The Inverse Barometer Effect on Antarctic Ice Shelves

Short-term height variations of Antarctic ice shelves must be removed before satellite-derived surface height can be used to assess climate trends, and satellite radar data can be used to determine ice motion. The dominant source of high-frequency vertical motion of ice shelves is their response to tides in the ocean cavities under the shelves. The tide-induced range (low tide to high tide) can exceed 7 m in the southern part of the Ronne Ice Shelf in the Weddell Sea. However, tides are now relatively predictable, and so we now focus on a second source of ice shelf vertical motion, which is due to the response of the underlying ocean to changes in atmospheric pressure (Pair). This response is known as the inverse barometer effect (IBE). Open-ocean measurements of Pair and sea level agree with the theoretical response of ~1 cm per millibar for low frequency variability of Pair. By looking at data from ice shelves, we find that that shelves experience a response of similar magnitude. A simple correction for the IBE is justified for ice shelf response to low-frequency (<0.5 cycles per day) of Pair. At higher frequencies the IBE becomes weaker. The IBE contribution to the ice shelf surface height, hIS, can exceed 50 cm, with typical magnitudes of ~10-20 cm. Although the IBE is usually smaller than the tidal contribution to hIS, the tide can be removed with current Antarctic tide models with an accuracy similar to the IBE. Global atmospheric models, however, do not presently predict Pair with sufficient accuracy to be used to correct measured variability of hIS. Thus, in the absence of concurrent in situ Pair data, the IBE is a major source of error in correcting ice shelf heights for the tasks we mentioned above.

An Example: Amery Ice Shelf

In the figure at below we show: