Squall line experiments: moderate-shear results
Run n95E: 300-km
along-front domain -
Mpeg /
QT movie
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Higher-RH case |
Some low-shear images |
Run history
A series of simulations were carried out in which a two-dimensional front
(modeled previously)
is used to initiate convection in a 3D cloud model.
Given the lineal form of the forcing, a squall line develops. Simulations were
performed with:
- Frontal forcing, random perturbations (only) - most realistic
- Frontal forcing, random + 5 thermals - isolate cell-cell interaction
- No frontal forcing, random + 5 thermals - isolate role of the front
The results shown here represent simulations currently being made.
As such, the content of this page will be changing frequently.
Random/frontal results
(vertical scale magnification factor: 3)
| Looking nw | Looking nnw |
 |
 |
Explanation of images |
movie (mpeg, 3 MB) |
movie (QuickTime, 12 MB)
The low-shear results were presented at the Mesoscale Processes
conference (Reading, England, Sept. 9-13).
From results available to date, the higher shear environments
produce longer-lived and more distinct cells, as expected. The storms
are supercellular in that they maintain low level rotation even as
continuous updraft growth occurs on the south side of each cell.
3D simulations in a more moist environment
The above results were taken from a specific time in the evolution
of the 2D simulation. 3D results from a later (2D run) time (though still
prior to convective initiation) are shown below. These simulations
are still underway.
Cloud+rain movie available (1.9 MB).
Comparison - lower shear simulation
Most of the lower-shear simulation data may be
found here.
A few images and a movie (also with vertical exaggeration=3) are here
for comparison.
Cloud+rain movie available (1.5 MB).
Experimental design
- Slab-symmetric
frontal simulations
- nested: horiz. resolutions 16, 5.3, 1.8 km
- used to simulate cold front at high resolution
- repeated until desired (1D) along-front conditions
reproduced by model
- final state represents more complete initial
state for the convection.
- 3D simulations
- 2D frontal simulation (see above) expanded in N-S direction
- Random perturbations introduced to allow 3D structures
to develop
- Experiments made with and without the presence of the front
to isolate the role of the front on the convection.
Simulation details
Go to:
Observations |
Low-shear simulations |
Moderate-shear simulations |
Top simulation page
Further information regarding this work may be found (for now) in the
conference preprint for the 1996 Severe Local Storms conference
(San Francisco) and the corresponding
preprint for the 1996 Mesoscale Processes conference (Reading).
Credit
Thanks go to Crystal Shaw of the Atmospheric Sciences Dept. & NCSA for
her assistance with Iris Explorer and with cleaning up the figures. Thanks
also to David Wojtowicz of Atmospheric Sciences for Explorer help and
for use of and help with his trajectory package.
Brian F. Jewett
| bjewett@ncsa.uiuc.edu
| homepage