Abstract:
The 2007 Intergovernmental Panel on Climate Change assessment established
that the effect of clouds on climate contributes the largest uncertainty in predicting the
future climate. Satellite observations provide an opportunity for learning about the
behavior of clouds. This thesis seeks to assess the accuracy of cloud properties
retrieved from multispectral satellite imagery and test the usefulness of satellite data in
verifying conclusions based on aircraft observations that marine stratus appear to be
formed through the nearly adiabatic ascent of moist air. Retrievals of cloud optical
depth, a measure of cloud thickness, using 0.64-μm reflectances and droplet radii
using separately 1.6, 2.1, and 3.7-μm reflectances were obtained with the MODerateresolution
Imaging Spectroradiometer (MODIS). Owing to different amounts of
absorption by liquid water in the near infrared, with the least at 1.6 μm and the most at
3.7 μm, the growth of droplet radius with cloud thickness should result in the largest
droplet radii retrieved using the 3.7-μm reflectances and the smallest using 1.6-μm
reflectances. Droplet radii retrieved using the 2.1-μm reflectances, however, are often
the largest, and those retrieved using 3.7-μm reflectances are often the smallest. In
addition aircraft observations indicate that the relationships between droplet radius, re,
and optical depth, t, d ln r / d lnt e ,should be approximately equal to 0.2 for marine
stratocumulus. While satellite observations in optically thick, overcast regions yielded
d ln re/d ln t consistent with this result, retrievals for regions with broken clouds often
yielded d ln r / d lnt e substantially smaller than 0.2.
Clouds often exhibit large horizontal and vertical variability. In this thesis a
simple radiative transfer model was used to predict reflectances at visible and near
infrared wavelengths for clouds formed through the adiabatic ascent of moist air, and
then a retrieval scheme based on vertically uniform clouds was used to determine if
the departures from the behavior expected for adiabatic clouds might be caused by the
assumption of spatial uniformity used in the retrievals. The simulations indicated that
at all cloud thicknesses the progression of droplet size using 1.6, 2.1, and 3.7-μm
reflectances followed that suggested by the absorptive properties of liquid water. The
simulation also indicated, however, contrary to the observations, that when the clouds
were optically thin, d ln r / d lnt e should be greater than 0.2, the value expected for
the adiabatic ascent of moist air.
The simulation was adapted to account for the effects of horizontal variations
within clouds. Each 1-km pixel was given a subpixel distribution of optical depths
based on a gamma distribution with mean taken from MODIS pixel-scale optical
depths and variance given by Kato et al. (2006), obtained from Large Eddy
Simulations of marine stratocumulus. Each subpixel was allowed to develop
vertically following the adiabatic ascent of moist air. The average of the reflectances
for the subpixels was used to retrieve the cloud properties for the pixels, and these
properties were compared with the average properties of the subpixels. The retrievals
obtained using 1.6-μm reflectances were most strongly affected by the addition of
subpixel variations in optical depth and droplet radius. Mean droplet radius retrieved
in the simulation was largest when using 1.6-μm reflectances, followed by that
retrieved using 2.1 and 3.7-μm reflectances. The simulation of large droplet radii at
the shorter wavelengths indicated that the large droplets observed in MODIS may
result from horizontal variations within the 1-km MODIS pixel. The values of
d ln r / d lnt e calculated for horizontally heterogeneous clouds were close to 0.2, but
showed variations that extend both above and below this value, consistent with the
MODIS observations.
To illustrate the findings based on the simulations, visible optical depth and
droplet radius were retrieved for MODIS 500-m pixels overcast by marine
stratocumulus. The 500-m pixels were used to represent the subpixel variability
within 2-km pixels constructed from the 500-m pixels. Differences between cloud
properties retrieved using average radiances and averages of the subpixel properties
were compared for overcast and broken-cloud regions using both MODIS and the
Partly Cloudy Pixel Retrieval (PCPR) schemes for identifying the overcast 2-km
pixels. In the regions overcast by optically thick marine stratocumulus, both methods
of identifying overcast pixels led to small biases in the retrieved droplet radii and
optical depths. Values of d ln r / d lnt e obtained in the overcast regions using the
PCPR identifications were closer to the value of 0.2 expected for adiabatic clouds than
those obtained using MODIS identifications. Additionally, values of d ln r / d lnt e
calculated using the 500-m overcast pixels yielded better results than those calculated
using the 2-km pixels. In regions containing broken clouds, the PCPR identification
provided a smaller bias than the MODIS identification, however both methods showed
greater biases than those calculated for regions overcast by optically thick marine
stratocumulus. Values of d ln r / d lnt e for the regions containing broken clouds
showed a positive value when using the PCPR scheme to identify overcast pixels, and
a negative value when using the MODIS cloud mask to identify overcast pixels.
Consistent with the results from the overcast regions, the d ln r / d lnt e obtained for
the 500-m overcast pixels were in closer conformity with adiabatic clouds than the
values obtained for the 2-km pixels using both the MODIS and PCPR identifications.