WW2010
University of Illinois

WW2010
 
welcome
 
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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

Severe Storms
 
introduction
 
dangers of t-storms
 
types of t-storms
 
tstorm components
 
tornadoes
 
modeling

Modeling
 
introduction
 
supercells
 
convective lines
 
forecasting

Convective Lines
 
convective lines
 
squall lines
 
tornadoes

User Interface
 
graphics
text

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Squall Lines

Squall lines generally form along or ahead of cold fronts and drylines and can produce severe weather in the form of heavy rainfall, strong winds, large hail, and frequent lightning.

Squall lines can extend to hundreds of miles in length, simultaneously affecting several states at a time. They also can travel quickly -- at speeds up to 60 mph. [Image: (38K)]
Photo by Doswell

Squall lines typically form in unstable atmospheric environments in which low-level air can rise unaided after being initially lifted (e.g., by a front) to the point where condensation of water vapor occurs. Heat is released during condensation, resulting in the rising air becoming lighter than nearby air at the same height. This leads to an increase in the speed of the rising air which sometimes reaches speeds above 30 mph. In models this initial lifting is specified through an idealization of the flow associated with the front or other lifting mechanism or through the use of observational flow information.

In this simulation, the clouds are shown in grey, and the surface color represents surface winds as seen by an observer moving with the line. Blue represents winds approaching the storm while greens and reds represent the winds in the cold air behind the storm outflow. [Embedded Object: Animation (1.53MB)]


Video by Jewett

The gust front is located along the line where these winds meet -- which extends from the surface well up into the the storm.


The schematic above is a depiction of the structure of a well-formed squall line. Such schematics are often a key result of a scientific investigation and can be based on observations, model and/or theory. They help communicate some of the key features in a simple and concise way. Note the similarity of the schematic to features in previous animation including the overshooting top, anvil, and gust front.



convective lines
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.

tornadoes