Abstract Tides on the Ross Ice Shelf observed with
ICESat Laurie Padman
Earth & Space Research, 1910 Fairview Ave. East,
Suite 210, Seattle, WA 98102, USA.
Helen A. Fricker
2Institute of Geophysics and Planetary Physics, Scripps
Institution of Oceanography, University of California, San Diego, La
Jolla, CA 92093-0225, USA.
The Ice, Cloud and land Elevation Satellite (ICESat) provides the first
opportunity for measurement of surface elevation hi
over the portions of the Antarctic ice shelves that are south of the
European Remote Sensing satellite maximum latitude (81.5oS).
The dominant source of short-period variability in hi
is ocean tides. We use crossover elevation difference (Δhi)
data from the Ross Ice Shelf (RIS) to demonstrate ICESat's ability to
detect the tidal signal, and to compare the accuracy of several tide
models. The root-mean-square (rms) value of all RIS measurements of
Δhi is ≈0.74 m; after removing the tide
using the most accurate model, the rms of the residual signal in regions
of optimal model performance is ≈0.16±0.03 m. This value corresponds
to an uncertainty in hi of 0.11 ± 0.02 m. We postulate that the
primary sources of the residual signal are tide model errors and the
inverse barometer effect. |