The impacts of gravity wave (GW) on the thermal and dynamic characteristics within the mesosphere/lower thermosphere, especially on the atmospheric instabilities, are still not fully understood. In this paper, we conduct a comprehensive and detailed investigation on one GW breaking event during a collaborative campaign between the Utah State University Na lidar and the Advanced Mesospheric Temperature Mapper (AMTM) on 9 September 2012. The AMTM provides direct evidence of the GW breaking as well as the horizontal parameters of the GWs involved, while the Na lidar's full diurnal cycle observations are utilized to uncover the roles of tide and GWs in generating a dynamical instability layer. By studying the changes of the OH layer peak altitude, we located the wave breaking altitude as well as the significance of a 2 h wave that are essential to this instability formation. By reconstructing the mean fields, tidal and GW variations during the wave breaking event, we find that the large-amplitude GWs significantly changed the Brunt-Vaisala frequency square and the horizontal wind shear when superimposed on the tidal wind, producing a transient dynamic unstable region between 84 km and 87 km around 11:00 UT that caused a subsequent small-scale GW breaking.
IntroductionThe gravity wave (GW) forcing and its related spectra within the mesosphere/lower thermosphere (MLT) are the key parameters for the understanding of energy and momentum transfers between the lower and middle atmosphere and the ionosphere. They have been known to drive the circulation and generate the counter intuitive cold summer and warm winter in the mesopause region [Garcia and Solomon, 1985], along with some irregularities in the ionosphere [Liu and Vadas, 2013]. Yet after decades of investigations, their characteristics and effects on the upper atmosphere are still not fully understood due to the GW's random spatial scales with their periods varying from a few minutes to several hours. Mainly generated in the troposphere by orographic, convection, and jet-front system, the GWs propagate upward with growing amplitude to compensate for the decrease of the air density due to conservation of the wave energy density during their propagation, before they reach the critical levels or become unstable and break . It is also possible that the GW breaking can generate secondary waves within the breaking region [Vadas et al., 2003;Smith et al., 2013], affecting the atmosphere above MLT region. The wave breaking process deposits momentum into the mean flow field, causing mean flow acceleration in the wave propagation direction; changes the thermal structure; and generates turbulence around the breaking region.Ground-based experimental studies have been playing the significant role in studying the GW dynamics and the associated atmospheric instabilities during the recent decades. However, single instrument only partially resolves the complex wave breaking process and the instability phenomenon. For example, the airglow measurement techniques like OH ima...