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Supercell storms: In-class demo and Experiment 3
ATM 419/563 Spring 2017 Fovell
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Goals Start idealized WRF 3D run to simulate a splitting supercell thunderstorm (in-class demo) Review supercell storm structure and behavior (while model runs) Analyze demo simulation Investigate sensitivity to microphysics Employ GrADS ensemble dimension, and compute ensemble mean and standard deviation Submit WRF jobs to the Snow batch system
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In-class portion
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Setup Create a folder called SUPERCELL in your lab space
Copy /network/rit/lab/atm419lab/SUPERCELL/SETUP.tar there and unpack Files included: make_all_links.csh, namelist.input, input_sounding, read_wrfinput.py, submit_wrf, control_file.z Pre-configured for a 2-h run in a 168km by 168km domain at 2km horizontal resolution Initial sounding derived from Weisman and Klemp (1982) “quarter-circle” wind profile favors storm splitting and right-mover Purdue Lin microphysics (mp_physics = 2) Time step 12 seconds History output every 10 min Computes some AFWA diagnostic fields (&afwa section) read_wrfinput.py WK sounding was slightly modified from original
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Boundary layer mixing ratio is 14 g/kg in input_sounding Weisman and Klemp (1982)
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Hodograph (see input_sounding)
2 km AGL 7 km AGL surface
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Using the Snow batch system
Look at the file submit_wrf: #!/bin/bash # Job name: #SBATCH --job-name=ATM419 #SBATCH -n 6 #SBATCH -N 1 #SBATCH --mem-per-cpu=7G #SBATCH -p snow #SBATCH -o sbatch.out #SBATCH -e sbatch.err.out […] echo "running WRF" srun -N 1 -n 6 -o wrf.srun.out ./wrf.exe Change to your name Requests 6 cpus on 1 node Where run time errors might be reported This runs the model. The –N and –n values must match those provided at the top
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Initialize model Allocate resources
csh make_all_links.csh srun ideal.exe This MPI version does not write to screen anymore To see if the job worked: type trsl, which stands for “tail –f rsl.out.0000”. Type CTRL-C to break free. What is the lowest scalar model level height? python read_wrfinput.py wrfinput_d01 Submit your batch job: $ sbatch –p snow submit_wrf Check on your job $ squeue –u yournetid Lowest scalar height: 285 m. Not uncommon for cloud model simulations. Not even trying to capture PBL properly.
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As the model runs… The model writes output to four kinds of files (in addition to wrfout…) rsl.out.XXXX (numbered 0000 to 1-n, n =number of nodes requested) rsl.error.XXXX (numered as above) sbatch.out (timing info when job completed) sbatch.err.out (hopefully it is empty!) As the model runs, you can “watch” it with $ trsl [This is an alias for tail -f rsl.out.0000] [type ‘CTRL-c’ to quit/escape from this] Look for SUCCESS COMPLETE WRF as usual
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Supercell structure and behavior
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Supercells Characterized by rotating updrafts (vertical velocity and vertical vorticity co-located) Mesocyclone and “hook echo” Develop in environments with large vertical wind shear Evolve from ordinary cells by “splitting” into “left-movers” and “right-movers” Clockwise directional vertical wind shear favors right-movers
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Split L mover weaker R mover turns right R mover hook Purple = hail
24apr2006_split_dfx_n0r01.GIF Split L mover weaker R mover turns right R mover hook Purple = hail
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Splitting storms Wilhelmson and Klemp (1981)
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Shear-induced horizontal vorticity
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Dynamics of storm splitting
• Lifting of vortex tubes by updraft creates counter-rotating vortices (vertical vorticity) • Low perturbation pressure develops that establishes new updrafts on flanks of original storm • New cells are rotational: CCW or CW • Old cell dies, giving appearance of split • Actually, precipitation does NOT cause the updraft split
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Original updraft
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Counter-rotating vortices
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New storms form on flanks
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Old cell decays
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reflectivity > 65+ dBZ (hail or airborne debris) hook echo
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radial velocity
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Supercell conceptual model
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Storm-scale fronts T = tornado location
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mesocyclone meso = Gk., middle
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Updraft velocities can easily
exceed 100 mph
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RFD = rear flank downdraft
FFD = forward flank downdraft
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warm, moist air lifted into updraft
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Supercell storm structure
Plan view at surface UD = updraft FFD = forward flank downdraft RFD = rear flank downdraft Gust front Hook echo Dot ~ tornado location Lemon and Doswell (1979)
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{Do Supercell in-class demo here}
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Experiment 3
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EXP03 overview Make 5 different simulations with 5 different microphysics schemes Do not select schemes 1, 3, 4, 5, 11, 12 or 14, as they do not produce radar reflectivity fields and/or have graupel as a species Do not select scheme 2, as we did that in class Do not choose bin schemes 30 or 32 Use the default time step of 12 sec srun ideal.exe as usual. Check tail of rsl.out.0000 file. WRF simulations have to be submitted to the Snow batch queue, using the submit_wrf script Given our setup, you can only run one job at a time Unpack the 5 simulations using control_file.z, using a naming convention like mpXX, where XX = mp_physics Note that some schemes create QHAIL but control_file.z will ignore this field. The ensemble members need identical CTL files
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EXP03 tasks You have created a small WRF microphysics ensemble
Write a GrADS CTL file for the ensemble Use the SQUALL demo’s mp_ensemble.ctl for guidance Run GrADS and open your ensemble CTL file Write a GrADS script to compute the mean and standard deviation of w_up_max at the final time (2 hours) Std deviation shaded and mean field contoured and superimposed. Use squall_ensemble.gs for guidance. Make a plot, and label axes Send to me: A list of which microphysics schemes you selected A PNG plot (or screenshot) of your w_up_max field Your GrADS script Your ensemble CTL file One additional plot, properly labeled, of anything you want. (Make sure I know what I am looking at.)
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