WW2010
University of Illinois

WW2010
 
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Meteorology
 
  introduction
 
  air masses, fronts
 
  clouds, precipitation
 
  el nino
 
  forces, winds
 
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> severe storms
 
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Severe Storms
 
  introduction
 
  dangers of t-storms
 
  types of t-storms
 
> tstorm components
 
  tornadoes
 
  modeling

Tstorm Components
 
  introduction
 
  updrafts/downdrafts
 
  wind shear
 
> outflow phenomena
 
  wall clouds

Outflow Phenomena
 
> introduction
 
  gust fronts
 
  microbursts
 
  scud clouds, virga
 
  rain foot, dust foot

User Interface
 
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Outflow Phenomena
downbursts

This section is on visual identification of macrobursts, microbursts, gust fronts and other outflow phenomena. Damaging thunderstorm winds have been termed downbursts by renowned severe storm researcher Dr. Ted Fujita. Dr. Fujita further classifies these events as macrobursts (greater than 2.5 miles in diameter) and microbursts (less than 2.5 miles in diameter).

[Image: downburst photograph (57K)]

The problems that aircraft have had with thunderstorm-induced wind shear, particularly microbursts, indicate that the spotting and reporting of microbursts is of paramount importance. Although some spotters will think that events such as microbursts and flash floods are less dramatic than tornadoes, in reality, they are just as lethal, if not more so, in some circumstances. Hopefully, pilots will find these slides beneficial in identifying outflow structures that could result in dangerous approach or take-off conditions, and delay their subsequent actions until danger has passed.

[Image: shelf cloud accopanying a macroburst (60K)]
Photograph by: Moller

A downburst is a strong downdraft which includes an outburst of potentially damaging winds on or near the ground and if the diameter of the downburst is greater than 2.5 miles, then it is called a macroburst. As a macroburst or a non-severe gust front passes overhead, the ragged, concave-shaped underside of the shelf cloud accompanies the onset of cold outflow winds at the ground. Although some rotation may be visible in these clouds, it is likely to be short-lived and without vertical continuity, precluding a major tornado. Another clue for spotters as to the potential of any observed rotation would be the lack of warm and moist surface-based inflow to the feature.

[Image: cloud hole behind of gust front (42K)]
Photograph by: Moller
Occasionally a cloud hole will appear behind, or in some cases immediately ahead of a gust front. The cause is frequently a small scale downdraft, possibly a microburst, which is resulting in rapid cloud dissipation.

There is little doubt about a small downdraft being the culprit in this particular case, as evidenced by the amount of blowing dust that has been kicked up beneath the cloud hole.



Wind Shear
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.

gust fronts