R. Meneghini et al., MICROPHYSICAL RETRIEVALS OVER STRATIFORM RAIN USING MEASUREMENTS FROMAN AIRBORNE DUAL-WAVELENGTH RADAR-RADIOMETER, IEEE transactions on geoscience and remote sensing, 35(3), 1997, pp. 487-506
The need to understand the complementarity of the radar and radiometer
is important not only to the Tropical Rain Measuring Mission (TRMM) p
rogram but to a growing number of multi-instrumented airborne experime
nt that combine single or dual-frequency radars with multichannel radi
ometers, The method of analysis used in this study begins with the der
ivation of dual-wavelength radar equations for the estimation of a two
-parameter drop size distribution (DSD), Defining a ''storm model'' as
the set of parameters that characterize snow density, cloud water, wa
ter vapor, and features of the melting layer, then to each storm model
there will usually correspond a set of range-profiled drop size distr
ibutions that are approximate solutions of the radar equations, To tes
t these solutions, a radiative transfer model is used to compute the b
rightness temperatures for the radiometric frequencies of interest, A
storm model or class of storm models is considered optimum if it provi
des the best reproduction of the radar and radiometer measurements, Te
sts of the method are made for stratiform rain using simulated storm m
odels as well as measured airborne data, Preliminary results show that
the best correspondence between the measured and estimated radar prof
iles usually can be obtained by using a moderate snow density (0.1-0.2
g/cm(-3)), the Maxwell-Garnett mixing formula for partially melted hy
drometeors (water matrix with snow inclusions), and low to moderate va
lues of the integrated cloud liquid water (less than 1 kg/m(-2)), The
storm-model parameters that yield the best reproductions of the measur
ed radar reflectivity factors also provide brightness temperatures at
10 GHz that agree well with the measurements, On the other hand, the c
orrespondence between the measured and modeled values usually worsens
in going to the higher frequency channels at 19 and 34 GHz. In searchi
ng for possible reasons for the discrepancies, it is found that change
s in the DSD parameter mu, the radar constants, or the path-integrated
attenuation can affect the high frequency channels significantly, In
particular, parameters that cause only modest increases in the median
mass diameter of the snow, and which have a minor effect on the radar
returns or the low frequency brightness temperature, can produce a str
ong cooling of the 34 GHz brightness temperature.