Antarctic Tides

Laurie Padman and Susan Howard Funded by the NSF and NASA.



Antarctic Tides.  Amplitude (color scale on right) and phase (black lines) for the sea surface elevation amplitude of the semidiurnal M2 tidal constituent.
Why We Study Tides

Barotropic Ocean Tides Models

Baroclinic Ocean Tides Model

Ice Shelf Response to Tides and Atmospheric Pressure Variations

Model Applications

Conference Presentations

Future Work

References

Useful Web Links

Outreach Work: Corvallis High School Antarctica Webpage

AnSlope 1 Cruise Photos


Barotropic tide models and processing packages for the Arctic Ocean and seas surrounding Antarctica are now available for download through our Polar Tides Model page.


Why We Study Tides


Complex interactions between the ocean, atmosphere, sea ice, and floating glacial ice sheets in the Weddell Sea lead to surface waters becoming cooler, saltier, and therefore denser. The dense water sinks, carrying surface-acquired properties such as O2 and CO2 into the deep ocean where they are distributed throughout the world ocean. This process is called "ventilation" and plays a major role in the coupled global ocean and atmosphere. Any modification of the sea ice distribution by oceanic or atmospheric forcing is also relevant to climate modeling because the reflectivity of ice is much greater than open water, thus more ice implies much greater reflection rather than absorption of incoming solar radiation.

The most vigorous cooling and salinization of surface water occur over the continental shelf and under the ice shelves around the perimeter of the Weddell Sea. Many processes help to modify the surface water, and determine the final property of the modified water as it sinks down the continental slope. Tides play a role in this system, both directly and through interactions with other components of the atmosphere-ocean-ice (AOI) environment. Some of the mechanisms that are of interest to us are as follows.

 

  • Tidal currents create turbulent mixing in the ocean, at the seabed, at the base of the ice, and in the stratified ocean interior.
  • Tidal currents modify sea ice properties and distribution by (a) increased upper ocean mixing (mixing brings subsurface warm water up to where it can melt ice) and (b) through the dynamical effect of tide-induced ocean stress on the ice base. This process also modifies the heat exchange rate between the ocean and atmosphere.
  • Tidal stirring under the ice shelves helps to melt the base of the shelves.
  • Tidal strain on the shelf ice helps to create the rifts that eventually form the detachment points for new icebergs.

 

For these reasons, we have been funded to carry out several studies to improve our understanding of the distribution of tidal energy in the Weddell and Scotia Seas, and to investigate the effects of tides on other processes. Our studies to date fall into two categories: improving numerical models that predict tidal energy distribution; and using the models to understand the role of tides in the large-scale circulation of the Weddell Sea and its cover of sea ice. Future funded work includes a detailed study of the interactions of ocean tides with the glacial ice shelves. More information on specific projects can be found by following the links below.



This work is funded by the Office of Polar Programs, National Science Foundation, and by the National Aeronautics and Space Administration.




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Future Work


Subject to funding, the next steps in the model development are to:
  1. couple sea-ice to the barotropic ocean model;
  2. investigate the interactions between the tides and the Filchner-Ronne Ice Shelves; and
  3. work towards a full 3-D baroclinic model, coupled to ice and atmospheric forcing.




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Questions or comments regarding this site may be sent to: Susan Howard
Site last updated on June 2, 2000.