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Tropospheric NO2 from space: retrieval issues and perspectives for the future

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Title: Tropospheric NO2 from space: retrieval issues and perspectives for the future


1
Tropospheric NO2 from space retrieval issues and
perspectives for the future
  • Michel Van Roozendael
  • BIRA-IASB, Brussels, Belgium

2
Overview
  • Retrieval method (basics)
  • Main issues regarding
  • Spectral fitting
  • Stratospheric correction
  • Tropospheric AMFs
  • Cloud correction
  • How to assess the accuracy of our retrievals?
  • Challenges for the future

3
GOME tropospheric NO2 intercomparison

Why such differences?
Van Noije et al., ACP, 2006

Who is right?

4
NO2 remote sensing using DOAS
  • UV-Vis NO2 absorption is
  • Structured
  • Independent of pressure
  • Weakly dependent on T
  • Total atmospheric attenuation is small (ltlt 1)
  • ? Atmospheric transmission follows Beer-Lambert
    law in a simple way

5
The 3 steps to tropospheric NO2 VCDs
  • STEP 1 DOAS ? NO2 SCD

Strat. NO2
NO2
Surface
6
STEP 1 Spectral fitting issues
  • Error on DOAS fit controlled by
  • S/N ratio, limited by shot noise of detector
  • Possible systematic bias due to
  • Temperature dependence of NO2 cross-sections
  • Interferences with unknown or badly known
    absorbers (e.g. absorption from water vapor
    and/or liquid water)
  • Inaccurate correction for Raman scattering by air
    and/or water
  • Instrumental artefacts. DOAS is insensitive to
    spectrally smooth radiometric errors, but very
    sensitive to offset type errors as well as to
    radiance errors displaying high frequency
    structures (e.g. polarisation, undersampling, )
  • Choice of fitting interval ? trade-off between
    S/N and minimisation of bias effects. Differences
    in settings/correction schemes applied by
    different groups may result in significant SCD
    differences.

7
Accuracy of measured radiances what does matter
for DOAS?
  • S/N ratio ? the more photons the best (in
    practice trade-off between spatial/spectral
    resolution and S/N)
  • Instrument/radiometric calibration issues
  • Wavelength calibration
  • Knowledge of instrumental slit function
  • Dark-current correction
  • Straylight correction
  • Polarization correction
  • Diffuser plate response

8
Examples of known instrumental problems affecting
DOAS retrievals
  • GOME diffusor plate spectral features interfering
    with NO2 absorption ? time-dependent bias,
    requiring special treatment

Richter Wagner, 2001
9
STEP 2 Stratospheric correction
  • Different methods can be used to extract the
    tropospheric signal from the total column seen
    from space (e.g. use cloud shielding effect,
    limb-nadir matching, wavelength dependence of
    AMFs, etc)
  • By far, the most popular ones are
  • The reference sector technique and its variants
    (e.g. harmonic analysis) ? use NO2 columns
    measured over unpolluted regions to infer the
    stratospheric part over source regions
  • The model based technique ? use NO2 columns from
    3D-CTM constrained by observations over
    unpolluted regions
  • The assimilation technique ? assimilate NO2 SCD
    in 3D-CTM (variant of model method)

10
STEP 3 get VCDs using tropospheric AMFs
  • Most complex and error prone part of the
    retrieval
  • Tropospheric NO2 AMFs depend on
  • Solar and viewing geometries
  • Surface properties (albedo, ground elevation)
  • Aerosols
  • Cloud properties
  • Shape of tropospheric NO2 profiles

Problem these properties are to a large extent
unknown, or there are known at inappropriate
resolution !
11
Examples of solutions currently in use
12
Cloud correction scheme
  • Clouds shield surface NO2
  • Clouds enhance sensitivity to NO2 located above
    or at cloud altitude
  • Clouds generally treated as lambertian reflectors
    ? effective cloud fraction and scattering cloud
    top height

AMF (1-f).AMFclear f.AMFcloud AMFcloud
requires estimation of the NO2 column underneath
the cloud (ghost column) !
NO2 layer
Surface
13
Impact of clouds on tropospheric AMFs
14
Clouds as a mean to retrieve information on the
NO2 vertical distribution
  • Idea because of their shielding effect and high
    albedo, clouds reduce the sensitivity to surface
    NO2 and increase the sensitivity to
    free-tropospheric NO2
  • Possible applications
  • Quantify NO2 produced by lightning (Boersma et
    al., 2005)
  • Relate altitude of NO2 plumes to the location of
    sources (Beirle et al., 2007)
  • Identify long-range transport events (TEMIS)

15
How to assess the accuracy of our NO2 retrievals?
  • Differences in retrieval strategies result in
    inconsistencies beteween NO2 products derived
    from different groups. Problem even larger when
    different instruments are analysed by different
    groups.
  • Strategies to assess the accuracy of NO2
    retrievals
  • Comprehensive error analysis (cf. Boersma et al.,
    2004)
  • Intercomparison of satellite data sets (cf. van
    Noije et al., 2006)
  • Validation using external correlative data sets

16
Tropospheric NO2 validation a challenge
  • Why is difficult to valide tropospheric NO2 from
    satellites?
  • NO2 emissions are extremely variable in space in
    time ? the NO2 field as sampled by the satellite
    can hardly be matched by correlative
    measurements.
  • Suitable validation data sets are currently
    limited
  • In-situ surface measurements (difficult to
    compare with satellite columns)
  • Remote-sensing network from NDACC (focus on
    stratospheric columns)
  • In-situ aircraft (excellent but expensive -gt lack
    of statistics)
  • MAXDOAS (promising technique under development
    need for network deployment)
  • NO2 Lidar (interesting but expensive -gt lack of
    statistics)

17
Status of tropospheric NO2 sounders
18
Current statusGOME, SCIAMACHY, GOME-2 and OMI
19
Requirements for future NO2 monitoring systems
  • Driving requirements for air quality (Capacity
    study)
  • Spatial resolution 5-20 km
  • Revisit time 0.5 2h
  • Can be met through
  • Option 1 combination of (at least one)
    geostationary satellite and one sun-synchronous
    low earth orbit satellite (LEO)
  • Option 2 constellation of several instruments in
    LEO a minimum of 3 instruments is needed to
    satisfy sampling requirements at mid-latitude

? Trade-off between Options 1 and 2 must be
evaluated (ongoing CAMELOT study)
20
Challenges for the future (1)
  • How to ensure the consistency of the global NO2
    observing system (GEOSS/GMES requirement) when
    the fleet of instruments expands more and more?
  • Evolve towards common retrieval approaches?
  • Rely on both operational (standardised) and
    scientific (state-of-art) retrieval approaches

21
Challenges for the future (2)
  • What to do to improve NO2 retrievals?
  • A) Enhance sensitivity to detect lower levels of
    pollution
  • Using better instruments ? improve S/N ratio
    through better photon collection efficiency
  • Larger throughput (limited by weight and size!)
  • Longer integration time (GEO)
  • Multiply instruments
  • Using improved algorithms
  • Expand fitting range using direct-fitting ? puts
    high requirements on the quality of Level 1 data,
    and on data processing

22
Challenges for the future (3)
  • B) Improve treatment of radiative transport
  • Use synergy with other (co-located) instruments
    to get better information on albedo, aerosols and
    clouds
  • Use more advanced model data or higher resolution
  • Improve cloud retrieval algorithms in synergy
    with those of NO2 (combined cloud-trace gas
    retrievals)
  • C) Get more than the column (vertical profiling)
  • Expand fitting range using direct-fitting and
    optimal estimation ? requirements on Level 1
    quality (cf. sensitivity)
  • Further develop cloud slicing techniques
  • Use dual/multiple view geometry?
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