Brine Movement in Antarctic Sea Ice by Victoria Lytle (Antarctic CRC and Australian Antarctic Division University of Tasmania) JTB 120, 3:20pm Monday, February 23, 1998 Abstract Sea ice around Antarctica undergoes an annual change in area from about 4 million square kilometres in February to 19 million square kilometres in September - one of the largest seasonal changes of surface characteristics on earth. This growth and melt cycle is crucial in the regulation of climate, and may be a driving force behind the biological productivity of the Southern Ocean. The dense, salty brine which is rejected as sea ice grows can cause deep ocean convection, increasing the upwelling of nutrients, and enhancing the global ocean circulation. The snow covered sea ice insulates the relatively warmer ocean from the cold winter atmosphere, reducing heat loss. Compared with open water, snow-covered sea ice reflects much of the incoming solar radiation, and reduces the amount of light available for photosynthesis under the ice. Sea ice is not, however, a simple homogeneous layer; currents, winds and tides constantly deform the ice creating open water with newly forming ice and thicker ridged regions. The ice itself is a multi-phase material, consisting of solid ice, liquid brine, and in some cases air bubbles. In the natural environment, it is found at its melting point, and small changes in temperature will alter the relative percentage of each of these phases. High salinity brine is found in small, vertically elongated pockets and where these pockets link up to form channels, they provide a conduit for the brine. Convection within these brine channels has been well documented in the laboratory and as the brine moves, it transports heat, salt and nutrients. In some cases, the weight of the snow cover can depress the surface of the ice below sea level, allowing sea water to infiltrate the snow, either from the side of the floe, or through this network of brine channels. As this slushy snow mixture freezes, snow ice is formed on the surface of the existing ice cover. Because of the reduced thermal insulation on the surface, this ice can form much quicker than ice growth at the base of the floe. This talk will review recent measurements taken in the sea ice zone around Antarctica which provide evidence of brine movement and its effect on algal blooms, heat fluxes and snow-ice formation. The rate of snow ice formation can be an order of magnitude greater than basal ice growth rates, and may be significantly underestimated in global climate models. Significant ice algal blooms have been found which rely on the supply of nutrients by brine convection. These processes depend on the linkage of the brine pockets, allowing percolation of brine through the ice. Requests for preprints and reprints to: v.lytle@utas.edu.au This source can be found at http://www.math.utah.edu/applied-math/