RTM
RTM Noise
A priori uncertainty
A priori spectrum
Synthetic Measurement
Retrieval algorithm
Analyze retrieved state, spectra, and associated
statistics
  • Sensitivity tests

6
Clear-Sky Retrieval Test
  • AIRS and FIRST T(z) retrievals comparable.
  • FIRST better than AIRS in H2O(z) retrievals
    200-300 mbar.
  • Residual signal in far IR seen 100-200 cm-1 ?
    low NeDT critical
  • Sensitivity tests

7
Clear-Sky Heating Rates
Tropical Conditions
Sub-Artic Winter Conditions
  • Spectra provide information about fluxes/heating
    rates
  • Error propagation (Taylor et al, 1994 Feldman et
    al, In Review) can be used
  • Heating rate error for scenes with clouds
    generally higher due to lack of vertical cloud
    information
  • Heating Rates

8
Extrapolating Far-IR with Clouds
  • Retrieval of T(z), H2O(z), CWC(z), CER(z)
    difficult with AIRS spectra
  • Use AIRS channels to extrapolate far-IR channels?
  • Depends on cloud conditions, T(Z), H2O(z)
  • Low BT channels from 6.3 µm band low BT
    channels in far-IR
  • High BT channels scale from mid- to far-IR
  • For tropics, channels with BT 250-270 K (emitting
    5-8 km) are complicated
  • Clouds

9
Test Flight on September 18, 2006Ft, Sumner NM
AQUA MODIS L1B RGB Image
AIRS Footprints
FIRST Balloon
CloudSat/CALIPSO Track
  • Test flight

10
CloudSat/CALIPSO signals
  • CloudSat and CALIPSO near collocation
  • No signal from CloudSat
  • CALIPSO signal consistent with FIRST residual
  • Test flight

11
FIRST and AIRS Cloud Signatures
  • Instrument collocation
  • FIRST balloon-borne spectra
  • AIRS
  • MODIS
  • Residuals are consistent with clouds 5 km, De
    60 µm

Cloud Detected !
  • Test flight

12
Climate Model Considerations
  • Climate models produce fields that specify mid-
    far-IR spectra.
  • Multi-moment statistical comparisons of measured
    spectra and modeled spectra avoid subtle biases
    from data processing.
  • Spectral and atmospheric state spaces should be
    considered jointly.
  • Far-IR climate model analysis requires more
    far-IR data
  • Far-IR extrapolation should retain physical basis
    and be verified with measurements.
  • Agreement with CERES is only partial verification
    and presents a non-unique checksum
  • Future work to assess how spectra impart
    information towards climate model processes.
  • Model evaluation

13
Conclusions
  • AIRS measures mid-IR, but far-IR is not covered
    A-Train spectrometers.
  • FIRST provides thorough description of far-IR but
    limited spectra are available.
  • FIRST clear-sky T retrievals comparable, improved
    UT H2O retrieval relative to AIRS
  • Implied cooling rate information difference is
    small .
  • Extrapolating far-IR channels good for Tb 220
    K, ok for Tb 300 K, difficult for Tb 250-270
    K.
  • Multi-instrument analysis with A-Train
    facilitates comprehensive understanding of FIRST
    test flight spectra.
  • AIRS mid-IR spectra can validate climate models,
    but far-IR should not be neglected.
  • Conclusions

14
Acknowledgements
  • NASA Earth Systems Science Fellowship, grant
    number NNG05GP90H.
  • Yuk Yung Radiation Group Jack Margolis, Vijay
    Natraj, King-Fai Li, Kuai Le
  • George Aumann and Duane Waliser from JPL
  • Xianglei Huang from U. Michigan and Yi Huang
    from Princeton
  • AIRS, CloudSat, and CALIPSO Data Processing Teams
  • Thank you for your time

15
Cloud Radiative Effect (CRE)
  • CRE TOA clear broadband flux TOA broadband
    flux
  • CERES provides collocated measurements of CRE
    from broadband radiometers
  • Most CERES products contain multiple data-streams
  • AIRS L3 CRE lower than CERES CRE
  • Other A-Train sets (CloudSat/CALIPSO) can
    arbitrate difference
  • Clouds

16
Towards CLARREO
  • NRC Decadal Survey recommended CLARREO for
  • Radiance calibration
  • Climate monitoring
  • CLARREO specified to cover 200 2000 cm-1 with lt
    2 cm-1 resolution
  • NIST traceability requirement
  • Prototyped far-IR instruments provide a science
    and engineering test-bed for next generation of
    satellite instruments
  • Further orbital simulations required to test how
    mid-IR state space uncertainties appear as far-IR
    spectral residuals
  • More integrated A-train analyses w.r.t. Far-IR
    warranted
  • Larger Far-IR dataset analysis needed to
    demonstrate utility of long wavelength
    measurements for climate monitoring
  • Dont forget about 50-200 cm-1 (200-50 µm).
  • Future directions
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