next up previous
Next: 5. Applied Aspects Up: Upper atmospheric wavesturbulence, Previous: 3. Tides and

4. Gravity Waves in the Upper Atmosphere

Recognition of the importance of gravity waves for upper atmosphere structures has led to numerous experimental and theoretical efforts. Important experimental tools for the measurement of individual gravity waves and gravity wave spectra include lidar [e.g., Bills and Gardner, 1993; She et al., 1991], radar [e.g., Fritts and VanZandt, 1993], satellite optical observations [ Mende et al., 1994] and all-sky imagery from the ground [e.g., Taylor and Hill, 1991]. Signatures of ``breaking'' gravity waves at mesopause altitudes (90 km) are of particular interest. These waves are generated at lower altitudes due to tropospheric effects, such as the passage of weather fronts and intense pressure regions. The waves propagate upwards and grow in amplitude, until they reach a critical level near the mesopause where they ``break,'' depositing energy and momentum.

Figure 3 [ Fritts et al., 1993] shows a photograph of a noctilucent cloud at 86 km altitude, together with a numerical model calculation of breaking gravity waves near the mesopause. Noctilucent clouds are visible from the ground typically only near twilight during late summer months at high latitudes. The clouds, which provide a screen on which the atmospheric waves in this region can be imaged, often exhibit wave structures that have multiple characteristic scales. The smallest scale waves (meters to kilometers) are thought to be the most important for forcing the mesosphere/lower thermosphere. The ongoing work is motivated by the desire to develop a quantitative description of gravity wave spectra and occurrence frequencies, which will lead to a greater understanding of energy transport and coupling between regions.

Theoretical advances in our understanding of gravity wave production and dissipation have also taken place recently, leading perhaps most significantly to methods for treatment in general circulation codes [ Fritts and Lu, 1993]. Figure 4, taken from the recent review by Gardner [1994] shows a schematic ``m-spectrum'' of gravity waves. Current models for the saturation (dissipation process) include the cascade model of Dewan [1994], the Doppler spreading theory of Hines [1991], the wave-induced diffusion theory of Gardner [1994], and the spectral collocation code of Fritts [1994] and Palmer et al., [1994].



next up previous
Next: 5. Applied Aspects Up: Upper atmospheric wavesturbulence, Previous: 3. Tides and



U.S. National Report to IUGG, 1991-1994
Rev. Geophys. Vol. 33 Suppl., © 1995 American Geophysical Union