This paper demonstrates that it is possible to use measurements of the Dopp
ler spectrum width front a high-resolution radar to obtain quantitative est
imates of dissipation rate during the passage of precipitating frontal zone
s. Using the high-resolution Chilbolton radar, this method has been applied
, for the first time, to infer the rate at which kinetic energy is dissipat
ed by turbulence within mid- and lower-tropospheric frontal zones. Analysis
of detailed measurements for one cold-frontal region showed multiple shall
ow sheets of high dissipation rate, with spatially averaged values around I
x 10(-3) m(2)s(-3). Comparable values were also observed in a warm-frontal
zone. The magnitude of the observed dissipation rate supports the hypothes
is that mixing played a major role in determining the mean properties of th
e fronts. in that the turbulence acted to destroy the frontal shear layer o
n a time-scale of several hours. These issues have particular relevance to
the representation of fronts within future very high-resolution numerical w
eather-prediction models.