Radar observations of updrafts, downdrafts, and turbulence in fair-weathercumuli

Citation
P. Kollias et al., Radar observations of updrafts, downdrafts, and turbulence in fair-weathercumuli, J ATMOS SCI, 58(13), 2001, pp. 1750-1766
Citations number
47
Categorie Soggetti
Earth Sciences
Journal title
JOURNAL OF THE ATMOSPHERIC SCIENCES
ISSN journal
00224928 → ACNP
Volume
58
Issue
13
Year of publication
2001
Pages
1750 - 1766
Database
ISI
SICI code
0022-4928(2001)58:13<1750:ROOUDA>2.0.ZU;2-Y
Abstract
Observations from a 94-GHz radar are used to define the vertical structure of marine fair-weather cumuli. Doppler spectra obtained from the radar prov ide mean vertical velocities as well as detailed spectral shapes that can b e used to infer small-scale vertical velocity shear, illuminate cloud micro physical processes, and provide estimates of turbulence dissipation rates. These new observations facilitate the analysis and understanding of in-clou d circulations and the physical processes involved, since the cloud boundar ies and dimensions are mapped along with the internal structure of the clou ds. Coincident observations from a 915-MHz radar (wind profiler) were used to further define the turbulence structure in and around the clouds. The ob servations document the detailed vertical and horizontal dimensions of updr aft and downdraft circulations in the clouds observed. The two cumuli studi ed in detail have similar circulation patterns-an updraft core surrounded b y downdrafts. Although the clouds have a horizontal depth of only about 700 m, updraft velocities of about 5.5 m s(-1) were observed. These updrafts, which are only about 400 m across, exhibit characteristics that are consist ent with adiabatic ascent, and penetrate about 150 m into the capping inver sion. No penetrating downdrafts are observed within the updraft cores. The downdrafts that flank the updraft on the downwind side of the cloud are rel atively narrow (less than 100 m) and extend from cloud top to cloud base. T he downdraft on the upwind side of the cloud is about 150 m across and pene trates about 200 m into the detraining cloud mass observed in this part of the cloud. This downdraft appears to be driven by the cooling associated wi th entrainment mixing at cloud top penetrating through detraining, dynamica lly inactive parts of the cloud matter. Analysis of the Doppler spectrum at the updraft-downdraft interfaces indicates large Doppler spectral widths d ue to turbulence and sharp shear zones in the radar sampling volume. Large Doppler spectral widths in the detraining upwind part of the cloud are cons istent with the presence of larger droplets. The updraft core structure in one of the clouds has a structure that is consistent with the idea that cum ulus clouds are composed of successive bubbles that emerge from the subclou d layer. Thus these small cumuli should be considered as convective complex es rather than simple growing elements that later decay into passive clouds . This study illustrates the potential of millimeter-wavelength radars for studying small cumuli.