WW2010
University of Illinois

WW2010
 
welcome
 
online guides
 
archives
 
educational cd-rom
 
current weather
 
about ww2010
 
index

Online Guides
 
introduction
 
meteorology
 
remote sensing
 
reading maps
 
projects, activities

Meteorology
 
introduction
 
air masses, fronts
 
clouds, precipitation
 
el nino
 
forces, winds
 
hurricanes
 
hydrologic cycle
 
light, optics
 
midlatitude cyclones
 
severe storms
 
weather forecasting

Clouds, Precipitation
 
introduction
 
mechanisms
 
precip processes
 
high level clouds
 
mid level clouds
 
low level clouds
 
vertically developed
 
other cloud types

Other Cloud Types
 
contrails
 
billow clouds
 
mammatus
 
orographic
 
pileus

User Interface
 
graphics
text

.
Billow Clouds
rotating eddies

Billow clouds are created from instability associated with flows having marked vertical shear and weak thermal stratification. The common name for this instability is Kelvin-Helmholtz instability. One may visualize these instabilities as a row of horizontal eddies aligned within this layer of vertical shear.

[Image: example of kelvin helmholtz waves (61K)]


Billow clouds are created in the upward branch of each of the eddies if the air within this branch has a high enough relative humidity that, upon lifting, the air parcel reaches saturation. Individual billow clouds generally have life times of a few minutes. The presence of billow clouds provides a visible signal to aviation interests of potentially dangerous turbulence.


Terms for using data resources. CD-ROM available.
Credits and Acknowledgments for WW2010.
Department of Atmospheric Sciences (DAS) at
the University of Illinois at Urbana-Champaign.