Simulation datasets for: Intense surface winds from gravity wave breaking in simulations of a destructive macroburst
Data files
Dec 07, 2022 version files 1.85 GB
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ako.d03.TS
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cph.d03.TS
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input_sounding
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namelist.input
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namelist.input.cm1
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nwyu.d03.TS
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onefile.F
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README.md
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sedg.d03.TS
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swph.d03.TS
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tslist
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wrfinput_d01
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wrfinput_d02
Dec 07, 2022 version files 1.85 GB
-
ako.d03.TS
-
cph.d03.TS
-
input_sounding
-
namelist.input
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namelist.input.cm1
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nwyu.d03.TS
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onefile.F
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README.md
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sedg.d03.TS
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swph.d03.TS
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tslist
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wrfinput_d01
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wrfinput_d02
Abstract
Shortly after 0600 UTC (midnight local time) 9 June 2020, a convective line produced severe winds across parts of northeast Colorado that caused extensive damage, especially in the town of Akron. High-resolution observations showed gusts exceeding 50 m sā1, accompanied by extremely large pressure fluctuations, including a 5-hPa pressure surge in 19 s immediately following the strongest winds and a 15-hPa pressure drop in the following 3 min. Numerical simulations of this event (using the WRF Model) and with horizontally homogeneous initial conditions (using Cloud Model 1) reveal that the severe winds in this event were associated with gravity wave dynamics. In a very stable postfrontal environment, elevated convection initiated and led to a long-lived gravity wave. Strong low-level vertical wind shear supported the amplification and eventual breaking of this wave, resulting in at least two sequential strong downbursts. This wave-breaking mechanism is different from the usual downburst mechanism associated with negative buoyancy resulting from latent cooling. The model output reproduces key features of the high-resolution observations, including similar convective structures, large temperature and pressure fluctuations, and intense near-surface wind speeds. The findings of this study reveal a series of previously unexplored mesoscale and storm-scale processes that can result in destructive winds.
Significance Statement
Downbursts of intense wind can produce significant damage, as was the case on 9 June 2020 in Akron, Colorado. Past research on downbursts has shown that they occur when raindrops, graupel, and hail in thunderstorms evaporate and melt, cooling the air and causing it to sink rapidly. In this research, we used numerical models of the atmosphere, along with high-resolution observations, to show that the Akron downburst was different. Unlike typical lines of thunderstorms, those responsible for the Akron macroburst produced a wave in the atmosphere, which broke, resulting in rapidly sinking air and severe surface winds.
README: Simulation datasets for "Intense surface winds from gravity wave breaking in simulations of a destructive macroburst"
Included here are the files required to configure and reproduce the numerical simulations presented in this manuscript. (Full model output is not included owing to its large size.) The manuscript includes simulations from the Weather Research and Forecasting model, version 4.0.3 (https://www.mmm.ucar.edu/models/wrf) and Cloud Model 1 (https://www2.mmm.ucar.edu/people/bryan/cm1/), version 20.1.
Description of the Data and file structure
For the WRF model, included are the 'namelist.input' configuration file, along with the 'wrfinput' files (netCDF format) for domains 1 and 2 that contain the model initial conditions. Also included are the time series output (plain text) for the locations shown in the manuscript, along with the configuration file 'tslist' for outputting these time series.
For the CM1 model, the 'namelist.input.cm1' configuration file and 'input_sounding' files are included, which can be used to initialize the model. The full fortran source code 'onefile.F' is also included.
Sharing/access Information
Links to other publicly accessible locations of the data: N/A
Was data derived from another source? No
Methods
This dataset includes the information required to reproduce the model simulations presented in the manuscript. This includes the namelist and initial and lateral boundary conditions for the WRF simulation, and the namelist and initial sounding for the CM1 simulation.