Abstract
The atmospheric mesoscales are characterized by a complex variety of meteorological phenomena that defy simple classification. Here a full space-time spectral analysis is carried out, based on a 7 day convection-permitting simulation of springtime midlatitude weather on a large domain. The kinetic energy is largest at synoptic scales, and on the mesoscale it is largely confined to an “advective band” where space and time scales are related by a constant of proportionality which corresponds to a velocity scale of about 10 m s−1. Computing the relative magnitude of different terms in the governing equations allows the identification of five dynamical regimes. These are tentatively identified as quasi-geostrophic flow, propagating gravity waves, stationary gravity waves related to orography, acoustic modes, and a weak temperature gradient regime, where vertical motions are forced by diabatic heating.
Author supplied keywords
Cite
CITATION STYLE
Craig, G. C., & Selz, T. (2018). Mesoscale Dynamical Regimes in the Midlatitudes. Geophysical Research Letters, 45(1), 410–417. https://doi.org/10.1002/2017GL076174
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.