TY - JOUR
T1 - Contributions of moist convection and internal gravity waves to building the atmospheric -5/3 kinetic energy spectra
AU - Qiang Sun, Y.
AU - Rotunno, Richard
AU - Zhang, Fuqing
N1 - Funding Information:
The authors thank Chris Snyder and Tiffany Shaw for thoughtful comments on the manuscript. Discussions with Dale Durran, Kerry Emanuel, Raf Ferrari, Joern Callies, and many other researchers on the subject were beneficial. Part of the research was conducted during the first author's summer visit to NCAR/MMM sponsored by the NCAR/Advanced Study Program Graduate Visitor Program. This research is partially supported by the National Science Foundation under AGS Grants 1114849 and 1305798. Computing was performed at the Texas Advanced Computing Center.
Publisher Copyright:
© 2017 American Meteorological Society.
PY - 2017
Y1 - 2017
N2 - With high-resolution mesoscale model simulations, the authors have confirmed a recent study demonstrating that convective systems, triggered in a horizontally homogeneous environment, are able to generate a background mesoscale kinetic energy spectrum with a slope close to -5/3, which is the observed value for the kinetic energy spectrum at mesoscales. This shallow slope can be identified at almost all height levels from the lower troposphere to the lower stratosphere in the simulations, implying a strong connection between different vertical levels. The present study also computes the spectral kinetic energy budget for these simulations to further analyze the processes associated with the creation of the spectrum. The buoyancy production generated by moist convection, while mainly injecting energy in the upper troposphere at small scales, could also contribute at larger scales, possibly as a result of the organization of convective cells into mesoscale convective systems. This latter injected energy is then transported by energy fluxes (due to gravity waves and/or convection) both upward and downward. Nonlinear interactions, associated with the velocity advection term, finally help build the approximate -5/3 slope through upscale and/or downscale propagation at all levels.
AB - With high-resolution mesoscale model simulations, the authors have confirmed a recent study demonstrating that convective systems, triggered in a horizontally homogeneous environment, are able to generate a background mesoscale kinetic energy spectrum with a slope close to -5/3, which is the observed value for the kinetic energy spectrum at mesoscales. This shallow slope can be identified at almost all height levels from the lower troposphere to the lower stratosphere in the simulations, implying a strong connection between different vertical levels. The present study also computes the spectral kinetic energy budget for these simulations to further analyze the processes associated with the creation of the spectrum. The buoyancy production generated by moist convection, while mainly injecting energy in the upper troposphere at small scales, could also contribute at larger scales, possibly as a result of the organization of convective cells into mesoscale convective systems. This latter injected energy is then transported by energy fluxes (due to gravity waves and/or convection) both upward and downward. Nonlinear interactions, associated with the velocity advection term, finally help build the approximate -5/3 slope through upscale and/or downscale propagation at all levels.
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U2 - 10.1175/JAS-D-16-0097.1
DO - 10.1175/JAS-D-16-0097.1
M3 - Article
AN - SCOPUS:85009381930
SN - 0022-4928
VL - 74
SP - 185
EP - 201
JO - Journal of the Atmospheric Sciences
JF - Journal of the Atmospheric Sciences
IS - 1
ER -