The purpose of this investigation is to examine the basic properties of convectively-generated gravity waves. Particular attention is paid to the evolution of the wave spectrum from initiation to propagation through the tropopause. Several case studies of deep convection over the United Kingdom are analyzed using both observation and high resolution numerical model simulation. Observations of high frequency waves are provided by a Mesosphere-Stratosphere-Troposphere (MST) wind profiling radar located at Aberystwyth in Wales. Numerical simulation is performed with the (UK) Met Office Unified Model (UM) on a limited area grid with horizontal grid spacing as high as 1 km at which resolution the convective parameterization is disengaged and the wave source is primarily explicit.
Using wavelets, the wave spectrum is demonstrated to be comprised of several distinct peaks that appear in both the MST observations and UM simulations. The spectral peaks exist within a range of horizontal wavelengths from approximately 5 km to 50 km with periods less than 30 min. The origin of these multiple peaks is presently under investigation. Possible causes include a resonant triad interaction or a wave-source interaction. The latter mechanism is examined in idealized model experiments in which a wave generation mechanism is externally imposed (e.g., an injection of vertical velocity of finite duration) against a background environment that allows for wave reflection and refraction near the wave source.