KH waves are remarkably common in deep stratiform precipitation systems especially in the vicinity of complex terrain, as is evident from transects of vertical velocity and 2D circulation, obtained from an airborne profiling Doppler radar, the Wyoming Cloud Radar. The high resolution of this radar (~30 m) allows detection and depiction of KH waves in fine detail. In this study, airborne Doppler radar data are used to explore the kinematics of KH waves, including the response of thermodynamic and kinematic variables above and below the instability layer. These waves are observed in a variety of wavelengths, depths, amplitudes, and turbulence intensities. KH waves are frequently locked to the terrain, and occur at various heights, including within the free troposphere, at the boundary layer top, and close to the surface. They are observed not only upwind of terrain barriers, as has been documented before, but also in the wake of steep terrain, where the waves can be highly turbulent.
This presentation will first establish the kinematic and dynamic framework of KH waves in orographic clouds, and will then address the question whether the presence of such waves improves seedability, or renders artificial seeding redundant.
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