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Submesoscale Eddies, Fronts, and Filaments in collaboration with Jeroen Molemaker (UCLA), Ben Holt (JPL), Carter Ohlmann (UCSB), Svein Vagle (IOS), Geoffrey Smith and George Marmorino (both NRL)
Currently, submesoscale eddies, fronts, and filaments on the scale of 10 m to 20 km represent a scientific frontier in oceanography. They are not very well sampled and have only been recently subject of numerical modeling. These submesoscale features are intermittent in space and time and present a formidable observational challenge. In addition to their role in the energy budget of the large-scale ocean circulation and their connection with local forward energy cascades, they are important for the understanding of mixing processes and the variability of the coastal ocean, also in connection with biogeochemical processes. To date, very little data exists on the physical in situ structure of submesoscale features as well as their biological/optical response and characteristics that truly resolve their very short temporal and spatial scales.
In order to resolve the very short temporal (few hours to days) and spatial time scales (10 m to 10 km) we are using fast and maneuverable vessels and planes. The variables that have to be measured are in situ bulk and skin temperature (representative of density in Southern California), horizontal currents, surfactant concentrations, and meteorological parameters, chlorophyll concentrations, dissolved oxygen, as well as the optical properties of sea water. |
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