F. Fabry et T. Zawadzki, LONG-TERM RADAR OBSERVATIONS OF THE MELTING LAYER OF PRECIPITATION AND THEIR INTERPRETATION, Journal of the atmospheric sciences, 52(7), 1995, pp. 838-851
In this study, 600 h of vertically pointing X-band radar data and 50 h
of UHF boundary layer wind profiler data were processed and analyzed
to characterize quantitatively the structure and the causes of the rad
ar signature from melting precipitation. Five classes of vertical prof
iles of reflectivity in rain were identified, with three of them havin
g precipitation undergoing a transition between the solid and liquid p
hase. Only one of them, albeit the most common, showed a radar brightb
and signature. In-depth study of the bright band and its dependence on
precipitation intensity reveals that the ratio of the brightband peak
reflectivity to the rainfall reflectivity is constant at 8 dB below 0
.5 mm h(-1) and then increases to reach 13 dB at 2.5 mm h(-1) and 16 d
B at 5 mm h(-1). The equivalent reflectivity factor of snow just above
the melting layer is on average 1-2 dB below the reflectivity of rain
just below the melting layer, independent of precipitation intensity.
The classical brightband explanation accounts for less than half of t
he observed reflectivity enhancement; the difference could be explaine
d by effects associated with the shape and density of melting snowflak
es and, to a smaller extent, by precipitation growth in the melting la
yer and aggregation in the early stages of the melting followed by bre
akup in the final stages. The brightband statistics were also signific
antly different for reflectivities in rain above 25 dBZ when observati
ons were made with an X-band radar as opposed to the wind profiler bec
ause of the combination of attenuation in the melting layer and the fa
ct that scattering from some of the large hydrometeors above and withi
n the melting layer depart from the Rayleigh approximation usually use
d to compute reflectivity. The bright band is often capped by a thin a
nd faint dark layer, which tends to be more evident at weak precipitat
ion intensities.