Jl. Caccia et Jp. Cammas, VHF-ST RADAR OBSERVATIONS OF AN UPPER-LEVEL FRONT USING VERTICAL AND OBLIQUE-BEAM C-N(2) MEASUREMENTS, Monthly weather review, 126(2), 1998, pp. 483-501
Mesoscale aspects of an upper-level front that moved over Brittany (Fr
ance) during the Mesoscale Frontal Dynamical Project 1987 experiment a
re investigated using very high frequency stratospheric-tropospheric (
VHF ST) radar data and European Centre for Medium-Range Weather Foreca
sts (ECMWF) analyses. The synoptic study shows that the upper-level fr
ont moved without significant change over the radar during the observa
tion period, from 0000 UTC 14 November 1987 to 0000 UTC 15 November 19
87. This allows radar data height-time cross sections to be interprete
d as representing the corresponding spatial data distributions. A rada
r technique of stable airmass detection using the measurement of the a
spect ratio, that is, the vertical to oblique power ratio, and the tur
bulence, that is, the structure constant of the refractive index fluct
uations C-N(2), is developed. This method is applied to the case study
of the upper-level frontal passage, which allows the associated stabl
e air masses above the radar site to be monitored when going from 9 km
down to the lower troposphere in the 2-4-km altitude range. Mesoscale
dynamical aspects of the upper-level frontal zone are described using
time series of radar-derived vertical wind shear. The 0.3 degrees slo
pe of the upper-level front, evaluated from the radar data and a 20 m
s(-1) eastward propagation velocity of the large-scale baroclinic syst
em, agrees well with the one derived from radiosounding data of the ne
arest synoptic stations. Along this slope, an enhancement of the turbu
lence and a maximum vertical wind shear of 20 m s(-1) km(-1) were foun
d. At a larger scale (timescale of 6 h), the reliability of the VHF-ST
radar measurements of the air vertical velocity in the vicinity of th
e frontal zone is supported by both a favorable cross comparison with
the vertical velocity calculated from the ECMWF analyses and downward
motions roughly deduced from the winds on the isentropic surfaces.