Abstract
On the afternoon of 18 January 2003, wildfires swept through several outer suburbs of Canberra (Australia) producing, inter alia, a series of large pyro-cumulonimbus cells and at least one tornado. The results of a large-eddy simulation with a parameterized fire are reported here. The simulation, motivated by the Canberra wildfires and severe storms, captures the main characteristics of the observed pyrocumulonimbi, including the formation of a tornado close to where one was observed. In addition, the model develops prominent horizontally oriented vortices on the western side of the fire in the direction of the low-level shear, and a series of horizontally oriented vortices on the upstream side of the convection column. The production of water by the fire is critical for the development of a pyro-cumulonimbus cell intense enough to reach the tropopause as observed and plays a significant role in the associated tornadogenesis. Copyright 2009 by the American Geophysical Union.
| Original language | English |
|---|---|
| Pages (from-to) | 1-5 |
| Number of pages | 6 |
| Journal | Geophysical Research Letters |
| Volume | 36 |
| Issue number | 12 |
| DOIs | |
| Publication status | Published - 2009 |
Keywords
- Australia
- Canberra
- Convective storms
- Main characteristics
- Numerical simulation
- Parameterized
- Severe storms
- Tornadogenesis
- Western side
- Cell membranes
- Clouds
- Computer simulation languages
- Large eddy simulation
- Storms
- Tornadoes
- Fires
- atmospheric convection
- atmospheric modeling
- cumulonimbus
- large eddy simulation
- numerical model
- tornado
- tropopause
- wildfire
- Australasia
- Australian Capital Territory
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