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Cross Evaluation of OMI, TES, and GEOS-Chem Tropospheric Ozone

Xiong Liu1, Lin Zhang2, Kelly Chance1, John R. Worden3, Kevin W. Bowman3, Thomas P. Kurosu1, Daniel J. Jacob2

1 Harvard-Smithsonian Center for Astrophysics

2 Harvard University

3 Jet Propulsion Laboratory

3rd GEOS-Chem Users’ Meeting 2007

Harvard University

April 11, 2007

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Outline

  • Motivation
  • TES retrievals and GEOS-Chem simulation
  • Preliminary OMI ozone profile retrievals
  • Comparison methodology
  • OMI/TES/GEOS-Chem comparison
  • Summary

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Motivation

  • Tropospheric ozone retrievals can be greatly improved with joint UV/IR retrievals [Worden et al., 2007].
  • Are OMI/TES data consistent?
  • How well does GEOS-Chem simulation compare with OMI/TES ozone?

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  • OMI/TES: both on EOS-AURA and measure tropospheric ozone
    • OMI: ~10-12 km FWHM in the troposphere, 13×24 km2, global coverage
    • TES: ~6 km FWHM in the troposphere, 5×8 km2

Worden et al., 2007

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TES Retrievals and GEOS-Chem Simulation

  • TES: V 2.0
    • Compares well with ozonesonde observations: generally biased higher by ~10% [Ray et al., 2007].
    • Compares well with DIAL obtained during the INTEX-B: Positive bias of 5-15% and a negative biases of up to 20% in the upper troposphere [Richard et al., 2007].

  • GEOS-Chem simulation: V7-04-09 with GEOS-4
    • Lightning NOx: 6 Tg/yr, rescaled with OTD/LIS climatology
    • Increase Chinese NOx emission by ~70% (2006)

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Preliminary OMI Ozone Profile Retrievals

  • OMI retrievals: O3 at 24 ~2.5 km layers with optimal estimation
    • Fitting window: 270-310 nm (UV-1), 310-330 nm, 368-372 nm (UV-2)
    • O3 climatology (month, lat, Z) [McPeters et al., 2007] as a priori

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(a)

May 8 2006

Overpass US

Partial

Column

Ozone (DU)

(a) Retrieval

(b) A priori

(b)

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Preliminary OMI Ozone Profile Retrievals

  • OMI calibration: wavelength and cross-track dependent errors
    • Derive soft correction (λ, θ, multiplicative) by simulating OMI radiances: McPeters (strat.) and Logan (1999) trop. O3 clima.

Assumption: climatology represents ozone fields on global average

    • Remove remaining systematic stripes

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(a)

May 8, 2006

  1. Original
  2. Soft calib.
  3. Soft calib. +destriping
  4. A Priori
  5. 600 mb

fc < 0.3

(b)

(c)

(d)

(e)

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Comparison Methodology

  • OMI/TES retrievals: different retrieval grid and a priori
    • Relatively coarser vertical resolution (vs. ozonesonde)
    • TES: more tropospheric ozone information (two defined peaks)
    • OMI: more stratospheric ozone information

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Examples of

coincident

clear-sky AKs

(a) TES (67 levels)

(b) OMI (24 layers)

15°N

40°N

60°N

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Comparison Methodology

  • Use GEOS-Chem as an intermediate, also evaluate GEOS-Chem:
    • Interpolate GEOS-Chem/TES to OMI grid (coarsest)
    • Append GEOS-Chem with TES stratospheric ozone
    • Compare GEOS-CEHM with TES (TES AKs + OMI a priori)
    • Compare GEOS-CEHM with OMI (OMI AKs + OMI a priori)
  • Compare OMI/TES directly, similar to Luo et al. [2007]:
    • Interpolate TES to OMI grid and adjust TES with OMI a priori
    • Apply OMI AKs to TES data
  • Compare OMI/TES with ozonesonde observation later (not here)
  • Present the comparison on May 08, 2006 (similar on other days)
    • Remove poor retrievals (i.e., TES master flag, emission layer flag, OMI fitting residuals) and cloudy pixels (OMI fc > 0.3)
    • 550 coincidences

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OMI/TES/GEOS-Chem TCO on May 8, 2006

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Generally consistent spatial distribution despite systematic biases

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OMI/TES/GEOS-Chem TCO on May 8, 2006

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MB = -8%

MB = -6%

MB = -7%

MB = 4%

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OMI/TES/GEOS-Chem Comparison

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  1. Difference due to OMI/TES AKs can be up to 10-15% especially in UT
  2. Large negative (10°N-20°N, high sun) and positive (40°S-25°S, low sun) biases may be caused by non-linearity of the OMI calibration.

(a)

(b)

Mainly systematic OMI/TES differences

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OMI/TES Comparison

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(b) Those biases are not caused by a priori

(a, c, d) Mostly systematic differences

a

b

c

d

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Summary

  • The spatial distribution of OMI, TES, and GEOS-Chem tropospheric ozone is similar on the global scale.
  • TES shows a systematic positive bias of ~10% relative to GEOS-Chem.
  • OMI shows a negative bias of ~15% relative to TES except for 10°N-20°N (~ -30%) and 45°S-25°S (~20%). The large negative bias at high sun and positive bias at low sun may be related to the non-linearity calibration of OMI.
  • OMI/TES differences cannot be explained by a priori and different averaging kernels, and are mainly systematic.

Acknowledgements

    • OMI and TES science team, GEOS-Chem community
    • NASA and Smithsonian Institution

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OMI/TES/GEOS-Chem Ozone (600 mb)�(North Pacific during INTEX-B, May 05-09, 2006)

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05/05

05/06

05/07

05/08

05/09

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OMI TCO (North Pacific on May 05-10, 2006)

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OMI tropospheric column ozone

fc < 0.3

Gridded to 2.5°×2°

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Persistent high O3 over Northern India from OMI, not clear from TES, not shown in GEOS-Chem. Maybe be due to OMI retrieval artifacts: (a) absorbing aerosols (b) incorrect terrain height

OMI/TES/GEOS-Chem Ozone (600 mb) on May 04-12, 06

05/04

05/06

05/08

05/10

05/12

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Append GEOS-Chem with TES stratospheric ozone

How does the Appending of Different Stratospheric Ozone to GEOS-Chem Affect the Comparison?

Append GEOS-Chem with OMI a Priori stratospheric ozone