It is widely appreciated that ocean mesoscales are filled with predominately westward-drifting sea- surface height (SSH) anomalies. These features are identified typically by closed height contours. They are geostrophically balanced, of spatial scales of O(10- 100) km, long-lived with a typical lifetime over 16 weeks, and are routinely tracked and archived in standard satellite altimeter products. Understanding the properties of these height anomalies is important because they represent a major source of energetic variability. Their drift also has key implications for material transport as their core could trap mass.
Despite the fact that their average zonal drift velocity is close to long Rossby waves, there is good evidence suggesting that these height anomalies are better described as nonlinear vortices, not linear Rossby waves.
Currently, we are investigating whether we could apply/extend force balance theory to understand the drift of these vortices and how they leak mass along their journey.Â
With mean flow (U = long Rossby wave phase speed)
No mean flow