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Initial 3D isotropic fractal field

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Title: Initial 3D isotropic fractal field


1
A 3D stochastic cloud model for investigating the
impact of cirrus inhomogeneity on radiative
transfer Robin J. Hogan and Sarah F.
Kew Department of Meteorology, University of
Reading, UK Email r.j.hogan_at_reading.ac.uk
3. Formulation of stochastic cloud model
  • A 1D power spectrum indicates variance at each
    scale but with no phase information.
  • An initial fractal cloud-like field can be
    generated by essentially performing an inverse 3D
    Fourier Transform on the 1D power spectrum, but
    introducing random phases for the Fourier
    components.
  • In practice this is more complicated as we need
    to add artificial scale breaks in the 1D spectrum
    to account for different grid spacing and domain
    sizes in the x, y and z directions.

Initial 3D isotropic fractal field
1. Introduction
  • The importance of ice clouds on the earths
    radiation budget is well recognized.
  • Ice cloud inhomogeneity can affect both mean
    longwave (Pomroy and Illingworth 2000) and
    shortwave fluxes (Carlin et al. 2002).
  • Most GCMs assume cloud is horizontally uniform,
    but non-uniform clouds have lower emissivity and
    albedo for same mean optical depth due to
    curvature in the relationships.

Simulated cirrus cloud (isosurface of IWC)
  • At each height we then
  • Translate to simulate fallstreaks.
  • Change the spectral slope to simulate mixing.
  • Scale to get the right mean and variance.
  • Exponentiate to produce a lognormal distribution.
  • Threshold at a certain IWC value to represent
    gaps in the cloud.
  • High resolution observations are required to
    characterize the horizontal inhomogeneity of
    cloud water content and radiative properties.
  • However, vertical decorrelation information is
    also required and this can only be derived from
    radar aircraft data are insufficient.
  • Cross-sections through the simulated field look
    encouragingly similar to the IWC field from the
    original radar image
  • Stochastic models are useful for quantifying the
    radiative effect of cloud structure but existing
    models have tended to concentrate on
    boundary-layer clouds (e.g. Cahalan et al. 1994,
    DiGuiseppe and Tompkins 2003, Evans and Wiscombe
    2004).
  • Here we present the first stochastic model
    capable of representing the important structural
    features unique to cirrus fallstreak geometry
    and shear induced mixing.
  • Preliminary radiative transfer calculations
    demonstrate the sensitivity of fluxes to
    fallstreak orientation, which is determined by
    wind shear.

4. Radiative properties of inhomogeneous cirrus
  • A thinner cloud, modelled on a case from 17 July
    1999, is now used to demonstrate the effect of
    wind shear on radiative fluxes

Stratocumulus simulation for comparison
Observed shear 2 m s-1 km-1
Higher shear 20 m s-1 km-1
Slice through simulation
2. Analysis of cloud radar data
Emissivity
  • We use the 94-GHz radar at Chilbolton, England.
    The case shown is from 27 Dec 1999 and
    demonstrates the effect of wind shear on
    fallstreak geometry.

Emissivity
Reflectance
Met Office model
Reflectance
  • Numerous published empirical relationships exist
    to estimate ice water content (IWC) from radar
    reflectivity factor, and we find that the
    resulting PDFs may usually be represented by a
    lognormal distribution (Hogan and Illingworth
    2003)

Reflectance
  • The changes to mean emissivity and albedo with
    shear correspond to changes in longwave and
    shortwave flux of 20-30 W m-2, of the same order
    as the error incurred in climate models due to
    not representing cirrus inhomogeneity at all.
  • By contrast, stratocumulus structure has little
    effect in the longwave as the higher optical
    depth means that the cloud behaves as a black
    body also the temperature contrast with the
    ground is much less.

MODIS reflectance
  • Spectral analysis of ln(IWC) reveals a spectral
    slope of close to 5/3 at cloud top which
    steepens lower down in the cloud due to
    preferential mixing at smaller scales.

5. Implications for spaceborne radar and lidar
  • We can use the stochastic model to simulate
    synergistic radar/lidar retrievals.
  • It is found that footprints within 1.5 km of each
    other (from an altitude of 700 km) are needed for
    the error due to mismatch to be less than 25 (1
    dB).

Spread of fall speeds (due to turbulence or size
distribution) leads to homogenisation of
fallstreaks and steeper power spectrum
CloudSat radar and Calipso lidar to be launched
in 2005
  • At each height we characterize the cloud by these
    parameters
  • Mean IWC
  • Fractional variance of IWC, fIWC (tends to be
    higher near cloud boundaries)
  • Power spectrum slope
  • Scale break (usually found to be around 50 km)
  • Horizontal wind speed (to estimate horizontal
    displacement)
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